4.3. Die trigonometrischen Funktionen


Die trigonometrischen Funktionen spielen nicht nur in der Mathematik selbst, sondern auch in ihren Anwendungsgebieten, speziell in der Physik, eine bedeutende Rolle. Ihre Ursprünge reichen sehr weit zurück und im Gegensatz zu den bisherigen Funktionen liegen ihre Wurzeln deutlich im geometrischen Bereich, und zwar in der Dreieckslehre. Unsere Einführung der trigonometrischen Funktionen trägt zunächst dieser geometrischen Herkunft Rechnung.

Die in der Dreieckslehre übliche Methode, Winkel in Graden zu messen, ist allerdings für unsere Zwecke ungeeignet. Ein geeignetes Maß, Winkel in Zahlen und nicht in Graden zu messen, ist das Bogenmaß (engl. radian). Die Grundidee liegt dabei in der Beobachtung, dass jeder Winkel, im Mittelpunkt eines vorgelegten Kreises angetragen, einen Ausschnitt des Kreisesbogens liefert. Da allerdings ein Winkel bei verschieden großen Kreisen unterschiedliche große Bögen ausschneidet, ist eine Festlegung auf einen bestimmten Kreis zwingend. Zur Winkelmessung durch Bögen werden wir daher stets einen Kreis mit Radius 1 und Mittelpunkt im Ursprung des Koordinatensystems zu Grunde legen, den sog. Einheitskreis.

Jedem gemäß nebenstehender Skizze eingetragenem Winkel α MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdegaaa@3787@ kommt nun neben seinem (orientierten) Gradmaß α° MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdeMaeyiSaalaaa@3973@ auch sein (orientiertes) Bogenmaß α ∩ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySde2aaWbaaSqabeaacqGHPiYXaaaaaa@3952@ (auch: α rad), d.h. die Länge des von ihm ausgeschnittenen Bogens zu. Dabei bezieht sich der Zusatz "orientiert" auf die Vereinbarung, dass im Gegenuhrzeigersinn (wie in der Skizze) eingezeichnete Winkel positive Maßzahlen haben, und Winkeln, die im Uhrzeigersinn eingetragen sind, negative Maßzahlen zukommen.

Natürlich kann man die beiden Maßsysteme ineinander umrechnen. So liefert z.B. ein Winkel vom Gradmaß 180° MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGymaiaaiIdacaaIWaGaeyiSaalaaa@3A0B@ den halben Umfang des Einheitskreises, also die Zahl π MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiWdahaaa@37A5@ als Bogenmaß. Daraus ergibt sich für einen beliebigen Winkel α MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdegaaa@3787@ :

Ist α° MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdeMaeyiSaalaaa@3973@ das Gradmaß von α MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdegaaa@3787@ , so ist α° 180° π MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaWaaSaaaeaacqaHXoqycqGHWcaSaeaacaaIXaGaaGioaiaaicdacqGHWcaSaaGaeqiWdahaaa@3F63@ das Bogenmaß von α MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdegaaa@3787@ .

Ist α ∩ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySde2aaWbaaSqabeaacqGHPiYXaaaaaa@3952@ das Bogenmaß von α MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdegaaa@3787@ , so ist α ∩ π 180° MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaWaaSaaaeaacqaHXoqydaahaaWcbeqaaiabgMIihdaaaOqaaiabec8aWbaacaaIXaGaaGioaiaaicdacqGHWcaSaaa@3F4C@ das Gradmaß von α MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdegaaa@3787@ .

Grad- und Bogenmaße einiger markanter Winkel kann man direkt aus der folgenden Tabelle ablesen. Für beliebige Winkel leistet das nachstehende Umrechnungsformular gute Dienste. Es berücksichtigt bis zu 8 Dezimalstellen.

α° 0° 30° 45° 60° 90° 180° 270° 360° 450° 720° −90° −180° −270° −360° α ∩ 0 π 6 π 4 π 3 π 2 π 3 π 2 2π 5 π 2 4π − π 2 −π −3 π 2 −2π MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=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@9B71@
α° MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySdeMaeyiSaalaaa@3973@   α ∩ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqySde2aaWbaaSqabeaacqGHPiYXaaaaaa@3952@
 

Nun können wir die beiden ersten trigonometrischen Funktionen, nämlich die Sinus- und die Cosinusfunktion

sin⁡,cos⁡:ℝ→ℝ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGaaiilaiGacogacaGGVbGaai4CaiaacQdacqWIDesOcqGHsgIRcqWIDesOaaa@41CE@

einführen. Statt einer präzisen Funktionsvorschrift geben wir hier eine geometrisch ausgerichtete Konstruktionsvorschrift an und tragen die exakte Definition in einem späteren Abschnitt

 i

In [5.9] setzen wir sin⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGaamiEaaaa@39BD@ , bzw. cos⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGGZbGaamiEaaaa@39B8@ als Grenzwert einer konvergenten Potenzreihe fest, und zwar

sin⁡x= ∑ i=0 ∞ (−1) i x 2i+1 (2i+1)! cos⁡x= ∑ i=0 ∞ (−1) i x 2i (2i)! MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=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@6523@

Da diese Definition auch im Komplexen möglich ist, liegen Sinus und Cosinus auch als Funktionen von ℂ→ℂ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeSOaHmQaeyOKH4QaeSOaHmkaaa@3A83@ vor. Darüber hinaus sind wir erst mit dieser analytischen Definition in der Lage, exakte Beweise zu führen.

nach. Eine gegebene reelle Zahl x∈ℝ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiEaiabgIGiolabl2riHcaa@39D9@ interpretieren wir als das Bogenmaß eines Winkels und tragen dieses Maß am Einheitskreis ab (positive Zahlen im Gegenuhrzeigersinn, negative im Uhrzeigersinn). Dadurch legen wir eindeutig einen von x abhängigen Punkt (a,b) MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikaiaadggacaGGSaGaamOyaiaacMcaaaa@39BE@ auf dem Kreis fest. Seine beiden Koordinaten a und b sind nun die Funktionswerte.

Definition:  Für x∈ℝ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiEaiabgIGiolabl2riHcaa@39D9@ setzen wir gemäß der vorgestellten Konstruktion fest:

cos⁡(x)≔a sin⁡(x)≔b MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqbaeaabiqaaaqaaiGacogacaGGVbGaai4CaiaacIcacaWG4bGaaiykaiabg2da9iaadggaaeaaciGGZbGaaiyAaiaac6gacaGGOaGaamiEaiaacMcacqGH9aqpcaWGIbaaaaaa@4424@
[4.3.1]

Es ist üblich, die Funktionswerte klammerfrei zu schreiben, also: sin⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGaamiEaaaa@39BD@ bzw. cos⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGGZbGaamiEaaaa@39B8@ .

Im allgemeinen wird man mit dieser Methode keine exakten Funktionswerte ermitteln können, für einige speziell gewählte x-Werte lassen sich sin⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGaamiEaaaa@39BD@ und cos⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGGZbGaamiEaaaa@39B8@ jedoch leicht am Einheitskreis ablesen:

x 0 π 2 π 3 π 2 2π − π 2 −π sin⁡x 0 1 0 −1 0 −1 0 cos⁡x 1 0 −1 0 1 0 −1 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqbaeqabmacaaaaaeaacaWG4baabaGaaGimaaqaamaalaaabaGaeqiWdahabaGaaGOmaaaaaeaacqaHapaCaeaacaaIZaWaaSaaaeaacqaHapaCaeaacaaIYaaaaaqaaiaaikdacqaHapaCaeaacqGHsisldaWcaaqaaiabec8aWbqaaiaaikdaaaaabaGaeyOeI0IaeqiWdahabaGaci4CaiaacMgacaGGUbGaamiEaaqaaiaaicdaaeaacaaIXaaabaGaaGimaaqaaiabgkHiTiaaigdaaeaacaaIWaaabaGaeyOeI0IaaGymaaqaaiaaicdaaeaaciGGJbGaai4BaiaacohacaWG4baabaGaaGymaaqaaiaaicdaaeaacqGHsislcaaIXaaabaGaaGimaaqaaiaaigdaaeaacaaIWaaabaGaeyOeI0IaaGymaaaaaaa@5D7B@

Wir erläutern das Ablesen an zwei Beispielen:

  • Der zu x= π 2 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiEaiabg2da9maalaaabaGaeqiWdahabaGaaGOmaaaaaaa@3A74@ gehörige Bogen ist ein Viertelkreis, der bei (1,0) MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikaiaaigdacaGGSaGaaGimaiaacMcaaaa@3966@ startet und bei (0,1) MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikaiaaicdacaGGSaGaaGymaiaacMcaaaa@3966@ endet. Die Koordinaten des Endpunkts sind die sin- bzw. cos-Werte: 1 ist der Sinuswert und 0 der Cosinuswert.

  • Zu x=0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiEaiabg2da9iaaicdaaaa@38A5@ gehört ein Bogen der Länge 0. Er endet also bereits im Startpunkt (1,0) MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikaiaaigdacaGGSaGaaGimaiaacMcaaaa@3966@ , d.h. der Sinuswert ist hier 0 und der Cosinuswert 1.

Um einen Funktionsgraphen zu zeichnen, reichen diese Daten allein natürlich nicht aus. Das folgende Applet simuliert jedoch die geometrische Konstruktion für die Sinusfunktion und stellt ausreichend viele Werte zur Verfügung. Mit dem Schieber kann man den Graphen bequem erzeugen.

sin und cos besitzen eine Fülle von Eigenschaften. Viele ergeben sich zwar direkt aus der Konstruktion über den Einheitskreis, ihre Gültigkeit aber können wir damit nicht sicherstellen. Für die weiteren Ausführungen legen wir daher die Definition aus [5.9] zu Grunde, also:

sin⁡x= ∑ i=0 ∞ (−1) i x 2i+1 (2i+1)! cos⁡x= ∑ i=0 ∞ (−1) i x 2i (2i)! MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqbaeaabiqaaaqaaiGacohacaGGPbGaaiOBaiaadIhacqGH9aqpdaaeWbqaaiaacIcacqGHsislcaaIXaGaaiykamaaCaaaleqabaGaamyAaaaakmaalaaabaGaamiEamaaCaaaleqabaGaaGOmaiaadMgacqGHRaWkcaaIXaaaaaGcbaGaaiikaiaaikdacaWGPbGaey4kaSIaaGymaiaacMcacaGGHaaaaaWcbaGaamyAaiabg2da9iaaicdaaeaacqGHEisPa0GaeyyeIuoaaOqaaiGacogacaGGVbGaai4CaiaadIhacqGH9aqpdaaeWbqaaiaacIcacqGHsislcaaIXaGaaiykamaaCaaaleqabaGaamyAaaaakmaalaaabaGaamiEamaaCaaaleqabaGaaGOmaiaadMgaaaaakeaacaGGOaGaaGOmaiaadMgacaGGPaGaaiyiaaaaaSqaaiaadMgacqGH9aqpcaaIWaaabaGaeyOhIukaniabggHiLdaaaaaa@6523@ [0]

Da durch [0] auch die komplexen Funktionen sin und cos definiert sind, hat dies zudem den Vorteil, dass (fast) jede der hier notierten Aussagen automatisch auch im Komplexen gültig ist.

Allerdings müssen wir erst sicherstellen, dass die durch [0] definierten Funktionen mit den geometrisch eingeführten identisch sind! Wir zeigen dies mit Techniken der Integralrechnung auf einer eigenen Seite. Ferner benötigen wir genauere Informationen über die Zahl π MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiWdahaaa@37A5@ . Dazu vergewissern wir uns zunächst, dass die Sinusfunktion positive Nullstellen besitzt.

Bemerkung:  Es gibt eine reelle Zahl x>0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiEaiabg6da+iaaicdaaaa@38A7@ , so dass

sin⁡x=0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGaamiEaiabg2da9iaaicdaaaa@3B7D@
[4.3.2]

Beweis:  Wir benötigen einige Abschätzungen. Zunächst hat man für i≥1 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamyAaiabgwMiZkaaigdaaaa@3957@ und 0<x< 6 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGimaiabgYda8iaadIhacqGH8aapdaGcaaqaaiaaiAdaaSqabaaaaa@3A82@ :

(−1) 2i x 4i+1 (4i+1)! + (−1) 2i+1 x 4i+3 (4i+3)! = x 4i+1 (4i+1)! (1− x 2 (4i+2)(4i+3) ) = x 4i+1 (4i+1)! ⋅ 16 i 2 +20i+6− x 2 (4i+2)(4i+3) > x 4i+1 (4i+1)! ⋅ 16 i 2 +20i+6−6 (4i+2)(4i+3) >0. MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=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@B2DA@

Für diese x gilt daher:

sin⁡x=x− x 3 6 + ∑ i=2 ∞ (−1) i x 2i+1 (2i+1)! =x− x 3 6 + ∑ i=1 ∞ (−1) 2i x 4i+1 (4i+1)! + (−1) 2i+1 x 4i+3 (4i+3)! ︸ >0 ≥x− x 3 6 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=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@8BD4@ ,

und damit schließlich:

sin⁡x≥x− x 3 6 = 1 6 x(6− x 2 )>0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGaamiEaiabgwMiZkaadIhacqGHsisldaWcaaqaaiaadIhadaahaaWcbeqaaiaaiodaaaaakeaacaaI2aaaaiabg2da9maalaaabaGaaGymaaqaaiaaiAdaaaGaamiEaiaacIcacaaI2aGaeyOeI0IaamiEamaaCaaaleqabaGaaGOmaaaakiaacMcacqGH+aGpcaaIWaaaaa@4A74@   für alle 0<x< 6 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGimaiabgYda8iaadIhacqGH8aapdaGcaaqaaiaaiAdaaSqabaaaaa@3A82@ .[+]

Somit ist z.B. sin⁡2>0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGaaGOmaiabg6da+iaaicdaaaa@3B3E@ und mit einer weiteren Abschätzung finden wir:

sin⁡4 = ∑ i=0 ∞ (−1) i 4 2i+1 (2i+1)! = ∑ i=0 4 (−1) i 4 2i+1 (2i+1)! + ∑ i=0 ∞ (−1) i+5 4 2i+11 (2i+11)! = ∑ i=0 4 (−1) i 4 2i+1 (2i+1)! + ∑ i=0 ∞ (−1) 2i+5 4 4i+11 (4i+11)! + (−1) 2i+6 4 4i+13 (4i+13)! =− 268 405 + ∑ i=0 ∞ 4 4i+11 4 2 −(4i+12)(4i+13) (4i+13)! ︸ ≤0 ≤− 268 405 <0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=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@EE91@

Da sin stetig ist ([6.2.17]), gibt es gemäß Nullstellensatz [6.6.1] eine Nullstelle zwischen 2 und 4.

In ℝ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeSyhHekaaa@3758@ gilt das Vollständigkeitsaxiom, d.h. jede nicht-leere, nach unten beschränkte Teilmenge besitzt eine größte untere Schranke, das Infimum. Mit [4.3.2] können wir daher festsetzen:

π≔inf⁡{x>0|sin⁡x=0} MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiWdaNaeyypa0JaciyAaiaac6gacaGGMbGaai4EaiaadIhacqGH+aGpcaaIWaGaaiiFaiGacohacaGGPbGaaiOBaiaadIhacqGH9aqpcaaIWaGaaiyFaaaa@46CA@
[4.3.3]

Dabei garantieren [+] und die letzte Abschätzung dass 6 ≤π≤4 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaWaaOaaaeaacaaI2aaaleqaaOGaeyizImQaeqiWdaNaeyizImQaaGinaaaa@3CB2@ . Insbesondere ist damit π>0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiWdaNaeyOpa4JaaGimaaaa@3967@ .

Von entscheidender Bedeutung für die Eigenschaften der trigonometrischen Funktionen sind die sog. Additionstheoreme.

Satz (Additionstheoreme):  Für alle x,y∈ℝ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiEaiaacYcacaWG5bGaeyicI4SaeSyhHekaaa@3B87@ ist

  1. sin⁡(x+y)=sin⁡x⋅cos⁡y+sin⁡y⋅cos⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGaaiikaiaadIhacqGHRaWkcaWG5bGaaiykaiabg2da9iGacohacaGGPbGaaiOBaiaadIhacqGHflY1ciGGJbGaai4BaiaacohacaWG5bGaey4kaSIaci4CaiaacMgacaGGUbGaamyEaiabgwSixlGacogacaGGVbGaai4CaiaadIhaaaa@52BE@

  2. cos⁡(x+y)=cos⁡x⋅cos⁡y−sin⁡x⋅sin⁡y MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGGZbGaaiikaiaadIhacqGHRaWkcaWG5bGaaiykaiabg2da9iGacogacaGGVbGaai4CaiaadIhacqGHflY1ciGGJbGaai4BaiaacohacaWG5bGaeyOeI0Iaci4CaiaacMgacaGGUbGaamiEaiabgwSixlGacohacaGGPbGaaiOBaiaadMhaaaa@52C4@

[4.3.4]

Beweis:  Mit den Abkürzungen

a i ≔{ (−1) i−1 2 i!   falls i ungerade  0  falls i gerade  MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamyyamaaBaaaleaacaWGPbaabeaakiabg2da9maaceaabaqbaeqabiqaaaqaamaalaaabaGaaiikaiabgkHiTiaaigdacaGGPaWaaWbaaSqabeaadaWcaaqaaiaadMgacqGHsislcaaIXaaabaGaaGOmaaaaaaaakeaacaWGPbGaaiyiaaaacaqGMbGaaeyyaiaabYgacaqGSbGaae4CaiaadMgacaqG1bGaaeOBaiaabEgacaqGLbGaaeOCaiaabggacaqGKbGaaeyzaaqaaiaaicdacaqGMbGaaeyyaiaabYgacaqGSbGaae4CaiaadMgacaqGNbGaaeyzaiaabkhacaqGHbGaaeizaiaabwgaaaaacaGL7baaaaa@5B11@   und   b i ≔{ (−1) i 2 i!   falls i gerade  0  falls i ungerade  MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOyamaaBaaaleaacaWGPbaabeaakiabg2da9maaceaabaqbaeqabiqaaaqaamaalaaabaGaaiikaiabgkHiTiaaigdacaGGPaWaaWbaaSqabeaadaWcaaqaaiaadMgaaeaacaaIYaaaaaaaaOqaaiaadMgacaGGHaaaaiaabAgacaqGHbGaaeiBaiaabYgacaqGZbGaamyAaiaabEgacaqGLbGaaeOCaiaabggacaqGKbGaaeyzaaqaaiaaicdacaqGMbGaaeyyaiaabYgacaqGSbGaae4CaiaadMgacaqG1bGaaeOBaiaabEgacaqGLbGaaeOCaiaabggacaqGKbGaaeyzaaaaaiaawUhaaaaa@596A@

können wir [0] umschreiben zu

sin⁡x= ∑ i=0 ∞ (−1) i x 2i+1 (2i+1)! = ∑ i=0 ∞ a i x i cos⁡x= ∑ i=0 ∞ (−1) i x 2i (2i)! = ∑ i=0 ∞ b i x i MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqbaeaabiqaaaqaaiGacohacaGGPbGaaiOBaiaadIhacqGH9aqpdaaeWbqaaiaacIcacqGHsislcaaIXaGaaiykamaaCaaaleqabaGaamyAaaaakmaalaaabaGaamiEamaaCaaaleqabaGaaGOmaiaadMgacqGHRaWkcaaIXaaaaaGcbaGaaiikaiaaikdacaWGPbGaey4kaSIaaGymaiaacMcacaGGHaaaaaWcbaGaamyAaiabg2da9iaaicdaaeaacqGHEisPa0GaeyyeIuoakiabg2da9maaqahabaGaamyyamaaBaaaleaacaWGPbaabeaakiaadIhadaahaaWcbeqaaiaadMgaaaaabaGaamyAaiabg2da9iaaicdaaeaacqGHEisPa0GaeyyeIuoaaOqaaiGacogacaGGVbGaai4CaiaadIhacqGH9aqpdaaeWbqaaiaacIcacqGHsislcaaIXaGaaiykamaaCaaaleqabaGaamyAaaaakmaalaaabaGaamiEamaaCaaaleqabaGaaGOmaiaadMgaaaaakeaacaGGOaGaaGOmaiaadMgacaGGPaGaaiyiaaaaaSqaaiaadMgacqGH9aqpcaaIWaaabaGaeyOhIukaniabggHiLdGccqGH9aqpdaaeWbqaaiaadkgadaWgaaWcbaGaamyAaaqabaGccaWG4bWaaWbaaSqabeaacaWGPbaaaaqaaiaadMgacqGH9aqpcaaIWaaabaGaeyOhIukaniabggHiLdaaaaaa@7C34@ [1]

Wir beweisen jetzt das Additionstheorem für den Sinus. Der Nachweis für den Cosinus verläuft ähnlich und kann hier aufgerufen werden.

Wir berechnen nun zunächst für 0≤k≤i MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGimaiabgsMiJkaadUgacqGHKjYOcaWGPbaaaa@3BEA@ :

a k b i−k + b k a i−k ={ (−1) k−1 2 k! ⋅ (−1) i−k 2 (i−k)!   falls k unger.,i−k gerade (−1) k 2 k! ⋅ (−1) i−k−1 2 (i−k)!   falls k gerade,i−k unger. 0  sonst ={ (−1) i−1 2 k!(i−k)!   falls i unger. 0  sonst MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=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@C441@

Man beachte dabei:   k ungerade,i−k gerade   ∨   k gerade,i−k ungerade ⇔ i ungerade MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaam4AaiaabwhacaqGUbGaae4zaiaabwgacaqGYbGaaeyyaiaabsgacaqGLbGaaiilaiaadMgacqGHsislcaWGRbGaae4zaiaabwgacaqGYbGaaeyyaiaabsgacaqGLbGaaGjbVlabgIIiAlaaysW7caWGRbGaae4zaiaabwgacaqGYbGaaeyyaiaabsgacaqGLbGaaiilaiaadMgacqGHsislcaWGRbGaaeyDaiaab6gacaqGNbGaaeyzaiaabkhacaqGHbGaaeizaiaabwgacaaMf8Uaeyi1HSTaaGzbVlaadMgacaqG1bGaaeOBaiaabEgacaqGLbGaaeOCaiaabggacaqGKbGaaeyzaaaa@6B0B@ .

Mit Hilfe des Binomialtheorems [5.2.5] und der Produktregel für konvergente Reihen

 i

∑ i=0 ∞ a i ⋅ ∑ i=0 ∞ b i = ∑ i=0 ∞ ∑ k=0 i a k ⋅ b i−k MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaWaaabCaeaacaWGHbWaaSbaaSqaaiaadMgaaeqaaaqaaiaadMgacqGH9aqpcaaIWaaabaGaeyOhIukaniabggHiLdGccqGHflY1daaeWbqaaiaadkgadaWgaaWcbaGaamyAaaqabaaabaGaamyAaiabg2da9iaaicdaaeaacqGHEisPa0GaeyyeIuoakiabg2da9maaqahabaWaaabCaeaacaWGHbWaaSbaaSqaaiaadUgaaeqaaOGaeyyXICTaamOyamaaBaaaleaacaWGPbGaeyOeI0Iaam4AaaqabaaabaGaam4Aaiabg2da9iaaicdaaeaacaWGPbaaniabggHiLdaaleaacaWGPbGaeyypa0JaaGimaaqaaiabg6HiLcqdcqGHris5aaaa@5E63@
haben wir jetzt:

sin⁡x⋅cos⁡y+sin⁡y⋅cos⁡x = ∑ i=0 ∞ a i x i ⋅ ∑ i=0 ∞ b i y i + ∑ i=0 ∞ b i x i ⋅ ∑ i=0 ∞ a i y i = ∑ i=0 ∞ ∑ k=0 i ( a k b i−k + b k a i−k ) x k y i−k = ∑ i=0 ∞ ∑ k=0 i { (−1) i−1 2 i!   falls i ungerade 0  falls i gerade } i! k!(i−k)! x k y i−k = ∑ i=0 ∞ a i ∑ k=0 i (T i k )T x k y i−k = ∑ i=0 ∞ a i (x+y) i = sin⁡(x+y). MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=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@0AE6@

Wir stellen nun weitere Eigenschaften der trigonometrischen Funktionen zusammen und beginnen mit einer Information zur Symmetrie: sin ist punkt- und cos achsensymmetrisch.

Bemerkung:  Für alle x∈ℝ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiEaiabgIGiolabl2riHcaa@39D9@ ist

  1. sin⁡(−x)=−sin⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGaaiikaiabgkHiTiaadIhacaGGPaGaeyypa0JaeyOeI0Iaci4CaiaacMgacaGGUbGaamiEaaaa@41CB@

  2. cos⁡(−x)=cos⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGGZbGaaiikaiabgkHiTiaadIhacaGGPaGaeyypa0Jaci4yaiaac+gacaGGZbGaamiEaaaa@40D4@

[4.3.5]

Beweis:

1. ►   sin⁡(−x)= ∑ i=0 ∞ (−1) i (−x) 2i+1 (2i+1)! = ∑ i=0 ∞ (−1) i − x 2i+1 (2i+1)! =− ∑ i=0 ∞ (−1) i x 2i+1 (2i+1)! =−sin⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=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@8620@ .

2. ►   cos⁡(−x)= ∑ i=0 ∞ (−1) i (−x) 2i (2i)! = ∑ i=0 ∞ (−1) i x 2i (2i)! =cos⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=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@6774@ .

Nun gelingt es auch, einige der anschaulich gewonnenen Funktionswerte rechnerisch zu bestätigen.

Bemerkung:  

sin⁡0=0 cos⁡0=1 sin⁡ π 2 =1 cos⁡ π 2 =0 sin⁡π=0 cos⁡π=−1 sin⁡3 π 2 =−1 cos⁡3 π 2 =0 sin⁡2π=0 cos⁡2π=1 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=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@7B34@
[4.3.6]

Beweis:  

  • Da 0 n MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGimamaaCaaaleqabaGaamOBaaaaaaa@37C2@ ist gleich 0 für n>0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOBaiabg6da+iaaicdaaaa@389D@ und gleich 1 für n=0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOBaiabg2da9iaaicdaaaa@389B@ hat man sofort:

    sin⁡0= ∑ i=0 ∞ (−1) i 0 2i+1 (2i+1)! =0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGaaGimaiabg2da9maaqahabaGaaiikaiabgkHiTiaaigdacaGGPaWaaWbaaSqabeaacaWGPbaaaOWaaSaaaeaacaaIWaWaaWbaaSqabeaacaaIYaGaamyAaiabgUcaRiaaigdaaaaakeaacaGGOaGaaGOmaiaadMgacqGHRaWkcaaIXaGaaiykaiaacgcaaaaaleaacaWGPbGaeyypa0JaaGimaaqaaiabg6HiLcqdcqGHris5aOGaeyypa0JaaGimaaaa@505E@   und   cos⁡0= ∑ i=0 ∞ (−1) i 0 2i (2i)! = (−1) 0 0 0 0! =1 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGGZbGaaGimaiabg2da9maaqahabaGaaiikaiabgkHiTiaaigdacaGGPaWaaWbaaSqabeaacaWGPbaaaOWaaSaaaeaacaaIWaWaaWbaaSqabeaacaaIYaGaamyAaaaaaOqaaiaacIcacaaIYaGaamyAaiaacMcacaGGHaaaaaWcbaGaamyAaiabg2da9iaaicdaaeaacqGHEisPa0GaeyyeIuoakiabg2da9iaacIcacqGHsislcaaIXaGaaiykamaaCaaaleqabaGaaGimaaaakmaalaaabaGaaGimamaaCaaaleqabaGaaGimaaaaaOqaaiaaicdacaGGHaaaaiabg2da9iaaigdaaaa@5532@ .
     
  • sin⁡π=0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGaeqiWdaNaeyypa0JaaGimaaaa@3C3D@ :  Gemäß [4.3.3] kann es unterhalb von π MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiWdahaaa@37A5@ keine positiven Nullstellen des Sinus geben, also ist sin⁡x≠0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGaamiEaiabgcMi5kaaicdaaaa@3C3E@ für alle 0<x<π MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGimaiabgYda8iaadIhacqGH8aapcqaHapaCaaa@3B64@ . Ist nun sin⁡π≠0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGaeqiWdaNaeyiyIKRaaGimaaaa@3CFE@ , so gilt dies aus Stetigkeitsgründen in ganzen Umgebung von π MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiWdahaaa@37A5@ . Es gibt also ein ε>0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqyTduMaeyOpa4JaaGimaaaa@3951@ , o.E. ε<π MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqyTduMaeyipaWJaeqiWdahaaa@3A50@ , so dass sin⁡x≠0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGaamiEaiabgcMi5kaaicdaaaa@3C3E@ in ]π−ε,π+ε[ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiyxaiabec8aWjabgkHiTiabew7aLjaacYcacqaHapaCcqGHRaWkcqaH1oqzcaGGBbaaaa@40EF@ . Damit aber hat man

    sin⁡x≠0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGaamiEaiabgcMi5kaaicdaaaa@3C3E@ für alle 0<x<π+ε MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGimaiabgYda8iaadIhacqGH8aapcqaHapaCcqGHRaWkcqaH1oqzaaa@3DED@

    und folglich: π+ε≤π MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiWdaNaey4kaSIaeqyTduMaeyizImQaeqiWdahaaa@3DA0@ - Widerspruch.

  • cos⁡ π 2 =0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGGZbWaaSaaaeaacqaHapaCaeaacaaIYaaaaiabg2da9iaaicdaaaa@3D04@ :  Mit dem Additionstheorem für den Sinus erhält man

    0=sin⁡π=sin⁡( π 2 + π 2 )=sin⁡ π 2 ⋅cos⁡ π 2 +sin⁡ π 2 ⋅cos⁡ π 2 =2 sin⁡ π 2 ︸ ≠0 ⋅cos⁡ π 2 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGimaiabg2da9iGacohacaGGPbGaaiOBaiabec8aWjabg2da9iGacohacaGGPbGaaiOBaiaacIcadaWcaaqaaiabec8aWbqaaiaaikdaaaGaey4kaSYaaSaaaeaacqaHapaCaeaacaaIYaaaaiaacMcacqGH9aqpciGGZbGaaiyAaiaac6gadaWcaaqaaiabec8aWbqaaiaaikdaaaGaeyyXICTaci4yaiaac+gacaGGZbWaaSaaaeaacqaHapaCaeaacaaIYaaaaiabgUcaRiGacohacaGGPbGaaiOBamaalaaabaGaeqiWdahabaGaaGOmaaaacqGHflY1ciGGJbGaai4BaiaacohadaWcaaqaaiabec8aWbqaaiaaikdaaaGaeyypa0JaaGOmamaayaaabaGaci4CaiaacMgacaGGUbWaaSaaaeaacqaHapaCaeaacaaIYaaaaaWcbaGaeyiyIKRaaGimaaGccaGL44pacqGHflY1ciGGJbGaai4BaiaacohadaWcaaqaaiabec8aWbqaaiaaikdaaaaaaa@76A8@ .

    Man beachte, dass sin⁡ π 2 ≠0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbWaaSaaaeaacqaHapaCaeaacaaIYaaaaiabgcMi5kaaicdaaaa@3DCA@ , da 0< π 2 <π MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGimaiabgYda8maalaaabaGaeqiWdahabaGaaGOmaaaacqGH8aapcqaHapaCaaa@3CF0@ (siehe [4.3.3]). Also ist cos⁡ π 2 =0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGGZbWaaSaaaeaacqaHapaCaeaacaaIYaaaaiabg2da9iaaicdaaaa@3D04@ .

  • sin⁡ π 2 =1 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbWaaSaaaeaacqaHapaCaeaacaaIYaaaaiabg2da9iaaigdaaaa@3D0A@ :  Diesmal setzen wir das Additionstheorem für den Cosinus ein und erhalten unter Beachtung der Symmetrie [4.3.5]:

    1=cos⁡( π 2 − π 2 )= (cos⁡ π 2 ) 2 + (sin⁡ π 2 ) 2 = (sin⁡ π 2 ) 2 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGymaiabg2da9iGacogacaGGVbGaai4CaiaacIcadaWcaaqaaiabec8aWbqaaiaaikdaaaGaeyOeI0YaaSaaaeaacqaHapaCaeaacaaIYaaaaiaacMcacqGH9aqpcaGGOaGaci4yaiaac+gacaGGZbWaaSaaaeaacqaHapaCaeaacaaIYaaaaiaacMcadaahaaWcbeqaaiaaikdaaaGccqGHRaWkcaGGOaGaci4CaiaacMgacaGGUbWaaSaaaeaacqaHapaCaeaacaaIYaaaaiaacMcadaahaaWcbeqaaiaaikdaaaGccqGH9aqpcaGGOaGaci4CaiaacMgacaGGUbWaaSaaaeaacqaHapaCaeaacaaIYaaaaiaacMcadaahaaWcbeqaaiaaikdaaaaaaa@5BBA@ ,

    also |sin⁡ π 2 |=1 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiiFaiGacohacaGGPbGaaiOBamaalaaabaGaeqiWdahabaGaaGOmaaaacaGG8bGaeyypa0JaaGymaaaa@3F0A@ . Das aber ist nach [+] die Behauptung, denn da π≤4 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiWdaNaeyizImQaaGinaaaa@3A18@ , ist 0< π 2 ≤2< 6 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGimaiabgYda8maalaaabaGaeqiWdahabaGaaGOmaaaacqGHKjYOcaaIYaGaeyipaWZaaOaaaeaacaaI2aaaleqaaaaa@3E7F@ .

  • cos⁡π=−1 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGGZbGaeqiWdaNaeyypa0JaeyOeI0IaaGymaaaa@3D26@ :  Wir greifen auf die beiden letzten Ergebnisse und das Additionstheorem zurück:

    cos⁡π=cos⁡( π 2 + π 2 )= (cos⁡ π 2 ) 2 − (sin⁡ π 2 ) 2 =−1 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGGZbGaeqiWdaNaeyypa0Jaci4yaiaac+gacaGGZbGaaiikamaalaaabaGaeqiWdahabaGaaGOmaaaacqGHRaWkdaWcaaqaaiabec8aWbqaaiaaikdaaaGaaiykaiabg2da9iaacIcaciGGJbGaai4BaiaacohadaWcaaqaaiabec8aWbqaaiaaikdaaaGaaiykamaaCaaaleqabaGaaGOmaaaakiabgkHiTiaacIcaciGGZbGaaiyAaiaac6gadaWcaaqaaiabec8aWbqaaiaaikdaaaGaaiykamaaCaaaleqabaGaaGOmaaaakiabg2da9iabgkHiTiaaigdaaaa@5994@ .
     
  • sin⁡3 π 2 =−1 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGaaG4mamaalaaabaGaeqiWdahabaGaaGOmaaaacqGH9aqpcqGHsislcaaIXaaaaa@3EB4@ :   sin⁡3 π 2 =sin⁡(π+ π 2 )=sin⁡π⋅cos⁡ π 2 +sin⁡ π 2 ⋅cos⁡π=0⋅0+1⋅(−1)=−1 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGaaG4mamaalaaabaGaeqiWdahabaGaaGOmaaaacqGH9aqpciGGZbGaaiyAaiaac6gacaGGOaGaeqiWdaNaey4kaSYaaSaaaeaacqaHapaCaeaacaaIYaaaaiaacMcacqGH9aqpciGGZbGaaiyAaiaac6gacqaHapaCcqGHflY1ciGGJbGaai4BaiaacohadaWcaaqaaiabec8aWbqaaiaaikdaaaGaey4kaSIaci4CaiaacMgacaGGUbWaaSaaaeaacqaHapaCaeaacaaIYaaaaiabgwSixlGacogacaGGVbGaai4Caiabec8aWjabg2da9iaaicdacqGHflY1caaIWaGaey4kaSIaaGymaiabgwSixlaacIcacqGHsislcaaIXaGaaiykaiabg2da9iabgkHiTiaaigdaaaa@6F1D@ .

  • cos⁡3 π 2 =0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGGZbGaaG4mamaalaaabaGaeqiWdahabaGaaGOmaaaacqGH9aqpcaaIWaaaaa@3DC1@ :   cos⁡3 π 2 =cos⁡(π+ π 2 )=cos⁡π⋅cos⁡ π 2 −sin⁡ π 2 ⋅sin⁡π=(−1)⋅0−1⋅0=0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGGZbGaaG4mamaalaaabaGaeqiWdahabaGaaGOmaaaacqGH9aqpciGGJbGaai4BaiaacohacaGGOaGaeqiWdaNaey4kaSYaaSaaaeaacqaHapaCaeaacaaIYaaaaiaacMcacqGH9aqpciGGJbGaai4BaiaacohacqaHapaCcqGHflY1ciGGJbGaai4BaiaacohadaWcaaqaaiabec8aWbqaaiaaikdaaaGaeyOeI0Iaci4CaiaacMgacaGGUbWaaSaaaeaacqaHapaCaeaacaaIYaaaaiabgwSixlGacohacaGGPbGaaiOBaiabec8aWjabg2da9iaacIcacqGHsislcaaIXaGaaiykaiabgwSixlaaicdacqGHsislcaaIXaGaeyyXICTaaGimaiabg2da9iaaicdaaaa@6E3B@ .

  • sin⁡2π=0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGaaGOmaiabec8aWjabg2da9iaaicdaaaa@3CF9@ :   sin⁡2π=sin⁡(π+π)=2sin⁡π⋅cos⁡π=2⋅0⋅(−1)=0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGaaGOmaiabec8aWjabg2da9iGacohacaGGPbGaaiOBaiaacIcacqaHapaCcqGHRaWkcqaHapaCcaGGPaGaeyypa0JaaGOmaiGacohacaGGPbGaaiOBaiabec8aWjabgwSixlGacogacaGGVbGaai4Caiabec8aWjabg2da9iaaikdacqGHflY1caaIWaGaeyyXICTaaiikaiabgkHiTiaaigdacaGGPaGaeyypa0JaaGimaaaa@5DCE@ .

  • cos⁡2π=1 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGGZbGaaGOmaiabec8aWjabg2da9iaaigdaaaa@3CF5@ :   cos⁡2π=cos⁡(π+π)= (cos⁡π) 2 − (sin⁡π) 2 =1−0=1 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGGZbGaaGOmaiabec8aWjabg2da9iGacogacaGGVbGaai4CaiaacIcacqaHapaCcqGHRaWkcqaHapaCcaGGPaGaeyypa0JaaiikaiGacogacaGGVbGaai4Caiabec8aWjaacMcadaahaaWcbeqaaiaaikdaaaGccqGHsislcaGGOaGaci4CaiaacMgacaGGUbGaeqiWdaNaaiykamaaCaaaleqabaGaaGOmaaaakiabg2da9iaaigdacqGHsislcaaIWaGaeyypa0JaaGymaaaa@599B@ .

Da nun einige markante Funktionswerte sicher sind, lassen sich weitere Eigenschaften nachweisen. Wir haben u.a. eine zusätzliche Notiz zur Symmetrie, zur Periodizität und zum Nullstellenverhalten.

Bemerkung:  Für alle x∈ℝ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiEaiabgIGiolabl2riHcaa@39D9@ gilt:

  1. sin⁡(x+ π 2 )=cos⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGaaiikaiaadIhacqGHRaWkdaWcaaqaaiabec8aWbqaaiaaikdaaaGaaiykaiabg2da9iGacogacaGGVbGaai4CaiaadIhaaaa@4357@
    cos⁡(x− π 2 )=sin⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGGZbGaaiikaiaadIhacqGHsisldaWcaaqaaiabec8aWbqaaiaaikdaaaGaaiykaiabg2da9iGacohacaGGPbGaaiOBaiaadIhaaaa@4362@

[4.3.7]

sin und cos lassen sich durch waagerechtes Verschieben in die jeweils andere Funktion überführen: Verschiebt man sin um − π 2 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeyOeI0YaaSaaaeaacqaHapaCaeaacaaIYaaaaaaa@395E@ Einheiten erhält man den Cosinus, Verschiebt man cos um π 2 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaWaaSaaaeaacqaHapaCaeaacaaIYaaaaaaa@3871@ Einheiten erhält man den Sinus. In 4.6 wird diese Technik näher beschrieben.

  1. sin⁡( π 2 +x)=sin⁡( π 2 −x) MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGaaiikamaalaaabaGaeqiWdahabaGaaGOmaaaacqGHRaWkcaWG4bGaaiykaiabg2da9iGacohacaGGPbGaaiOBaiaacIcadaWcaaqaaiabec8aWbqaaiaaikdaaaGaeyOeI0IaamiEaiaacMcaaaa@482B@
    cos⁡( π 2 +x)=−cos⁡( π 2 −x) MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGGZbGaaiikamaalaaabaGaeqiWdahabaGaaGOmaaaacqGHRaWkcaWG4bGaaiykaiabg2da9iabgkHiTiGacogacaGGVbGaai4CaiaacIcadaWcaaqaaiabec8aWbqaaiaaikdaaaGaeyOeI0IaamiEaiaacMcaaaa@490E@

[4.3.8]

Der Sinus ist symmetrisch zur Senkrechten x= π 2 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiEaiabg2da9maalaaabaGaeqiWdahabaGaaGOmaaaaaaa@3A74@ und der Cosinus punktsymmetrisch zu ( π 2 ,0) MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikamaalaaabaGaeqiWdahabaGaaGOmaaaacaGGSaGaaGimaiaacMcaaaa@3B34@ .

  1. sin⁡(x+2kπ)=sin⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGaaiikaiaadIhacqGHRaWkcaaIYaGaam4Aaiabec8aWjaacMcacqGH9aqpciGGZbGaaiyAaiaac6gacaWG4baaaa@443C@   für jedes k∈ℤ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaam4AaiabgIGiolablssiIcaa@39D4@
    cos⁡(x+2kπ)=cos⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGGZbGaaiikaiaadIhacqGHRaWkcaaIYaGaam4Aaiabec8aWjaacMcacqGH9aqpciGGJbGaai4BaiaacohacaWG4baaaa@4432@   für jedes k∈ℤ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaam4AaiabgIGiolablssiIcaa@39D4@

[4.3.9]

sin und cos wiederholen ihre Werte im Abstand von 2π MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGOmaiabec8aWbaa@3861@ , sie sind also 2π MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGOmaiabec8aWbaa@3861@ -periodisch.

  1. sin⁡x=0 ⇔ x=kπ=2k π 2 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGaamiEaiabg2da9iaaicdacaaMf8Uaeyi1HSTaaGzbVlaadIhacqGH9aqpcaWGRbGaeqiWdaNaeyypa0JaaGOmaiaadUgadaWcaaqaaiabec8aWbqaaiaaikdaaaaaaa@4AE0@   für ein k∈ℤ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaam4AaiabgIGiolablssiIcaa@39D4@
    cos⁡x=0 ⇔ x=(2k−1) π 2 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGGZbGaamiEaiabg2da9iaaicdacaaMf8Uaeyi1HSTaaGzbVlaadIhacqGH9aqpcaGGOaGaaGOmaiaadUgacqGHsislcaaIXaGaaiykamaalaaabaGaeqiWdahabaGaaGOmaaaaaaa@4A29@   für ein k∈ℤ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaam4AaiabgIGiolablssiIcaa@39D4@

[4.3.10]

Die Nullstellen des (reellen) Sinus sind genau die geraden Vielfachen von π 2 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaWaaSaaaeaacqaHapaCaeaacaaIYaaaaaaa@3871@ , die des Cosinus genau die ungeraden. Im Komplexen gibt es keine weiteren Nullstellen.

  1. (sin⁡x) 2 + (cos⁡x) 2 =1 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikaiGacohacaGGPbGaaiOBaiaadIhacaGGPaWaaWbaaSqabeaacaaIYaaaaOGaey4kaSIaaiikaiGacogacaGGVbGaai4CaiaadIhacaGGPaWaaWbaaSqabeaacaaIYaaaaOGaeyypa0JaaGymaaaa@44C8@

[4.3.11]

Diese Gleichheit, oft abgekürzt zu sin⁡ 2 x+ cos⁡ 2 x=1 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbWaaWbaaSqabeaacaaIYaaaaOGaamiEaiabgUcaRiGacogacaGGVbGaai4CamaaCaaaleqabaGaaGOmaaaakiaadIhacqGH9aqpcaaIXaaaaa@4216@ , ist der Satz des Pythagoras, denn |sin⁡x| MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiiFaiGacohacaGGPbGaaiOBaiaadIhacaGG8baaaa@3BBD@ und |cos⁡x| MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiiFaiGacogacaGGVbGaai4CaiaadIhacaGG8baaaa@3BB8@ sind die Kathetenlängen eines rechtwinkligen Dreiecks dessen Hypotenuse die Länge 1 hat.

 i

  1. −1≤sin⁡x≤1 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeyOeI0IaaGymaiabgsMiJkGacohacaGGPbGaaiOBaiaadIhacqGHKjYOcaaIXaaaaa@3F8A@
    −1≤cos⁡x≤1 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeyOeI0IaaGymaiabgsMiJkGacogacaGGVbGaai4CaiaadIhacqGHKjYOcaaIXaaaaa@3F85@

[4.3.12]

Diese Abschätzungen belegen die Beschränktheit von sin und cos, eine Eigenschaft die nur im Reellen gültig ist!

Beweis:  Wir benötigen lediglich die Additionstheoreme und das Symmetrieverhalten.

1. ►   sin⁡(x+ π 2 )=sin⁡x⋅ cos⁡ π 2 ︸ =0 + sin⁡ π 2 ︸ =1 ⋅cos⁡x=cos⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGaaiikaiaadIhacqGHRaWkdaWcaaqaaiabec8aWbqaaiaaikdaaaGaaiykaiabg2da9iGacohacaGGPbGaaiOBaiaadIhacqGHflY1daagaaqaaiGacogacaGGVbGaai4CamaalaaabaGaeqiWdahabaGaaGOmaaaaaSqaaiabg2da9iaaicdaaOGaayjo+dGaey4kaSYaaGbaaeaaciGGZbGaaiyAaiaac6gadaWcaaqaaiabec8aWbqaaiaaikdaaaaaleaacqGH9aqpcaaIXaaakiaawIJ=aiabgwSixlGacogacaGGVbGaai4CaiaadIhacqGH9aqpciGGJbGaai4BaiaacohacaWG4baaaa@63B6@ .

cos⁡(x− π 2 )=sin⁡(x− π 2 + π 2 )=sin⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGGZbGaaiikaiaadIhacqGHsisldaWcaaqaaiabec8aWbqaaiaaikdaaaGaaiykaiabg2da9iGacohacaGGPbGaaiOBaiaacIcacaWG4bGaeyOeI0YaaSaaaeaacqaHapaCaeaacaaIYaaaaiabgUcaRmaalaaabaGaeqiWdahabaGaaGOmaaaacaGGPaGaeyypa0Jaci4CaiaacMgacaGGUbGaamiEaaaa@5077@ .

2. ►   sin⁡( π 2 +x) = ︸ 1. cos⁡x=cos⁡(−x) = ︸ 1. sin⁡( π 2 −x) MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGaaiikamaalaaabaGaeqiWdahabaGaaGOmaaaacqGHRaWkcaWG4bGaaiykamaayaaabaGaeyypa0daleaacaaIXaGaaiOlaaGccaGL44paciGGJbGaai4BaiaacohacaWG4bGaeyypa0Jaci4yaiaac+gacaGGZbGaaiikaiabgkHiTiaadIhacaGGPaWaaGbaaeaacqGH9aqpaSqaaiaaigdacaGGUaaakiaawIJ=aiGacohacaGGPbGaaiOBaiaacIcadaWcaaqaaiabec8aWbqaaiaaikdaaaGaeyOeI0IaamiEaiaacMcaaaa@5AF7@ .

cos⁡( π 2 +x)=cos⁡(−x− π 2 ) = ︸ 1. sin⁡(−x)=−sin⁡x = ︸ 1. −cos⁡(x− π 2 )=−cos⁡( π 2 −x) MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=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@71F5@ .

3. ►  Wir zeigen zunächst per Induktion:

sin⁡(x±2kπ)=sin⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGaaiikaiaadIhacqGHXcqScaaIYaGaam4Aaiabec8aWjaacMcacqGH9aqpciGGZbGaaiyAaiaac6gacaWG4baaaa@4548@   für alle k∈ℕ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaam4AaiabgIGiolablwriLcaa@39C8@ .

Für k=0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaam4Aaiabg2da9iaaicdaaaa@3898@ ist nichts zu zeigen, der Induktionsanfang also trivial. Ist nun die Aussage für ein k∈ℕ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaam4AaiabgIGiolablwriLcaa@39C8@ bereits gültig, so hat man:

sin⁡(x±2(k+1)π) =sin⁡(x±2kπ±2π) =sin⁡(x±2kπ)⋅ cos⁡2π ︸ =1 ± sin⁡2π ︸ =0 ⋅cos⁡(x±2kπ) =sin⁡(x±2kπ) =sin⁡x. MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqbaeaabqGaaaaabaGaci4CaiaacMgacaGGUbGaaiikaiaadIhacqGHXcqScaaIYaGaaiikaiaadUgacqGHRaWkcaaIXaGaaiykaiabec8aWjaacMcaaeaacqGH9aqpciGGZbGaaiyAaiaac6gacaGGOaGaamiEaiabgglaXkaaikdacaWGRbGaeqiWdaNaeyySaeRaaGOmaiabec8aWjaacMcaaeaaaeaacqGH9aqpciGGZbGaaiyAaiaac6gacaGGOaGaamiEaiabgglaXkaaikdacaWGRbGaeqiWdaNaaiykaiabgwSixpaayaaabaGaci4yaiaac+gacaGGZbGaaGOmaiabec8aWbWcbaGaeyypa0JaaGymaaGccaGL44pacqGHXcqSdaagaaqaaiGacohacaGGPbGaaiOBaiaaikdacqaHapaCaSqaaiabg2da9iaaicdaaOGaayjo+dGaeyyXICTaci4yaiaac+gacaGGZbGaaiikaiaadIhacqGHXcqScaaIYaGaam4Aaiabec8aWjaacMcaaeaaaeaacqGH9aqpciGGZbGaaiyAaiaac6gacaGGOaGaamiEaiabgglaXkaaikdacaWGRbGaeqiWdaNaaiykaaqaaaqaaiabg2da9iGacohacaGGPbGaaiOBaiaadIhaaaaaaa@927B@

Damit ist 3. für den Sinus bewiesen. Weiterhin haben wir damit für ein beliebiges k∈ℤ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaam4AaiabgIGiolablssiIcaa@39D4@ :

cos⁡(x+2kπ)=sin⁡(x+ π 2 +2kπ)=sin⁡(x+ π 2 )=cos⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGGZbGaaiikaiaadIhacqGHRaWkcaaIYaGaam4Aaiabec8aWjaacMcacqGH9aqpciGGZbGaaiyAaiaac6gacaGGOaGaamiEaiabgUcaRmaalaaabaGaeqiWdahabaGaaGOmaaaacqGHRaWkcaaIYaGaam4Aaiabec8aWjaacMcacqGH9aqpciGGZbGaaiyAaiaac6gacaGGOaGaamiEaiabgUcaRmaalaaabaGaeqiWdahabaGaaGOmaaaacaGGPaGaeyypa0Jaci4yaiaac+gacaGGZbGaamiEaaaa@5BBB@ .

4. ►  Wir betrachten zunächst nur den Sinus und haben hier wegen der Periodizität:

sin⁡(2kπ)=sin⁡(0+2kπ)=sin⁡0=0 sin⁡((2k+1)π)=sin⁡(π+2kπ)=sin⁡π=0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqbaeaabiqaaaqaaiGacohacaGGPbGaaiOBaiaacIcacaaIYaGaam4Aaiabec8aWjaacMcacqGH9aqpciGGZbGaaiyAaiaac6gacaGGOaGaaGimaiabgUcaRiaaikdacaWGRbGaeqiWdaNaaiykaiabg2da9iGacohacaGGPbGaaiOBaiaaicdacqGH9aqpcaaIWaaabaGaci4CaiaacMgacaGGUbGaaiikaiaacIcacaaIYaGaam4AaiabgUcaRiaaigdacaGGPaGaeqiWdaNaaiykaiabg2da9iGacohacaGGPbGaaiOBaiaacIcacqaHapaCcqGHRaWkcaaIYaGaam4Aaiabec8aWjaacMcacqGH9aqpciGGZbGaaiyAaiaac6gacqaHapaCcqGH9aqpcaaIWaaaaaaa@6B4C@

sin ist also sowohl an den geraden wie auch an den ungeraden Vielfachen von π gleich Null, d.h. jedes Vielfache von π ist eine Nullstelle.

Sei jetzt x eine beliebige Nullstelle des Sinus. Wir müssen zeigen, dass x ein Vielfaches von π ist. O.E. sei dabei x>0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiEaiabg6da+iaaicdaaaa@38A7@ , denn für x=0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiEaiabg2da9iaaicdaaaa@38A5@ ist nichts zu zeigen und nach [4.3.5] ist mit x auch −x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeyOeI0IaamiEaaaa@37D2@ eine Nullstelle.

Mit k≔max⁡{j∈ℕ|2jπ<x} MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaam4Aaiabg2da9iGac2gacaGGHbGaaiiEaiaacUhacaWGQbGaeyicI4SaeSyfHuQaaiiFaiaaikdacaWGQbGaeqiWdaNaeyipaWJaamiEaiaac2haaaa@46FA@ grenzen wir zunächst die Lage von x ein: 2kπ<x≤2(k+1)π MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGOmaiaadUgacqaHapaCcqGH8aapcaWG4bGaeyizImQaaGOmaiaacIcacaWGRbGaey4kaSIaaGymaiaacMcacqaHapaCaaa@4366@ . Für

x ′ ≔x−2kπ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGabmiEayaafaGaeyypa0JaamiEaiabgkHiTiaaikdacaWGRbGaeqiWdahaaa@3D4A@

ist dann 0< x ′ ≤2π MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGimaiabgYda8iqadIhagaqbaiabgsMiJkaaikdacqaHapaCaaa@3CDD@ , ja sogar π≤ x ′ ≤2π MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqiWdaNaeyizImQabmiEayaafaGaeyizImQaaGOmaiabec8aWbaa@3E91@ , denn wegen der Periodizität ist sin x ′ =sin⁡x=0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGabmiEayaafaGaeyypa0Jaci4CaiaacMgacaGGUbGaamiEaiabg2da9iaaicdaaaa@4064@ und gemäß [4.3.3] liegen unterhalb von π keine positiven Nullstellen. Ist nun x ′ =π MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGabmiEayaafaGaeyypa0JaeqiWdahaaa@39B4@ , also

x= x ′ +2kπ=π+2kπ=(2k+1)π MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiEaiabg2da9iqadIhagaqbaiabgUcaRiaaikdacaWGRbGaeqiWdaNaeyypa0JaeqiWdaNaey4kaSIaaGOmaiaadUgacqaHapaCcqGH9aqpcaGGOaGaaGOmaiaadUgacqGHRaWkcaaIXaGaaiykaiabec8aWbaa@4BB2@ ,

so ist nichts weiter zu zeigen. Ist dagegen x ′ >π MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGabmiEayaafaGaeyOpa4JaeqiWdahaaa@39B6@ , so hat man 0≤2π− x ′ <π MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGimaiabgsMiJkaaikdacqaHapaCcqGHsislceWG4bGbauaacqGH8aapcqaHapaCaaa@3F87@ , und da

sin⁡(2π− x ′ )=sin⁡(− x ′ )=−sin x ′ =0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGaaiikaiaaikdacqaHapaCcqGHsislceWG4bGbauaacaGGPaGaeyypa0Jaci4CaiaacMgacaGGUbGaaiikaiabgkHiTiqadIhagaqbaiaacMcacqGH9aqpcqGHsislciGGZbGaaiyAaiaac6gaceWG4bGbauaacqGH9aqpcaaIWaaaaa@4D49@ ,

muss 2π− x ′ =0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGOmaiabec8aWjabgkHiTiqadIhagaqbaiabg2da9iaaicdaaaa@3C17@ , also x ′ =2π MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGabmiEayaafaGaeyypa0JaaGOmaiabec8aWbaa@3A70@ , gelten (wieder mit [4.3.3]) und damit:

x= x ′ +2kπ=2π+2kπ=(2k+2)π MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiEaiabg2da9iqadIhagaqbaiabgUcaRiaaikdacaWGRbGaeqiWdaNaeyypa0JaaGOmaiabec8aWjabgUcaRiaaikdacaWGRbGaeqiWdaNaeyypa0JaaiikaiaaikdacaWGRbGaey4kaSIaaGOmaiaacMcacqaHapaCaaa@4C6F@ .

Die Nullstellen des Cosinus sind jetzt mit [4.3.7] leicht zu beschreiben:

cos⁡x=0  ⇔ sin⁡(x+ π 2 )=0 ⇔ x+ π 2 =kπ   für ein   k∈ℤ ⇔ x=kπ− π 2 =(2k−1) π 2    für ein   k∈ℤ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqbaeaabmGaaaqaaiGacogacaGGVbGaai4CaiaadIhacqGH9aqpcaaIWaGaaGzbVdqaaiabgsDiBlaaywW7ciGGZbGaaiyAaiaac6gacaGGOaGaamiEaiabgUcaRmaalaaabaGaeqiWdahabaGaaGOmaaaacaGGPaGaeyypa0JaaGimaaqaaaqaaiabgsDiBlaaywW7caWG4bGaey4kaSYaaSaaaeaacqaHapaCaeaacaaIYaaaaiabg2da9iaadUgacqaHapaCcaaMe8UaaeOzaiaabYpacaqGYbGaaeiiaiaabwgacaqGPbGaaeOBaiaaysW7caWGRbGaeyicI4SaeSijHikabaaabaGaeyi1HSTaaGzbVlaadIhacqGH9aqpcaWGRbGaeqiWdaNaeyOeI0YaaSaaaeaacqaHapaCaeaacaaIYaaaaiabg2da9iaacIcacaaIYaGaam4AaiabgkHiTiaaigdacaGGPaWaaSaaaeaacqaHapaCaeaacaaIYaaaaiaaysW7caqGMbGaaei=aiaabkhacaqGGaGaaeyzaiaabMgacaqGUbGaaGjbVlaadUgacqGHiiIZcqWIKeIOaaaaaa@8742@

5. ►  Mit dem Additionstheorem [4.3.4] für den Cosinus und dem Symmetrieverhalten hat man:

1=cos⁡(x−x)=cos⁡x⋅cos⁡(−x)−sin⁡x⋅sin⁡(−x)=cos⁡x⋅cos⁡x+sin⁡x⋅sin⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGymaiabg2da9iGacogacaGGVbGaai4CaiaacIcacaWG4bGaeyOeI0IaamiEaiaacMcacqGH9aqpciGGJbGaai4BaiaacohacaWG4bGaeyyXICTaci4yaiaac+gacaGGZbGaaiikaiabgkHiTiaadIhacaGGPaGaeyOeI0Iaci4CaiaacMgacaGGUbGaamiEaiabgwSixlGacohacaGGPbGaaiOBaiaacIcacqGHsislcaWG4bGaaiykaiabg2da9iGacogacaGGVbGaai4CaiaadIhacqGHflY1ciGGJbGaai4BaiaacohacaWG4bGaey4kaSIaci4CaiaacMgacaGGUbGaamiEaiabgwSixlGacohacaGGPbGaaiOBaiaadIhaaaa@6EDF@ .

6. ►  Da (in ℝ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeSyhHekaaa@3758@ ) Quadrate stets positiv sind, hat man nach 5. z.B. für den Sinus:

(sin⁡x) 2 =1− (cos⁡x) 2 ︸ ≥0 ≤1 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiikaiGacohacaGGPbGaaiOBaiaadIhacaGGPaWaaWbaaSqabeaacaaIYaaaaOGaeyypa0JaaGymaiabgkHiTmaayaaabaGaaiikaiGacogacaGGVbGaai4CaiaadIhacaGGPaWaaWbaaSqabeaacaaIYaaaaaqaaiabgwMiZkaaicdaaOGaayjo+dGaeyizImQaaGymaaaa@4BAE@ ,

also: |sin⁡x|≤1 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaiiFaiGacohacaGGPbGaaiOBaiaadIhacaGG8bGaeyizImQaaGymaaaa@3E2D@ . Das ist die Behauptung.

Mit einem kleinen Exkurs in die Physik, und zwar in die Schwingungslehre, stellen wir Modifikationen der Sinusfunktion vor. Dort beschreibt eine Funktion des Typs

f=a sin⁡(ωX+φ) MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOzaiabg2da9iaadggacaaMc8Uaci4CaiaacMgacaGGUbGaaiikaiabeM8a3jaadIfacqGHRaWkcqaHgpGzcaGGPaaaaa@43C0@

eine ungedämpfte Schwingung, wie sie etwa bei einer idealen Pendelbewegung auftritt. Die x-Achse wird hier als "Zeitachse" interpretiert, so dass π als Einheit ungünstig ist; statt dessen kehren wir wieder zu 1 als Einheit zurück und messen mit ihr z.B. Sekunden. Auch die Namen der Parameter haben hier ihren Ursprung:

  • Die Amplitude | a | gibt die maximale Auslenkung (Elongation) der Schwingung an.

  • Mit der Kreisfrequenz ω berechnet man die Frequenz ν der Schwingung: ν= ω 2π MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqyVd4Maeyypa0ZaaSaaaeaacqaHjpWDaeaacaaIYaGaeqiWdahaaaaa@3CFC@ ist die Anzahl der Perioden pro Zeiteinheit. Die Schwingungsdauer T= 1 ν = 2π ω MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamivaiabg2da9maalaaabaGaaGymaaqaaiabe27aUbaacqGH9aqpdaWcaaqaaiaaikdacqaHapaCaeaacqaHjpWDaaaaaa@3FA6@ gibt die für eine Periode benötigte Zeit an.

  • Allgemein nennt man ωX+φ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqyYdCNaamiwaiabgUcaRiabeA8aMbaa@3B2D@ den Phasenwinkel und speziell φ den Nullphasenwinkel, bzw. die Phasenverschiebung der Schwingung. Sie bestimmt die Anfangselongation   f(0)=a sin⁡φ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOzaiaacIcacaaIWaGaaiykaiabg2da9iaadggacaaMc8Uaci4CaiaacMgacaGGUbGaeqOXdygaaa@40EE@ .

Unter den Schwingungen kommen Sinus ( a=ω=1,   φ=0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamyyaiabg2da9iabeM8a3jabg2da9iaaigdacaGGSaGaaGjbVlabeA8aMjabg2da9iaaicdaaaa@4118@ ) und Cosinus ( a=ω=1,   φ= π 2 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamyyaiabg2da9iabeM8a3jabg2da9iaaigdacaGGSaGaaGjbVlabeA8aMjabg2da9maalaaabaGaeqiWdahabaGaaGOmaaaaaaa@42E7@ ) natürlich auch vor. Man beachte, dass die Pixelgrafik bei hohen Frequenzen überfordert ist. Die Darstellung entspricht dann nicht mehr der angegebenen Funktion, zeigt aber z.T. eine interessante Periodiztät. Ich habe daher in diesen Fällen auf ein Ausblenden verzichtet.

 i

​3 sin(−4X+5) ( MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeyOeI0IaaG4maiaaykW7ciGGZbGaaiyAaiaac6gacaGGOaGaeyOeI0IaaGinaiaadIfacqGHRaWkcaaI1aGaaiykaaaa@4177@

Amplitude
1

Frequenz
0.1591545

Schwingungs-
dauer
6.2831853

Anfangs-
elongation
0

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Mit Hilfe von Sinus und Cosinus führen wir nun zwei weitere trigonometrische Funktionen ein. Allerdings werden bei den Funktionsvorschriften Divisionen durchgeführt, so dass die Definitionsbereiche geeignet zu wählen sind. [4.3.10] gibt uns dabei Auskunft über die Lage der Nullstellen von sin und cos.

Definition:  Die Funktionen

tan⁡:ℝ\{(2k−1) π 2 |k∈ℤ}→ℝ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaciiDaiaacggacaGGUbGaaiOoaiabl2riHIqaaiaa=XfacaGG7bGaaiikaiaaikdacaWGRbGaeyOeI0IaaGymaiaacMcadaWcaaqaaiabec8aWbqaaiaaikdaaaGaaiiFaiaadUgacqGHiiIZcqWIKeIOcaGG9bGaeyOKH4QaeSyhHekaaa@4D4C@ gegeben durch  tan⁡(x)≔ sin⁡x cos⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaciiDaiaacggacaGGUbGaaiikaiaadIhacaGGPaGaeyypa0ZaaSaaaeaaciGGZbGaaiyAaiaac6gacaWG4baabaGaci4yaiaac+gacaGGZbGaamiEaaaaaaa@43CA@

[4.3.13]

cot⁡:ℝ\{kπ|k∈ℤ}→ℝ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGG0bGaaiOoaiabl2riHIqaaiaa=XfacaGG7bGaam4Aaiabec8aWjaacYhacaWGRbGaeyicI4SaeSijHiQaaiyFaiabgkziUkabl2riHcaa@48C6@ gegeben durch  cot⁡(x)≔ cos⁡x sin⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGG0bGaaiikaiaadIhacaGGPaGaeyypa0ZaaSaaaeaaciGGJbGaai4BaiaacohacaWG4baabaGaci4CaiaacMgacaGGUbGaamiEaaaaaaa@43CD@

[4.3.14]

sind der Tangens und der Cotangens.

Auch hier werden die Funktionswerte meist klammerfrei geschrieben: tan⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaciiDaiaacggacaGGUbGaamiEaaaa@39B6@ bzw. cot⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGG0bGaamiEaaaa@39B9@ . Man beachte ferner, dass beide Funktionen unendliche viele Definitionslücken besitzen, und zwar Polstellen. Dabei sind die Polstellen des Tangens genau die Nullstellen des Cosinus und die des Cotangens genau die Nullstellen des Sinus.

Die Werte tan⁡0=0=cot⁡ π 2 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaciiDaiaacggacaGGUbGaaGimaiabg2da9iaaicdacqGH9aqpciGGJbGaai4BaiaacshadaWcaaqaaiabec8aWbqaaiaaikdaaaaaaa@4196@ sind direkt einsehbar. Mit ein wenig Mühe finden wir auch einen nicht trivialen Wert: Mit dem Additionstheorem hat man zunächst

1=sin⁡ π 2 =sin⁡( π 4 + π 4 )=2sin⁡ π 4 ⋅cos⁡ π 4 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGymaiabg2da9iGacohacaGGPbGaaiOBamaalaaabaGaeqiWdahabaGaaGOmaaaacqGH9aqpciGGZbGaaiyAaiaac6gacaGGOaWaaSaaaeaacqaHapaCaeaacaaI0aaaaiabgUcaRmaalaaabaGaeqiWdahabaGaaGinaaaacaGGPaGaeyypa0JaaGOmaiGacohacaGGPbGaaiOBamaalaaabaGaeqiWdahabaGaaGinaaaacqGHflY1ciGGJbGaai4BaiaacohadaWcaaqaaiabec8aWbqaaiaaisdaaaaaaa@5706@ ,

und daraus mit Pythagoras:

(sin⁡ π 4 −cos⁡ π 4 ) 2 = sin⁡ 2 π 4 −2sin⁡ π 4 ⋅cos⁡ π 4 + cos⁡ 2 π 4 =1−1=0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=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@664E@ .

Also sind sin⁡ π 4 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbWaaSaaaeaacqaHapaCaeaacaaI0aaaaaaa@3B4B@ und cos⁡ π 4 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGGZbWaaSaaaeaacqaHapaCaeaacaaI0aaaaaaa@3B46@ identisch.

 i

und zwar ist

sin⁡ π 4 = 1 2 =cos⁡ π 4 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbWaaSaaaeaacqaHapaCaeaacaaI0aaaaiabg2da9maalaaabaGaaGymaaqaamaakaaabaGaaGOmaaWcbeaaaaGccqGH9aqpciGGJbGaai4BaiaacohadaWcaaqaaiabec8aWbqaaiaaisdaaaaaaa@4461@ ,

denn wieder mit Pythagoras ist

1= sin⁡ 2 π 4 + cos⁡ 2 π 4 =2 sin⁡ 2 π 4 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGymaiabg2da9iGacohacaGGPbGaaiOBamaaCaaaleqabaGaaGOmaaaakmaalaaabaGaeqiWdahabaGaaGinaaaacqGHRaWkciGGJbGaai4BaiaacohadaahaaWcbeqaaiaaikdaaaGcdaWcaaqaaiabec8aWbqaaiaaisdaaaGaeyypa0JaaGOmaiGacohacaGGPbGaaiOBamaaCaaaleqabaGaaGOmaaaakmaalaaabaGaeqiWdahabaGaaGinaaaaaaa@4D4A@

Also ist sin⁡ π 4 =|sin⁡ π 4 |= 1 2 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbWaaSaaaeaacqaHapaCaeaacaaI0aaaaiabg2da9iaacYhaciGGZbGaaiyAaiaac6gadaWcaaqaaiabec8aWbqaaiaaisdaaaGaaiiFaiabg2da9maakaaabaWaaSaaaeaacaaIXaaabaGaaGOmaaaaaSqabaaaaa@465C@ , denn nach [+] ist sin⁡ π 4 >0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbWaaSaaaeaacqaHapaCaeaacaaI0aaaaiabg6da+iaaicdaaaa@3D0D@ .

  Das aber bedeutet:

tan⁡ π 4 =1=cot⁡ π 4 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaciiDaiaacggacaGGUbWaaSaaaeaacqaHapaCaeaacaaI0aaaaiabg2da9iaaigdacqGH9aqpciGGJbGaai4BaiaacshadaWcaaqaaiabec8aWbqaaiaaisdaaaaaaa@436A@ .

Wir stellen den Tangens in einer Skizze vor. Dabei verzichten wir auf Bezüge zur Physik und betrachten jetzt Funktionen der Form

f=atan⁡(bX−cπ)+d MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOzaiabg2da9iaadggaciGG0bGaaiyyaiaac6gacaGGOaGaamOyaiaadIfacqGHsislcaWGJbGaeqiWdaNaaiykaiabgUcaRiaadsgaaaa@440A@

 i

−3tan⁡(−4X+5π)−8 ( MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeyOeI0IaaG4maiGacshacaGGHbGaaiOBaiaacIcacqGHsislcaaI0aGaamiwaiabgUcaRiaaiwdacqaHapaCcaGGPaGaeyOeI0IaaGioaaaa@4351@

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Tangens und Cotangens besitzen zahlreiche Eigenschaften. Naturgemäß sind sie in der Regel direkt auf entsprechende Sachverhalte bei sin und cos zurückzuführen. Die folgende Bemerkung stellt einige Eigenschaften zusammen.

Bemerkung:  Für alle x,y∈ℝ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiEaiaacYcacaWG5bGaeyicI4SaeSyhHekaaa@3B87@ mit x,y≠(2k−1) π 2 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiEaiaacYcacaWG5bGaeyiyIKRaaiikaiaaikdacaWGRbGaeyOeI0IaaGymaiaacMcadaWcaaqaaiabec8aWbqaaiaaikdaaaaaaa@4190@ bzw. x,y≠kπ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiEaiaacYcacaWG5bGaeyiyIKRaam4Aaiabec8aWbaa@3D07@ gilt:

  1. −tan⁡(x− π 2 )=cot⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeyOeI0IaciiDaiaacggacaGGUbGaaiikaiaadIhacqGHsisldaWcaaqaaiabec8aWbqaaiaaikdaaaGaaiykaiabg2da9iGacogacaGGVbGaaiiDaiaadIhaaaa@4449@
    −cot⁡(x− π 2 )=tan⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeyOeI0Iaci4yaiaac+gacaGG0bGaaiikaiaadIhacqGHsisldaWcaaqaaiabec8aWbqaaiaaikdaaaGaaiykaiabg2da9iGacshacaGGHbGaaiOBaiaadIhaaaa@4449@

[4.3.15]

Die beiden Funktionen gehen durch waagerechtes Verschieben um π 2 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaWaaSaaaeaacqaHapaCaeaacaaIYaaaaaaa@3871@ und anschließendes Spiegeln an der x-Achse ineinander über.

  1. tan⁡x=0 ⇔ x=kπ=2k π 2 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaciiDaiaacggacaGGUbGaamiEaiabg2da9iaaicdacaaMf8Uaeyi1HSTaaGzbVlaadIhacqGH9aqpcaWGRbGaeqiWdaNaeyypa0JaaGOmaiaadUgadaWcaaqaaiabec8aWbqaaiaaikdaaaaaaa@4AD9@   für ein k∈ℤ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaam4AaiabgIGiolablssiIcaa@39D4@
    cot⁡x=0 ⇔ x=(2k−1) π 2 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGG0bGaamiEaiabg2da9iaaicdacaaMf8Uaeyi1HSTaaGzbVlaadIhacqGH9aqpcaGGOaGaaGOmaiaadUgacqGHsislcaaIXaGaaiykamaalaaabaGaeqiWdahabaGaaGOmaaaaaaa@4A2A@   für ein k∈ℤ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaam4AaiabgIGiolablssiIcaa@39D4@

[4.3.16]

Der Tangens hat also dieselben Nullstellen wie sin, der Cotangens dieselben wie cos.

  1. tan⁡x⋅cot⁡x=1 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaciiDaiaacggacaGGUbGaamiEaiabgwSixlGacogacaGGVbGaaiiDaiaadIhacqGH9aqpcaaIXaaaaa@4192@

[4.3.17]

Sind beide Funktionswerte gleichzeitig vorhanden, so ist der eine stets Kehrwert des anderen.

  1. tan⁡(−x)=−tan⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaciiDaiaacggacaGGUbGaaiikaiabgkHiTiaadIhacaGGPaGaeyypa0JaeyOeI0IaciiDaiaacggacaGGUbGaamiEaaaa@41BD@
    cot⁡(−x)=−cot⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGG0bGaaiikaiabgkHiTiaadIhacaGGPaGaeyypa0JaeyOeI0Iaci4yaiaac+gacaGG0bGaamiEaaaa@41C3@

[4.3.18]

Tangens und Cotangens sind punktsymmetrisch.

  1. tan⁡(x+kπ)=tan⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaciiDaiaacggacaGGUbGaaiikaiaadIhacqGHRaWkcaWGRbGaeqiWdaNaaiykaiabg2da9iGacshacaGGHbGaaiOBaiaadIhaaaa@4372@   für jedes k∈ℤ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaam4AaiabgIGiolablssiIcaa@39D4@
    cot⁡(x+kπ)=cot⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGG0bGaaiikaiaadIhacqGHRaWkcaWGRbGaeqiWdaNaaiykaiabg2da9iGacogacaGGVbGaaiiDaiaadIhaaaa@4378@   für jedes k∈ℤ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaam4AaiabgIGiolablssiIcaa@39D4@

[4.3.19]

Tangens und Cotangens sind π-periodisch.

  1. 1+ tan⁡ 2 x= 1 cos⁡ 2 x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGymaiabgUcaRiGacshacaGGHbGaaiOBamaaCaaaleqabaGaaGOmaaaakiaadIhacqGH9aqpdaWcaaqaaiaaigdaaeaaciGGJbGaai4BaiaacohadaahaaWcbeqaaiaaikdaaaGccaWG4baaaaaa@42DA@
    1+ cot⁡ 2 x= 1 sin⁡ 2 x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGymaiabgUcaRiGacogacaGGVbGaaiiDamaaCaaaleqabaGaaGOmaaaakiaadIhacqGH9aqpdaWcaaqaaiaaigdaaeaaciGGZbGaaiyAaiaac6gadaahaaWcbeqaaiaaikdaaaGccaWG4baaaaaa@42E2@

[4.3.20]

  1. tan⁡(x+y)= tan⁡x+tan⁡y 1−tan⁡x⋅tan⁡y MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaciiDaiaacggacaGGUbGaaiikaiaadIhacqGHRaWkcaWG5bGaaiykaiabg2da9maalaaabaGaciiDaiaacggacaGGUbGaamiEaiabgUcaRiGacshacaGGHbGaaiOBaiaadMhaaeaacaaIXaGaeyOeI0IaciiDaiaacggacaGGUbGaamiEaiabgwSixlGacshacaGGHbGaaiOBaiaadMhaaaaaaa@5213@ für tan⁡x⋅tan⁡y≠1 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaciiDaiaacggacaGGUbGaamiEaiabgwSixlGacshacaGGHbGaaiOBaiaadMhacqGHGjsUcaaIXaaaaa@4251@
    cot⁡(x+y)= cot⁡x⋅cot⁡y−1 cot⁡x+cot⁡y MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGG0bGaaiikaiaadIhacqGHRaWkcaWG5bGaaiykaiabg2da9maalaaabaGaci4yaiaac+gacaGG0bGaamiEaiabgwSixlGacogacaGGVbGaaiiDaiaadMhacqGHsislcaaIXaaabaGaci4yaiaac+gacaGG0bGaamiEaiabgUcaRiGacogacaGGVbGaaiiDaiaadMhaaaaaaa@5222@ für cot⁡x+cot⁡y≠0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGG0bGaamiEaiabgUcaRiGacogacaGGVbGaaiiDaiaadMhacqGHGjsUcaaIWaaaaa@40EE@

[4.3.21]

Das sind die Additionstheoreme für Tangens und Cotangens.

Beweis:  

1. ►  Mit [4.3.8] und [4.3.7] ergibt sich:

−tan⁡(x− π 2 )= −sin⁡(x− π 2 ) cos⁡(x− π 2 ) = sin⁡(−x+ π 2 ) cos⁡(x− π 2 ) = sin⁡(x+ π 2 ) cos⁡(x− π 2 ) = cos⁡x sin⁡x =cot⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeyOeI0IaciiDaiaacggacaGGUbGaaiikaiaadIhacqGHsisldaWcaaqaaiabec8aWbqaaiaaikdaaaGaaiykaiabg2da9maalaaabaGaeyOeI0Iaci4CaiaacMgacaGGUbGaaiikaiaadIhacqGHsisldaWcaaqaaiabec8aWbqaaiaaikdaaaGaaiykaaqaaiGacogacaGGVbGaai4CaiaacIcacaWG4bGaeyOeI0YaaSaaaeaacqaHapaCaeaacaaIYaaaaiaacMcaaaGaeyypa0ZaaSaaaeaaciGGZbGaaiyAaiaac6gacaGGOaGaeyOeI0IaamiEaiabgUcaRmaalaaabaGaeqiWdahabaGaaGOmaaaacaGGPaaabaGaci4yaiaac+gacaGGZbGaaiikaiaadIhacqGHsisldaWcaaqaaiabec8aWbqaaiaaikdaaaGaaiykaaaacqGH9aqpdaWcaaqaaiGacohacaGGPbGaaiOBaiaacIcacaWG4bGaey4kaSYaaSaaaeaacqaHapaCaeaacaaIYaaaaiaacMcaaeaaciGGJbGaai4BaiaacohacaGGOaGaamiEaiabgkHiTmaalaaabaGaeqiWdahabaGaaGOmaaaacaGGPaaaaiabg2da9maalaaabaGaci4yaiaac+gacaGGZbGaamiEaaqaaiGacohacaGGPbGaaiOBaiaadIhaaaGaeyypa0Jaci4yaiaac+gacaGG0bGaamiEaaaa@85D3@ ,

und damit:

−cot⁡(x− π 2 )= 1 −tan⁡(x− π 2 ) = 1 cot⁡x =tan⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeyOeI0Iaci4yaiaac+gacaGG0bGaaiikaiaadIhacqGHsisldaWcaaqaaiabec8aWbqaaiaaikdaaaGaaiykaiabg2da9maalaaabaGaaGymaaqaaiabgkHiTiGacshacaGGHbGaaiOBaiaacIcacaWG4bGaeyOeI0YaaSaaaeaacqaHapaCaeaacaaIYaaaaiaacMcaaaGaeyypa0ZaaSaaaeaacaaIXaaabaGaci4yaiaac+gacaGG0bGaamiEaaaacqGH9aqpciGG0bGaaiyyaiaac6gacaWG4baaaa@5546@ .

2. ►   tan⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaciiDaiaacggacaGGUbGaamiEaaaa@39B6@ wird genau dann Null, wenn der Zähler sin⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4CaiaacMgacaGGUbGaamiEaaaa@39BD@ gleich Null ist. Nach [4.3.10] also genau dann, wenn x=kπ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiEaiabg2da9iaadUgacqaHapaCaaa@3A98@ ist. Beim Cotangens argumentiert man analog.

3. ►   tan⁡x⋅cot⁡x= sin⁡x cos⁡x ⋅ cos⁡x sin⁡x =1 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaciiDaiaacggacaGGUbGaamiEaiabgwSixlGacogacaGGVbGaaiiDaiaadIhacqGH9aqpdaWcaaqaaiGacohacaGGPbGaaiOBaiaadIhaaeaaciGGJbGaai4BaiaacohacaWG4baaaiabgwSixpaalaaabaGaci4yaiaac+gacaGGZbGaamiEaaqaaiGacohacaGGPbGaaiOBaiaadIhaaaGaeyypa0JaaGymaaaa@544C@ .

4. ►  Wir benutzen das Symmetrieverhalten [4.3.5]:

tan⁡(−x)= sin⁡(−x) cos⁡(−x) = −sin⁡x cos⁡x =−tan⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaciiDaiaacggacaGGUbGaaiikaiabgkHiTiaadIhacaGGPaGaeyypa0ZaaSaaaeaaciGGZbGaaiyAaiaac6gacaGGOaGaeyOeI0IaamiEaiaacMcaaeaaciGGJbGaai4BaiaacohacaGGOaGaeyOeI0IaamiEaiaacMcaaaGaeyypa0ZaaSaaaeaacqGHsislciGGZbGaaiyAaiaac6gacaWG4baabaGaci4yaiaac+gacaGGZbGaamiEaaaacqGH9aqpcqGHsislciGG0bGaaiyyaiaac6gacaWG4baaaa@58AC@ .

Die entsprechende Eigenschaft des Cotangens erhält man analog.

5. ►  Wir benötigen einige Vorüberlegungen. Zunächst erhält man mit [4.3.8]:

sin⁡(x+π)=sin⁡( π 2 +x+ π 2 )=sin⁡( π 2 −x− π 2 )=sin⁡(−x)=−sin⁡x cos⁡(x+π)=cos⁡( π 2 +x+ π 2 )=−cos⁡( π 2 −x− π 2 )=−cos⁡(−x)=−cos⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=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@9575@

und über die Periodizität von Sinus und Cosinus dann auch:

sin⁡(x−π)=sin⁡(x−π+2π)=sin⁡(x+π)=−sin⁡x cos⁡(x−π)=cos⁡(x−π+2π)=cos⁡(x+π)=−cos⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=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@7B38@

Damit schließlich haben wir:

tan⁡(x±π)= sin⁡(x±π) cos⁡(x±π) = −sin⁡x −cos⁡x = sin⁡x cos⁡x =tan⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaciiDaiaacggacaGGUbGaaiikaiaadIhacqGHXcqScqaHapaCcaGGPaGaeyypa0ZaaSaaaeaaciGGZbGaaiyAaiaac6gacaGGOaGaamiEaiabgglaXkabec8aWjaacMcaaeaaciGGJbGaai4BaiaacohacaGGOaGaamiEaiabgglaXkabec8aWjaacMcaaaGaeyypa0ZaaSaaaeaacqGHsislciGGZbGaaiyAaiaac6gacaWG4baabaGaeyOeI0Iaci4yaiaac+gacaGGZbGaamiEaaaacqGH9aqpdaWcaaqaaiGacohacaGGPbGaaiOBaiaadIhaaeaaciGGJbGaai4BaiaacohacaWG4baaaiabg2da9iGacshacaGGHbGaaiOBaiaadIhaaaa@69A1@ .[++]

Nun zeigen wir per Induktion: tan⁡(x±kπ)=tan⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaciiDaiaacggacaGGUbGaaiikaiaadIhacqGHXcqScaWGRbGaeqiWdaNaaiykaiabg2da9iGacshacaGGHbGaaiOBaiaadIhaaaa@447E@ für alle k∈ℕ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaam4AaiabgIGiolablwriLcaa@39C8@ . Da für k=0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaam4Aaiabg2da9iaaicdaaaa@3898@ offensichtlich nichts zu tun ist, bleibt nur der Induktionsschluss: Mit [++] ergibt sich aus der Induktionsvoraussetzung:

tan⁡(x±(k+1)π)=tan⁡(x±kπ±π)=tan⁡(x±kπ)=tan⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaciiDaiaacggacaGGUbGaaiikaiaadIhacqGHXcqScaGGOaGaam4AaiabgUcaRiaaigdacaGGPaGaeqiWdaNaaiykaiabg2da9iGacshacaGGHbGaaiOBaiaacIcacaWG4bGaeyySaeRaam4Aaiabec8aWjabgglaXkabec8aWjaacMcacqGH9aqpciGG0bGaaiyyaiaac6gacaGGOaGaamiEaiabgglaXkaadUgacqaHapaCcaGGPaGaeyypa0JaciiDaiaacggacaGGUbGaamiEaaaa@60AF@ .

Nun zum Cotangens: Ist x, und damit auch x+kπ MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiEaiabgUcaRiaadUgacqaHapaCaaa@3A74@ , ein ungerades Vielfaches von π 2 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaWaaSaaaeaacqaHapaCaeaacaaIYaaaaaaa@3871@ , so hat man nach [4.3.16]:   cot⁡(x+kπ)=0=cot⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGG0bGaaiikaiaadIhacqGHRaWkcaWGRbGaeqiWdaNaaiykaiabg2da9iaaicdacqGH9aqpciGGJbGaai4BaiaacshacaWG4baaaa@4538@ . In allen anderen Fällen greift man auf das gerade Bewiesene zurück:

cot⁡(x+kπ)= 1 tan⁡(x+kπ) = 1 tan⁡x =cot⁡x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGG0bGaaiikaiaadIhacqGHRaWkcaWGRbGaeqiWdaNaaiykaiabg2da9maalaaabaGaaGymaaqaaiGacshacaGGHbGaaiOBaiaacIcacaWG4bGaey4kaSIaam4Aaiabec8aWjaacMcaaaGaeyypa0ZaaSaaaeaacaaIXaaabaGaciiDaiaacggacaGGUbGaamiEaaaacqGH9aqpciGGJbGaai4BaiaacshacaWG4baaaa@539E@ .

6. ►  Diese Gleichungen ergeben sich aus dem Satz des Pythagoras [4.3.11], z.B. für den Tangens:

1+ tan⁡ 2 x=1+ sin⁡ 2 x cos⁡ 2 x = cos⁡ 2 x+ sin⁡ 2 x cos⁡ 2 x = 1 cos⁡ 2 x MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaaGymaiabgUcaRiGacshacaGGHbGaaiOBamaaCaaaleqabaGaaGOmaaaakiaadIhacqGH9aqpcaaIXaGaey4kaSYaaSaaaeaaciGGZbGaaiyAaiaac6gadaahaaWcbeqaaiaaikdaaaGccaWG4baabaGaci4yaiaac+gacaGGZbWaaWbaaSqabeaacaaIYaaaaOGaamiEaaaacqGH9aqpdaWcaaqaaiGacogacaGGVbGaai4CamaaCaaaleqabaGaaGOmaaaakiaadIhacqGHRaWkciGGZbGaaiyAaiaac6gadaahaaWcbeqaaiaaikdaaaGccaWG4baabaGaci4yaiaac+gacaGGZbWaaWbaaSqabeaacaaIYaaaaOGaamiEaaaacqGH9aqpdaWcaaqaaiaaigdaaeaaciGGJbGaai4BaiaacohadaahaaWcbeqaaiaaikdaaaGccaWG4baaaaaa@5F5E@ .

7. ►  Mit den Additionstheoremen [4.3.4] für Sinus und Cosinus beweisen wir die erste Gleichung:

tan⁡x+tan⁡y 1−tan⁡x⋅tan⁡y = sin⁡x cos⁡x + sin⁡y cos⁡y 1− sin⁡x⋅sin⁡y cos⁡x⋅cos⁡y = sin⁡x⋅cos⁡y+cos⁡x⋅sin⁡y cos⁡x⋅cos⁡y cos⁡x⋅cos⁡y−sin⁡x⋅sin⁡y cos⁡x⋅cos⁡y = sin⁡x⋅cos⁡y+cos⁡x⋅sin⁡y cos⁡x⋅cos⁡y−sin⁡x⋅sin⁡y = sin⁡(x+y) cos⁡(x+y) =tan⁡(x+y). MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaqbaeaabuGaaaaabaWaaSaaaeaaciGG0bGaaiyyaiaac6gacaWG4bGaey4kaSIaciiDaiaacggacaGGUbGaamyEaaqaaiaaigdacqGHsislciGG0bGaaiyyaiaac6gacaWG4bGaeyyXICTaciiDaiaacggacaGGUbGaamyEaaaaaeaacqGH9aqpdaWcaaqaamaalaaabaGaci4CaiaacMgacaGGUbGaamiEaaqaaiGacogacaGGVbGaai4CaiaadIhaaaGaey4kaSYaaSaaaeaaciGGZbGaaiyAaiaac6gacaWG5baabaGaci4yaiaac+gacaGGZbGaamyEaaaaaeaacaaIXaGaeyOeI0YaaSaaaeaaciGGZbGaaiyAaiaac6gacaWG4bGaeyyXICTaci4CaiaacMgacaGGUbGaamyEaaqaaiGacogacaGGVbGaai4CaiaadIhacqGHflY1ciGGJbGaai4BaiaacohacaWG5baaaaaaaeaaaeaacqGH9aqpdaWcaaqaamaalaaabaGaci4CaiaacMgacaGGUbGaamiEaiabgwSixlGacogacaGGVbGaai4CaiaadMhacqGHRaWkciGGJbGaai4BaiaacohacaWG4bGaeyyXICTaci4CaiaacMgacaGGUbGaamyEaaqaaiGacogacaGGVbGaai4CaiaadIhacqGHflY1ciGGJbGaai4BaiaacohacaWG5baaaaqaamaalaaabaGaci4yaiaac+gacaGGZbGaamiEaiabgwSixlGacogacaGGVbGaai4CaiaadMhacqGHsislciGGZbGaaiyAaiaac6gacaWG4bGaeyyXICTaci4CaiaacMgacaGGUbGaamyEaaqaaiGacogacaGGVbGaai4CaiaadIhacqGHflY1ciGGJbGaai4BaiaacohacaWG5baaaaaaaeaaaeaacqGH9aqpdaWcaaqaaiGacohacaGGPbGaaiOBaiaadIhacqGHflY1ciGGJbGaai4BaiaacohacaWG5bGaey4kaSIaci4yaiaac+gacaGGZbGaamiEaiabgwSixlGacohacaGGPbGaaiOBaiaadMhaaeaaciGGJbGaai4BaiaacohacaWG4bGaeyyXICTaci4yaiaac+gacaGGZbGaamyEaiabgkHiTiGacohacaGGPbGaaiOBaiaadIhacqGHflY1ciGGZbGaaiyAaiaac6gacaWG5baaaaqaaaqaaiabg2da9maalaaabaGaci4CaiaacMgacaGGUbGaaiikaiaadIhacqGHRaWkcaWG5bGaaiykaaqaaiGacogacaGGVbGaai4CaiaacIcacaWG4bGaey4kaSIaamyEaiaacMcaaaaabaaabaGaeyypa0JaciiDaiaacggacaGGUbGaaiikaiaadIhacqGHRaWkcaWG5bGaaiykaaaaaaa@F194@

Falls cot⁡(x+y)≠0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGG0bGaaiikaiaadIhacqGHRaWkcaWG5bGaaiykaiabgcMi5kaaicdaaaa@3F73@ ( ⇔   cos⁡(x+y)≠0   ⇔   cos⁡x⋅cos⁡y≠sin⁡x⋅sin⁡y   ⇔   cot⁡x⋅cot⁡y≠1 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeyi1HSTaaGjbVlGacogacaGGVbGaai4CaiaacIcacaWG4bGaey4kaSIaamyEaiaacMcacqGHGjsUcaaIWaGaaGjbVlabgsDiBlaaysW7ciGGJbGaai4BaiaacohacaWG4bGaeyyXICTaci4yaiaac+gacaGGZbGaamyEaiabgcMi5kGacohacaGGPbGaaiOBaiaadIhacqGHflY1ciGGZbGaaiyAaiaac6gacaWG5bGaaGjbVlabgsDiBlaaysW7ciGGJbGaai4BaiaacshacaWG4bGaeyyXICTaci4yaiaac+gacaGG0bGaamyEaiabgcMi5kaaigdaaaa@705D@ ), gelingt damit auch der Nachweis der zweiten Gleichung:

cot⁡(x+y)= 1 tan⁡(x+y) = 1−tan⁡x⋅tan⁡y tan⁡x+tan⁡y = 1− 1 cot⁡x⋅cot⁡y 1 cot⁡x + 1 cot⁡y = cot⁡x⋅cot⁡y−1 cot⁡x+cot⁡y MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGG0bGaaiikaiaadIhacqGHRaWkcaWG5bGaaiykaiabg2da9maalaaabaGaaGymaaqaaiGacshacaGGHbGaaiOBaiaacIcacaWG4bGaey4kaSIaamyEaiaacMcaaaGaeyypa0ZaaSaaaeaacaaIXaGaeyOeI0IaciiDaiaacggacaGGUbGaamiEaiabgwSixlGacshacaGGHbGaaiOBaiaadMhaaeaaciGG0bGaaiyyaiaac6gacaWG4bGaey4kaSIaciiDaiaacggacaGGUbGaamyEaaaacqGH9aqpdaWcaaqaaiaaigdacqGHsisldaWcaaqaaiaaigdaaeaaciGGJbGaai4BaiaacshacaWG4bGaeyyXICTaci4yaiaac+gacaGG0bGaamyEaaaaaeaadaWcaaqaaiaaigdaaeaaciGGJbGaai4BaiaacshacaWG4baaaiabgUcaRmaalaaabaGaaGymaaqaaiGacogacaGGVbGaaiiDaiaadMhaaaaaaiabg2da9maalaaabaGaci4yaiaac+gacaGG0bGaamiEaiabgwSixlGacogacaGGVbGaaiiDaiaadMhacqGHsislcaaIXaaabaGaci4yaiaac+gacaGG0bGaamiEaiabgUcaRiGacogacaGGVbGaaiiDaiaadMhaaaaaaa@87AF@ .

Ist cot⁡(x+y)=0 MathType@MTEF@5@5@+=feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLnhiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFepeea0xe9Lq=Jc9vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=xfr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaci4yaiaac+gacaGG0bGaaiikaiaadIhacqGHRaWkcaWG5bGaaiykaiabg2da9iaaicdaaaa@3EB2@ , so steht auf beiden Seiten der Gleichung Null.


4.2. 4.4.