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Trigonometric Addition Formulas

date2026-07-14document_iddoc_f55dc0b074d7c255fc9dd693f5544655description三角関数の加法定理を回転行列の合成から導出し、差角、倍角、半角公式とその適用条件を証明する。prerequisites三角関数 / 単位円type講義content_typelecturestatusactiverelateddata/lecture/math/trigonometry/trigonometric-functions.lecture.n.md / data/lecture/math/vector/geometric-vectors-and-dot-products.lecture.n.md / data/lecture/math/algebra/complex-numbers-and-complex-plane.lecture.n.md
mathtrigonometryhighschoollecture

1Introduction

The addition formulas express in coordinates the fact that composing two plane rotations gives one rotation through the sum of their angles. This lecture derives them rigorously from rotation matrices and organizes the difference-angle, double-angle, and half-angle formulas as consequences.

data/lecture/math/trigonometry/trigonometric-functions.lecture.n.md

2Rotation Matrices

For a 2×2 matrix A=(aij) and a column vector (x,y)T, define

A(xy)=(a11x+a12ya21x+a22y).

For two matrices A,B, define (AB)ij=k=12aikbkj. This product represents composition: first apply B, then apply A. Write a point at distance r0 and with argument t as rPt, and define rotation by Qθ(rPt)=rPt+θ. Addition of signed arc lengths gives QαQβ=Qα+β. A rotation fixes the origin and preserves both parallelograms spanned by vectors and directed distances along lines; hence it preserves vector addition and real scalar multiplication. Thus Qθ is linear.

Let e1=(1,0)T and e2=(0,1)T be the standard basis. The map Qθ is linear and preserves lengths, orthogonality, and orientation. It sends e1 to u=(cosθ,sinθ)T. The image of e2 must be the unique unit vector perpendicular to u for which (u,v) has positive orientation, namely v=(-sinθ,cosθ)T. Hence the matrix of Qθ is

Rθ=(cosθ-sinθsinθcosθ)

Applying Rβ and then Rα geometrically rotates every vector through a total angle α+β. Thus, without using the addition formulas,

RαRβ=Rα+β.

Direct multiplication gives

RαRβ=(cosαcosβ-sinαsinβ-(cosαsinβ+sinαcosβ)sinαcosβ+cosαsinβcosαcosβ-sinαsinβ).

Comparison with Rα+β proves, for all real α,β,

[PARSE ERROR: Undefined("Command(\"boxed\")")]cos(α+β)=cosαcosβ-sinαsinβ
[PARSE ERROR: Undefined("Command(\"boxed\")")]sin(α+β)=sinαcosβ+cosαsinβ.

3Difference-Angle Formulas

Replace β by -β and use cos(-β)=cosβ and sin(-β)=-sinβ:

[PARSE ERROR: Undefined("Command(\"boxed\")")]cos(α-β)=cosαcosβ+sinαsinβ
[PARSE ERROR: Undefined("Command(\"boxed\")")]sin(α-β)=sinαcosβ-cosαsinβ.

4Double-Angle Formulas

Setting β=α=θ gives

[PARSE ERROR: Undefined("Command(\"boxed\")")]sin2θ=2sinθcosθ
[PARSE ERROR: Undefined("Command(\"boxed\")")]cos2θ=cos2θ-sin2θ=2cos2θ-1=1-2sin2θ.

The last two forms use sin2θ+cos2θ=1.

5Addition Formulas for Tangent

If cosαcosβ0 and 1-tanαtanβ0, divide the sine addition formula by the cosine addition formula to obtain

[PARSE ERROR: Undefined("Command(\"boxed\")")]tan(α+β)=tanα+tanβ1-tanαtanβ.

Similarly, if cosαcosβ0 and 1+tanαtanβ0, then

[PARSE ERROR: Undefined("Command(\"boxed\")")]tan(α-β)=tanα-tanβ1+tanαtanβ.

6Half-Angle Formulas and Signs

Replacing θ by θ/2 in the double-angle formulas gives

sin2θ2=1-cosθ2,cos2θ2=1+cosθ2.

Taking square roots yields

sinθ2=±1-cosθ2,cosθ2=±1+cosθ2,

where the sign is determined by the position of θ/2, including both quadrants and coordinate axes. Formulas involving tangent apply only where their denominators are nonzero.

7An Alternative Proof Using Complex Numbers

This section is an alternative proof to be used only after complex numbers and Euler's formula have been introduced; it is not a prerequisite for the rotation-matrix proof.

Substitute eiθ=cosθ+isinθ into

ei(α+β)=eiαeiβ

and compare real and imaginary parts to obtain the same addition formulas.

8Scope

The sine and cosine formulas for sums, differences, and double angles hold for all real angles. The tangent formulas hold under the nonzero conditions stated above; every transformation involving a quotient requires a nonzero denominator. When square roots are taken in the half-angle formulas, the signs must be selected from the position of the half-angle, including both quadrants and coordinate axes.

9Related Lectures

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