Trigonometric functions
Trigonometric functions
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Trigonometric functions

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Basis of trigonometry: if two right triangles have equal acute angles, they are similar, so their corresponding side lengths are proportional.

In mathematics, the trigonometric functions (also called circular functions, angle functions or goniometric functions)[1] are real functions which relate an angle of a right-angled triangle to ratios of two side lengths. They are widely used in all sciences that are related to geometry, such as navigation, solid mechanics, celestial mechanics, geodesy, and many others. They are among the simplest periodic functions, and as such are also widely used for studying periodic phenomena through Fourier analysis.

The trigonometric functions most widely used in modern mathematics are the sine, the cosine, and the tangent functions. Their reciprocals are respectively the cosecant, the secant, and the cotangent functions, which are less used. Each of these six trigonometric functions has a corresponding inverse function and has an analog among the hyperbolic functions.

The oldest definitions of trigonometric functions, related to right-angle triangles, define them only for acute angles. To extend the sine and cosine functions to functions whose domain is the whole real line, geometrical definitions using the standard unit circle (i.e., a circle with radius 1 unit) are often used; then the domain of the other functions is the real line with some isolated points removed. Modern definitions express trigonometric functions as infinite series or as solutions of differential equations. This allows extending the domain of sine and cosine functions to the whole complex plane, and the domain of the other trigonometric functions to the complex plane with some isolated points removed.

Notation

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Conventionally, an abbreviation of each trigonometric function's name is used as its symbol in formulas. Today, the most common versions of these abbreviations are "sin" for sine, "cos" for cosine, "tan" or "tg" for tangent, "sec" for secant, "csc" or "cosec" for cosecant, and "cot" or "ctg" for cotangent. Historically, these abbreviations were first used in prose sentences to indicate particular line segments or their lengths related to an arc of an arbitrary circle, and later to indicate ratios of lengths, but as the function concept developed in the 17th–18th century, they began to be considered as functions of real-number-valued angle measures, and written with functional notation, for example sin(x). Parentheses are still often omitted to reduce clutter, but are sometimes necessary; for example the expression would typically be interpreted to mean so parentheses are required to express

A positive integer appearing as a superscript after the symbol of the function denotes exponentiation, not function composition. For example and denote not This differs from the (historically later) general functional notation in which

In contrast, the superscript is commonly used to denote the inverse function, not the reciprocal. For example and denote the inverse trigonometric function alternatively written The equation implies not In this case, the superscript could be considered as denoting a composed or iterated function, but negative superscripts other than are not in common use.

Right-angled triangle definitions

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In this right triangle, denoting the measure of angle BAC as A: sin A = a/c; cos A = b/c; tan A = a/b.
Plot of the six trigonometric functions, the unit circle, and a line for the angle θ = 0.7 radians. The points labeled 1, Sec(θ), Csc(θ) represent the length of the line segment from the origin to that point. Sin(θ), Tan(θ), and 1 are the heights to the line starting from the x-axis, while Cos(θ), 1, and Cot(θ) are lengths along the x-axis starting from the origin.

If the acute angle θ is given, then any right triangles that have an angle of θ are similar to each other. This means that the ratio of any two side lengths depends only on θ. Thus these six ratios define six functions of θ, which are the trigonometric functions. In the following definitions, the hypotenuse is the length of the side opposite the right angle, opposite represents the side opposite the given angle θ, and adjacent represents the side between the angle θ and the right angle.[2][3]

sine
cosecant
cosine
secant
tangent
cotangent

Various mnemonics can be used to remember these definitions.

In a right-angled triangle, the sum of the two acute angles is a right angle, that is, 90° or π/2 radians. Therefore and represent the same ratio, and thus are equal. This identity and analogous relationships between the other trigonometric functions are summarized in the following table.

Top: Trigonometric function sin θ for selected angles θ, πθ, π + θ, and 2πθ in the four quadrants.
Bottom: Graph of sine versus angle. Angles from the top panel are identified.
Summary of relationships between trigonometric functions[4]
Function Description Relationship
using radians using degrees
sine opposite/hypotenuse
cosine adjacent/hypotenuse
tangent opposite/adjacent
cotangent adjacent/opposite
secant hypotenuse/adjacent
cosecant hypotenuse/opposite

Radians versus degrees

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In geometric applications, the argument of a trigonometric function is generally the measure of an angle. For this purpose, any angular unit is convenient. One common unit is degrees, in which a right angle is 90° and a complete turn is 360° (particularly in elementary mathematics).

However, in calculus and mathematical analysis, the trigonometric functions are generally regarded more abstractly as functions of real or complex numbers, rather than angles. In fact, the functions sin and cos can be defined for all complex numbers in terms of the exponential function, via power series,[5] or as solutions to differential equations given particular initial values[6] (see below), without reference to any geometric notions. The other four trigonometric functions (tan, cot, sec, csc) can be defined as quotients and reciprocals of sin and cos, except where zero occurs in the denominator. It can be proved, for real arguments, that these definitions coincide with elementary geometric definitions if the argument is regarded as an angle in radians.[5] Moreover, these definitions result in simple expressions for the derivatives and indefinite integrals for the trigonometric functions.[7] Thus, in settings beyond elementary geometry, radians are regarded as the mathematically natural unit for describing angle measures.

When radians (rad) are employed, the angle is given as the length of the arc of the unit circle subtended by it: the angle that subtends an arc of length 1 on the unit circle is 1 rad (≈ 57.3°),[8] and a complete turn (360°) is an angle of 2π (≈ 6.28) rad.[9] Since radian is dimensionless, i.e. 1 rad = 1, the degree symbol can also be regarded as a mathematical constant factor such that 1° = π/180 ≈ 0.0175.[citation needed]

Unit-circle definitions

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All of the trigonometric functions of the angle θ (theta) can be constructed geometrically in terms of a unit circle centered at O.
Sine function on unit circle (top) and its graph (bottom)
In this illustration, the six trigonometric functions of an arbitrary angle θ are represented as Cartesian coordinates of points related to the unit circle. The y-axis ordinates of A, B and D are sin θ, tan θ and csc θ, respectively, while the x-axis abscissas of A, C and E are cos θ, cot θ and sec θ, respectively.
Signs of trigonometric functions in each quadrant. Mnemonics like "all students take calculus" indicates when sine, cosine, and tangent are positive from quadrants I to IV.[10]

The six trigonometric functions can be defined as coordinate values of points on the Euclidean plane that are related to the unit circle, which is the circle of radius one centered at the origin O of this coordinate system. While right-angled triangle definitions allow for the definition of the trigonometric functions for angles between 0 and radians (90°), the unit circle definitions allow the domain of trigonometric functions to be extended to all positive and negative real numbers.

Let be the ray obtained by rotating by an angle θ the positive half of the x-axis (counterclockwise rotation for and clockwise rotation for ). This ray intersects the unit circle at the point The ray extended to a line if necessary, intersects the line of equation at point and the line of equation at point The tangent line to the unit circle at the point A, is perpendicular to and intersects the y- and x-axes at points and The coordinates of these points give the values of all trigonometric functions for any arbitrary real value of θ in the following manner.

The trigonometric functions cos and sin are defined, respectively, as the x- and y-coordinate values of point A. That is, and [11]

In the range , this definition coincides with the right-angled triangle definition, by taking the right-angled triangle to have the unit radius OA as hypotenuse. And since the equation holds for all points on the unit circle, this definition of cosine and sine also satisfies the Pythagorean identity.

The other trigonometric functions can be found along the unit circle as and and

By applying the Pythagorean identity and geometric proof methods, these definitions can readily be shown to coincide with the definitions of tangent, cotangent, secant and cosecant in terms of sine and cosine, that is

Trigonometric functions: Sine, Cosine, Tangent, Cosecant (dotted), Secant (dotted), Cotangent (dotted)animation

Since a rotation of an angle of does not change the position or size of a shape, the points A, B, C, D, and E are the same for two angles whose difference is an integer multiple of . Thus trigonometric functions are periodic functions with period . That is, the equalities and hold for any angle θ and any integer k. The same is true for the four other trigonometric functions. By observing the sign and the monotonicity of the functions sine, cosine, cosecant, and secant in the four quadrants, one can show that is the smallest value for which they are periodic (i.e., is the fundamental period of these functions). However, after a rotation by an angle , the points B and C already return to their original position, so that the tangent function and the cotangent function have a fundamental period of . That is, the equalities and hold for any angle θ and any integer k.

Algebraic values

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The unit circle, with some points labeled with their cosine and sine (in this order), and the corresponding angles in radians and degrees.

The algebraic expressions for the most important angles are as follows:

(zero angle) (right angle)

Writing the numerators as square roots of consecutive non-negative integers, with a denominator of 2, provides an easy way to remember the values.[12]

Such simple expressions generally do not exist for other angles which are rational multiples of a right angle.

  • For an angle which, measured in degrees, is a multiple of three, the exact trigonometric values of the sine and the cosine may be expressed in terms of square roots. These values of the sine and the cosine may thus be constructed by ruler and compass.
  • For an angle of an integer number of degrees, the sine and the cosine may be expressed in terms of square roots and the cube root of a non-real complex number. Galois theory allows a proof that, if the angle is not a multiple of 3°, non-real cube roots are unavoidable.
  • For an angle which, expressed in degrees, is a rational number, the sine and the cosine are algebraic numbers, which may be expressed in terms of n-th roots. This results from the fact that the Galois groups of the cyclotomic polynomials are cyclic.
  • For an angle which, expressed in degrees, is not a rational number, then either the angle or both the sine and the cosine are transcendental numbers. This is a corollary of Baker's theorem, proved in 1966.
  • If the sine of an angle is a rational number then the cosine is not necessarily a rational number, and vice-versa. However if the tangent of an angle is rational then both the sine and cosine of the double angle will be rational.

Simple algebraic values

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The following table lists the sines, cosines, and tangents of multiples of 15 degrees from 0 to 90 degrees.

Angle, θ, in
radians degrees
Undefined

Definitions in analysis

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Graphs of sine, cosine and tangent
The sine function (blue) is closely approximated by its Taylor polynomial of degree 7 (pink) for a full cycle centered on the origin.
Animation for the approximation of cosine via Taylor polynomials.
together with the first Taylor polynomials

G. H. Hardy noted in his 1908 work A Course of Pure Mathematics that the definition of the trigonometric functions in terms of the unit circle is not satisfactory, because it depends implicitly on a notion of angle that can be measured by a real number.[clarification needed][13] Thus in modern analysis, trigonometric functions are usually constructed without reference to geometry.

Various ways exist in the literature for defining the trigonometric functions in a manner suitable for analysis; they include:

  • Using the "geometry" of the unit circle, which requires formulating the arc length of a circle (or area of a sector) analytically.[13]
  • By a power series, which is particularly well-suited to complex variables.[13][14]
  • By using an infinite product expansion.[13]
  • By inverting the inverse trigonometric functions, which can be defined as integrals of algebraic or rational functions.[13]
  • As solutions of a differential equation.[15]

Definition by differential equations

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Sine and cosine can be defined as the unique solution to the initial value problem:[16]

Differentiating again, and , so both sine and cosine are solutions of the same ordinary differential equation Sine is the unique solution with y(0) = 0 and y′(0) = 1; cosine is the unique solution with y(0) = 1 and y′(0) = 0.

One can then prove, as a theorem, that solutions are periodic, having the same period. Writing this period as is then a definition of the real number which is independent of geometry.

Applying the quotient rule to the tangent , so the tangent function satisfies the ordinary differential equation It is the unique solution with y(0) = 0.

Power series expansion

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The basic trigonometric functions can be defined by the following power series expansions.[17] These series are also known as the Taylor series or Maclaurin series of these trigonometric functions: The radius of convergence of these series is infinite. Therefore, the sine and the cosine can be extended to entire functions (also called "sine" and "cosine"), which are (by definition) complex-valued functions that are defined and holomorphic on the whole complex plane.

Term-by-term differentiation shows that the sine and cosine defined by the series obey the differential equation discussed previously, and conversely one can obtain these series from elementary recursion relations derived from the differential equation.

Being defined as fractions of entire functions, the other trigonometric functions may be extended to meromorphic functions, that is functions that are holomorphic in the whole complex plane, except some isolated points called poles. Here, the poles are the numbers of the form for the tangent and the secant, or for the cotangent and the cosecant, where k is an arbitrary integer.

Recurrences relations may also be computed for the coefficients of the Taylor series of the other trigonometric functions. These series have a finite radius of convergence. Their coefficients have a combinatorial interpretation: they enumerate alternating permutations of finite sets.[18]

More precisely, defining

Un, the n-th up/down number,
Bn, the n-th Bernoulli number, and
En, is the n-th Euler number,

one has the following series expansions:[19]

Continued fraction expansion

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The following continued fractions are valid in the whole complex plane:

[citation needed]


The last one was used in the historically first proof that π is irrational.[20]

Partial fraction expansion

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There is a series representation as partial fraction expansion where just translated reciprocal functions are summed up, such that the poles of the cotangent function and the reciprocal functions match:[21] This identity can be proved with the Herglotz trick.[22] Combining the (–n)-th with the n-th term lead to absolutely convergent series: Similarly, one can find a partial fraction expansion for the secant, cosecant and tangent functions:

Infinite product expansion

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The following infinite product for the sine is due to Leonhard Euler, and is of great importance in complex analysis:[23] This may be obtained from the partial fraction decomposition of given above, which is the logarithmic derivative of .[24] From this, it can be deduced also that

Euler's formula and the exponential function

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and are the real and imaginary part of respectively.

Euler's formula relates sine and cosine to the exponential function: This formula is commonly considered for real values of x, but it remains true for all complex values.

Proof: Let and One has for j = 1, 2. The quotient rule implies thus that . Therefore, is a constant function, which equals 1, as This proves the formula.

One has

Solving this linear system in sine and cosine, one can express them in terms of the exponential function:

When x is real, this may be rewritten as

Most trigonometric identities can be proved by expressing trigonometric functions in terms of the complex exponential function by using above formulas, and then using the identity for simplifying the result.

Euler's formula can also be used to define the basic trigonometric function directly, as follows, using the language of topological groups.[25] The set of complex numbers of unit modulus is a compact and connected topological group, which has a neighborhood of the identity that is homeomorphic to the real line. Therefore, it is isomorphic as a topological group to the one-dimensional torus group , via an isomorphism In simple terms, , and this isomorphism is unique up to taking complex conjugates.

For a nonzero real number (the base), the function defines an isomorphism of the group . The real and imaginary parts of are the cosine and sine, where is used as the base for measuring angles. For example, when , we get the measure in radians, and the usual trigonometric functions. When , we get the sine and cosine of angles measured in degrees.

Note that is the unique value at which the derivative becomes a unit vector with positive imaginary part at . This fact can, in turn, be used to define the constant .

Definition via integration

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Another way to define the trigonometric functions in analysis is using integration.[13][26] For a real number , put where this defines this inverse tangent function. Also, is defined by a definition that goes back to Karl Weierstrass.[27]

On the interval , the trigonometric functions are defined by inverting the relation . Thus we define the trigonometric functions by where the point is on the graph of and the positive square root is taken.

This defines the trigonometric functions on . The definition can be extended to all real numbers by first observing that, as , , and so and . Thus and are extended continuously so that . Now the conditions and define the sine and cosine as periodic functions with period , for all real numbers.

Proving the basic properties of sine and cosine, including the fact that sine and cosine are analytic, one may first establish the addition formulae. First, holds, provided , since after the substitution . In particular, the limiting case as gives Thus we have and So the sine and cosine functions are related by translation over a quarter period .

Definitions using functional equations

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One can also define the trigonometric functions using various functional equations.

For example,[28] the sine and the cosine form the unique pair of continuous functions that satisfy the difference formula and the added condition

In the complex plane

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The sine and cosine of a complex number can be expressed in terms of real sines, cosines, and hyperbolic functions as follows:

By taking advantage of domain coloring, it is possible to graph the trigonometric functions as complex-valued functions. Various features unique to the complex functions can be seen from the graph; for example, the sine and cosine functions can be seen to be unbounded as the imaginary part of becomes larger (since the color white represents infinity), and the fact that the functions contain simple zeros or poles is apparent from the fact that the hue cycles around each zero or pole exactly once. Comparing these graphs with those of the corresponding Hyperbolic functions highlights the relationships between the two.

Trigonometric functions in the complex plane

Periodicity and asymptotes

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The sine and cosine functions are periodic, with period , which is the smallest positive period: Consequently, the cosecant and secant also have as their period.

The functions sine and cosine also have semiperiods , and and consequently Also, (see Complementary angles).

The function has a unique zero (at ) in the strip . The function has the pair of zeros in the same strip. Because of the periodicity, the zeros of sine are There zeros of cosine are All of the zeros are simple zeros, and both functions have derivative at each of the zeros.

The tangent function has a simple zero at and vertical asymptotes at , where it has a simple pole of residue . Again, owing to the periodicity, the zeros are all the integer multiples of and the poles are odd multiples of , all having the same residue. The poles correspond to vertical asymptotes

The cotangent function has a simple pole of residue 1 at the integer multiples of and simple zeros at odd multiples of . The poles correspond to vertical asymptotes

Basic identities

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Many identities interrelate the trigonometric functions. This section contains the most basic ones; for more identities, see List of trigonometric identities. These identities may be proved geometrically from the unit-circle definitions or the right-angled-triangle definitions (although, for the latter definitions, care must be taken for angles that are not in the interval [0, π/2], see Proofs of trigonometric identities). For non-geometrical proofs using only tools of calculus, one may use directly the differential equations, in a way that is similar to that of the above proof of Euler's identity. One can also use Euler's identity for expressing all trigonometric functions in terms of complex exponentials and using properties of the exponential function.

Parity

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The cosine and the secant are even functions; the other trigonometric functions are odd functions. That is:

Periods

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All trigonometric functions are periodic functions of period 2π. This is the smallest period, except for the tangent and the cotangent, which have π as smallest period. This means that, for every integer k, one has See Periodicity and asymptotes.

Pythagorean identity

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The Pythagorean identity, is the expression of the Pythagorean theorem in terms of trigonometric functions. It is . Dividing through by either or gives and .

Sum and difference formulas

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The sum and difference formulas allow expanding the sine, the cosine, and the tangent of a sum or a difference of two angles in terms of sines and cosines and tangents of the angles themselves. These can be derived geometrically, using arguments that date to Ptolemy (see Angle sum and difference identities). One can also produce them algebraically using Euler's formula.

Sum

Difference

When the two angles are equal, the sum formulas reduce to simpler equations known as the double-angle formulae.

These identities can be used to derive the product-to-sum identities.

By setting (see half-angle formulae), all trigonometric functions of can be expressed as rational fractions of : Together with this is the tangent half-angle substitution, which reduces the computation of integrals and antiderivatives of trigonometric functions to that of rational fractions.

Derivatives and antiderivatives

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The derivatives of trigonometric functions result from those of sine and cosine by applying the quotient rule. The values given for the antiderivatives in the following table can be verified by differentiating them. The number C is a constant of integration.

Note: For the integral of can also be written as and the integral of for as where is the inverse hyperbolic sine.

Alternatively, the derivatives of the 'co-functions' can be obtained using trigonometric identities and the chain rule:

Inverse functions

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The trigonometric functions are periodic, and hence not injective, so strictly speaking, they do not have an inverse function. However, on each interval on which a trigonometric function is monotonic, one can define an inverse function, and this defines inverse trigonometric functions as multivalued functions. To define a true inverse function, one must restrict the domain to an interval where the function is monotonic, and is thus bijective from this interval to its image by the function. The common choice for this interval, called the set of principal values, is given in the following table. As usual, the inverse trigonometric functions are denoted with the prefix "arc" before the name or its abbreviation of the function.

Function Definition Domain Set of principal values

The notations sin−1, cos−1, etc. are often used for arcsin and arccos, etc. When this notation is used, inverse functions could be confused with multiplicative inverses. The notation with the "arc" prefix avoids such a confusion, though "arcsec" for arcsecant can be confused with "arcsecond".

Just like the sine and cosine, the inverse trigonometric functions can also be expressed in terms of infinite series. They can also be expressed in terms of complex logarithms.

Applications

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Angles and sides of a triangle

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In this section A, B, C denote the three (interior) angles of a triangle, and a, b, c denote the lengths of the respective opposite edges. They are related by various formulas, which are named by the trigonometric functions they involve.

Law of sines

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The law of sines states that for an arbitrary triangle with sides a, b, and c and angles opposite those sides A, B and C: where Δ is the area of the triangle, or, equivalently, where R is the triangle's circumradius.

It can be proved by dividing the triangle into two right ones and using the above definition of sine. The law of sines is useful for computing the lengths of the unknown sides in a triangle if two angles and one side are known. This is a common situation occurring in triangulation, a technique to determine unknown distances by measuring two angles and an accessible enclosed distance.

Law of cosines

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The law of cosines (also known as the cosine formula or cosine rule) is an extension of the Pythagorean theorem: or equivalently,

In this formula the angle at C is opposite to the side c. This theorem can be proved by dividing the triangle into two right ones and using the Pythagorean theorem.

The law of cosines can be used to determine a side of a triangle if two sides and the angle between them are known. It can also be used to find the cosines of an angle (and consequently the angles themselves) if the lengths of all the sides are known.

Law of tangents

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The law of tangents says that: .

Law of cotangents

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If s is the triangle's semiperimeter, (a + b + c)/2, and r is the radius of the triangle's incircle, then rs is the triangle's area. Therefore Heron's formula implies that:

.

The law of cotangents says that:[29] It follows that

Periodic functions

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A Lissajous curve, a figure formed with a trigonometry-based function.
An animation of the additive synthesis of a square wave with an increasing number of harmonics
Sinusoidal basis functions (bottom) can form a sawtooth wave (top) when added. All the basis functions have nodes at the nodes of the sawtooth, and all but the fundamental (k = 1) have additional nodes. The oscillation seen about the sawtooth when k is large is called the Gibbs phenomenon.

The trigonometric functions are also important in physics. The sine and the cosine functions, for example, are used to describe simple harmonic motion, which models many natural phenomena, such as the movement of a mass attached to a spring and, for small angles, the pendular motion of a mass hanging by a string. The sine and cosine functions are one-dimensional projections of uniform circular motion.

Trigonometric functions also prove to be useful in the study of general periodic functions. The characteristic wave patterns of periodic functions are useful for modeling recurring phenomena such as sound or light waves.[30]

Under rather general conditions, a periodic function f (x) can be expressed as a sum of sine waves or cosine waves in a Fourier series.[31] Denoting the sine or cosine basis functions by φk, the expansion of the periodic function f (t) takes the form:

For example, the square wave can be written as the Fourier series

In the animation of a square wave at top right it can be seen that just a few terms already produce a fairly good approximation. The superposition of several terms in the expansion of a sawtooth wave are shown underneath.

History

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While the early study of trigonometry can be traced to antiquity, the trigonometric functions as they are in use today were developed in the medieval period. The chord function was defined by Hipparchus of Nicaea (180–125 BCE) and Ptolemy of Roman Egypt (90–165 CE). The functions of sine and versine (1 − cosine) are closely related to the jyā and koti-jyā functions used in Gupta period Indian astronomy (Aryabhatiya, Surya Siddhanta), via translation from Sanskrit to Arabic and then from Arabic to Latin.[32] (See Aryabhata's sine table.)

All six trigonometric functions in current use were known in Islamic mathematics by the 9th century, as was the law of sines, used in solving triangles.[33] Al-Khwārizmī (c. 780–850) produced tables of sines and cosines. Circa 860, Habash al-Hasib al-Marwazi defined the tangent and the cotangent, and produced their tables.[34][35] Muhammad ibn Jābir al-Harrānī al-Battānī (853–929) defined the reciprocal functions of secant and cosecant, and produced the first table of cosecants for each degree from 1° to 90°.[35] The trigonometric functions were later studied by mathematicians including Omar Khayyám, Bhāskara II, Nasir al-Din al-Tusi, Jamshīd al-Kāshī (14th century), Ulugh Beg (14th century), Regiomontanus (1464), Rheticus, and Rheticus' student Valentinus Otho.

Madhava of Sangamagrama (c. 1400) made early strides in the analysis of trigonometric functions in terms of infinite series.[36] (See Madhava series and Madhava's sine table.)

The tangent function was brought to Europe by Giovanni Bianchini in 1467 in trigonometry tables he created to support the calculation of stellar coordinates.[37]

The terms tangent and secant were first introduced by the Danish mathematician Thomas Fincke in his book Geometria rotundi (1583).[38]

The 17th century French mathematician Albert Girard made the first published use of the abbreviations sin, cos, and tan in his book Trigonométrie.[39]

In a paper published in 1682, Gottfried Leibniz proved that sin x is not an algebraic function of x.[40] Though defined as ratios of sides of a right triangle, and thus appearing to be rational functions, Leibnitz result established that they are actually transcendental functions of their argument. The task of assimilating circular functions into algebraic expressions was accomplished by Euler in his Introduction to the Analysis of the Infinite (1748). His method was to show that the sine and cosine functions are alternating series formed from the even and odd terms respectively of the exponential series. He presented "Euler's formula", as well as near-modern abbreviations (sin., cos., tang., cot., sec., and cosec.).[32]

A few functions were common historically, but are now seldom used, such as the chord, versine (which appeared in the earliest tables[32]), haversine, coversine,[41] half-tangent (tangent of half an angle), and exsecant. List of trigonometric identities shows more relations between these functions.

Historically, trigonometric functions were often combined with logarithms in compound functions like the logarithmic sine, logarithmic cosine, logarithmic secant, logarithmic cosecant, logarithmic tangent and logarithmic cotangent.[42][43][44][45]

Etymology

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The word sine derives[46] from Latin sinus, meaning "bend; bay", and more specifically "the hanging fold of the upper part of a toga", "the bosom of a garment", which was chosen as the translation of what was interpreted as the Arabic word jaib, meaning "pocket" or "fold" in the twelfth-century translations of works by Al-Battani and al-Khwārizmī into Medieval Latin.[47] The choice was based on a misreading of the Arabic written form j-y-b (جيب), which itself originated as a transliteration from Sanskrit jīvā, which along with its synonym jyā (the standard Sanskrit term for the sine) translates to "bowstring", being in turn adopted from Ancient Greek χορδή "string".[48]

The word tangent comes from Latin tangens meaning "touching", since the line touches the circle of unit radius, whereas secant stems from Latin secans—"cutting"—since the line cuts the circle.[49]

The prefix "co-" (in "cosine", "cotangent", "cosecant") is found in Edmund Gunter's Canon triangulorum (1620), which defines the cosinus as an abbreviation of the sinus complementi (sine of the complementary angle) and proceeds to define the cotangens similarly.[50][51]

See also

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Notes

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References

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Trigonometric functions are real-valued functions in mathematics that relate angles, typically in right-angled triangles, to the ratios of the lengths of the triangle's sides, providing a foundational tool for analyzing geometric relationships and periodic phenomena.[1] The six principal trigonometric functions—sine (sin), cosine (cos), tangent (tan), cosecant (csc), secant (sec), and cotangent (cot)—are defined as follows for an acute angle θ in a right triangle with opposite side o, adjacent side a, and hypotenuse h: sin θ = o/h, cos θ = a/h, tan θ = o/a, csc θ = h/o, sec θ = h/a, and cot θ = a/o.[1] These functions extend beyond triangles to the unit circle, where sin θ and cos θ represent the y- and x-coordinates, respectively, of the point on the circle reached by rotating θ radians (or degrees) counterclockwise from the positive x-axis, enabling their application to any real angle.[2] Tan θ is then defined as the ratio sin θ / cos θ, with the reciprocal functions following accordingly.[2] Key properties include their periodicity—sin and cos repeat every 2π radians, while tan repeats every π radians—and bounded ranges, such as -1 ≤ sin θ ≤ 1 and -1 ≤ cos θ ≤ 1 for all real θ.[2] The development of trigonometric functions traces back to ancient astronomy and geometry, with Hipparchus around 140 BC creating the first tables of chord lengths in circles, laying the groundwork for modern sine and cosine.[3] Subsequent advancements by figures like Ptolemy, who established the identity sin²θ + cos²θ = 1, and Arab mathematicians such as Abu'l-Wafa, who derived tangent formulas, evolved these from practical astronomical tools into systematic functions by the medieval period.[3] By the 17th and 18th centuries, contributions from Euler and others standardized notation and integrated them with complex numbers and calculus.[3] In contemporary mathematics and science, trigonometric functions are indispensable for modeling oscillatory behaviors, such as waves in physics and signals in engineering, as well as in calculus for derivatives and integrals, linear algebra for rotations, and statistics for periodic data analysis.[4] They also underpin real-world applications, including navigation for determining positions at sea, structural engineering for bridge and building design, and astronomy for calculating celestial distances.[5]

Introductory Concepts

Notation

The primary trigonometric functions are denoted using the following standard symbols: sine by sin\sin, cosine by cos\cos, tangent by tan\tan, cotangent by cot\cot, secant by sec\sec, and cosecant by csc\csc. These abbreviations, shortened from their full names (such as "sine" from Latin sinus and "tangent" from the geometric line), have become the conventional notation in mathematical texts since the 17th century. The reciprocal relationships are implicit in the notation, with csc\csc as the reciprocal of sin\sin, sec\sec of cos\cos, and cot\cot of tan\tan.[6] Historically, trigonometric notation evolved from earlier forms using full words or alternative abbreviations, such as "S" for sine or "R" for the radius in chord-based computations, to the more compact modern symbols introduced in the 1600s. For instance, the abbreviations "sin" and "cos" were introduced by Edmund Gunter around 1620–1624, while "tan" dates to Thomas Fincke's 1583 text; Gottfried Wilhelm Leibniz further popularized functional notation like sinx\sin x in the late 17th century, treating these as functions of a variable rather than fixed ratios.[7] This shift from verbose or geometric-specific symbols to concise, function-oriented ones facilitated the integration of trigonometry into calculus and analysis.[3] The argument of a trigonometric function, which represents the input angle or value, is typically denoted by θ\theta (theta) in geometric and introductory contexts to highlight its angular interpretation, often in conjunction with units like degrees or radians. In contrast, xx is the standard variable for arguments in broader mathematical applications, including real or complex numbers, allowing trigonometric functions to be analyzed as part of general function theory.[8] Multi-angle notations, such as sin(2x)\sin(2x) or cos(nθ)\cos(n\theta) where nn is an integer, extend the basic function symbols to express compositions or multiples of the argument, enabling compact representation of periodic extensions and laying the groundwork for exploring relationships among trigonometric values.[9] These forms underscore the functions' versatility in modeling oscillations and waves without altering the core symbolic conventions.

Angle Measurement

Angles are measured using two primary units: degrees and radians. The degree, denoted by the symbol °, is defined such that one complete rotation around a circle corresponds to 360 degrees. This unit traces its origins to ancient Babylonian astronomy, where the sexagesimal (base-60) system led to the division of the full circle—or the ecliptic path of the sun—into 360 equal parts for tracking celestial movements.[10][11] In contrast, the radian provides a more geometrically natural measure of angles. One radian is the central angle subtended at the center of a circle by an arc whose length equals the circle's radius. Consequently, a full rotation around the circle measures exactly 2π2\pi radians, linking angular measure directly to the circle's circumference. To convert between these units, the formula radians = degrees ×π180\times \frac{\pi}{180} is used, reflecting the proportional relationship between the two systems. This conversion is essential for applications spanning geometry and analysis. Radians hold particular advantages in calculus, where trigonometric functions are differentiated and integrated. For instance, the derivative of sin(x)\sin(x) is cos(x)\cos(x) precisely when xx is measured in radians, avoiding extraneous scaling factors that arise with degrees. This property simplifies many analytical computations and aligns angular measures with linear dimensions in a unit circle.[12]

Right Triangle Definitions

The trigonometric functions can be defined geometrically using the ratios of the sides of a right-angled triangle, where one angle is exactly 90° and the other two angles are acute. In such a triangle, the side opposite the right angle is called the hypotenuse, which is the longest side, while the other two sides are the legs: one adjacent to the acute angle of interest and the other opposite to it.[13][14] Consider an acute angle θ\theta in a right triangle, with the opposite side of length aa, the adjacent side of length bb, and the hypotenuse of length cc. The sine function is defined as the ratio of the opposite side to the hypotenuse: sinθ=ac\sin \theta = \frac{a}{c}. The cosine function is the ratio of the adjacent side to the hypotenuse: cosθ=bc\cos \theta = \frac{b}{c}. The tangent function is the ratio of the opposite side to the adjacent side: tanθ=ab\tan \theta = \frac{a}{b}.[13][14] The remaining three trigonometric functions are the reciprocals of these: the cosecant is cscθ=1sinθ=ca\csc \theta = \frac{1}{\sin \theta} = \frac{c}{a}, the secant is secθ=1cosθ=cb\sec \theta = \frac{1}{\cos \theta} = \frac{c}{b}, and the cotangent is cotθ=1tanθ=ba\cot \theta = \frac{1}{\tan \theta} = \frac{b}{a}. These definitions apply specifically to acute angles θ\theta in the right triangle, so 0<θ<900^\circ < \theta < 90^\circ (or 0<θ<π20 < \theta < \frac{\pi}{2} in radians), where all ratios are positive.[13][14] To visualize, imagine a right triangle with the right angle at vertex C, acute angle θ\theta at vertex A, opposite side aa (from B to C), adjacent side bb (from A to C), and hypotenuse cc (from A to B); the labels align with the standard ratios above. A common mnemonic for recalling the definitions of sine, cosine, and tangent is SOH-CAH-TOA, where SOH stands for "sine equals opposite over hypotenuse," CAH for "cosine equals adjacent over hypotenuse," and TOA for "tangent equals opposite over adjacent."[15]

Unit Circle Definitions

The unit circle provides a geometric foundation for defining the trigonometric functions sine and cosine for any real number θ, extending beyond the limitations of right triangles to encompass all angles, including those greater than 90° or negative. Consider a circle of radius 1 centered at the origin (0,0) in the Cartesian plane. An angle θ is formed by rotating a ray from the positive x-axis counterclockwise (positive θ) or clockwise (negative θ) to a terminal side that intersects the unit circle at a point P = (x, y). The cosine of θ is defined as the x-coordinate of P, so cos θ = x, and the sine of θ is defined as the y-coordinate, so sin θ = y. This definition ensures that sin²θ + cos²θ = 1 for all θ, as (x, y) lies on the circle x² + y² = 1.[16][17][13] The signs of sin θ and cos θ depend on the quadrant in which the terminal side of θ lies. In quadrant I (0 < θ < π/2), both sin θ and cos θ are positive. In quadrant II (π/2 < θ < π), sin θ is positive while cos θ is negative. In quadrant III (π < θ < 3π/2), both are negative. In quadrant IV (3π/2 < θ < 2π), sin θ is negative while cos θ is positive. For angles beyond one full rotation or negative values, the position repeats periodically every 2π radians due to the circular nature of the definitions.[18][19][20] For example, consider an angle θ in standard position whose terminal side passes through the point (4, -3) in quadrant IV. The distance from the origin to this point is r = √(4² + (-3)²) = √(25) = 5. The trigonometric values are then sin θ = y/r = -3/5, cos θ = x/r = 4/5, tan θ = y/x = -3/4, csc θ = 1/sin θ = -5/3, sec θ = 1/cos θ = 5/4, and cot θ = 1/tan θ = -4/3. These values match the coordinates of the point where the terminal ray intersects the unit circle, which is (4/5, -3/5). This illustrates the extension of the unit circle definitions to any point on the terminal ray, with signs determined by the quadrant: in quadrant IV, sine and tangent are negative while cosine is positive. To evaluate sin θ and cos θ for angles in quadrants II, III, or IV, the reference angle is used, defined as the acute angle between the terminal side of θ and the nearest x-axis. The reference angle θ' equals θ for quadrant I, π - θ for quadrant II, θ - π for quadrant III, and 2π - θ for quadrant IV (adjusting for coterminal angles if necessary). The values are then computed as sin θ = ± sin θ' and cos θ = ± cos θ', with the sign determined by the quadrant. This approach leverages known values from quadrant I while accounting for the geometric positions on the unit circle.[21][22][23] When angles are measured in radians, θ represents the arc length along the unit circle from the positive x-axis to point P, since the radius is 1 and arc length s = rθ simplifies to s = θ. This radian measure facilitates natural connections between angles, arc lengths, and trigonometric functions, as the coordinates (cos θ, sin θ) directly correspond to positions traversed by that arc. The unit circle definitions thus generalize the ratios from right triangles—where sin θ = opposite/hypotenuse and cos θ = adjacent/hypotenuse for acute angles—to arbitrary θ by embedding the triangle within the circle's geometry.[24][25][26]

Exact Values

Common Algebraic Values

The exact values of trigonometric functions at standard angles such as 0°, 30°, 45°, 60°, and 90° (or their radian equivalents 0, π/6, π/4, π/3, and π/2) are derived primarily from special right triangles, where the side lengths follow specific ratios that allow algebraic expressions without approximation.[14] For the 45° angle, consider an isosceles right triangle with legs of length 1 and hypotenuse √2, formed by placing the right angle at the origin and the equal angles at 45°. The sine of 45° is the opposite side over the hypotenuse, yielding sin(45°) = 1/√2 = √2/2; similarly, cos(45°) = adjacent/hypotenuse = √2/2, and tan(45°) = opposite/adjacent = 1.[14] The 30° and 60° angles arise from a 30°-60°-90° triangle, obtained by bisecting an equilateral triangle with side length 2, resulting in side ratios of 1 (opposite 30°), √3 (opposite 60°), and 2 (hypotenuse). Thus, sin(30°) = 1/2, cos(30°) = √3/2, tan(30°) = 1/√3 = √3/3; for 60°, sin(60°) = √3/2, cos(60°) = 1/2, tan(60°) = √3.[14] At 0° and 90°, the values follow directly from the right triangle definitions or the unit circle, where sin(0°) = 0, cos(0°) = 1, tan(0°) = 0, sin(90°) = 1, cos(90°) = 0, and tan(90°) is undefined due to division by zero.[14] For angles at multiples of π/2 beyond the first quadrant, such as π/2, π, 3π/2, and 2π (equivalent to 90°, 180°, 270°, and 360°), the unit circle provides the coordinates of intersection points, with cos(θ) as the x-coordinate and sin(θ) as the y-coordinate on the circle of radius 1.[27] These yield sin(π/2) = 1, cos(π/2) = 0, tan(π/2) undefined; sin(π) = 0, cos(π) = -1, tan(π) = 0; sin(3π/2) = -1, cos(3π/2) = 0, tan(3π/2) undefined; sin(2π) = 0, cos(2π) = 1, tan(2π) = 0.[27] The following table summarizes the exact values for sine, cosine, and tangent at these standard angles:
Angle (degrees)Angle (radians)sincostan
0010
30°π/61/2√3/2√3/3
45°π/4√2/2√2/21
60°π/3√3/21/2√3
90°π/210undefined
180°π0-10
270°3π/2-10undefined
360°010
These values are foundational for computations in trigonometry and arise consistently from the geometric definitions.[14][27]

Properties and Identities

Periodicity and Symmetry

Trigonometric functions exhibit periodicity, meaning their values repeat at regular intervals. The sine and cosine functions are periodic with a fundamental period of 2π2\pi, such that sin(θ+2π)=sinθ\sin(\theta + 2\pi) = \sin \theta and cos(θ+2π)=cosθ\cos(\theta + 2\pi) = \cos \theta for all θ\theta. This periodicity arises from their definitions on the unit circle, where angles differing by 2π2\pi correspond to the same point. The tangent and cotangent functions have a smaller fundamental period of π\pi, with tan(θ+π)=tanθ\tan(\theta + \pi) = \tan \theta and cot(θ+π)=cotθ\cot(\theta + \pi) = \cot \theta. These periods reflect the repeating patterns in their ratios of sine and cosine. The graphs of these functions illustrate their periodicity over one full period. For the sine function, the graph over [0,2π][0, 2\pi] starts at (0, 0), rises to a maximum of 1 at π/2\pi/2, returns to 0 at π\pi, reaches a minimum of -1 at 3π/23\pi/2, and ends at 0 at 2π2\pi, forming a smooth wave that repeats thereafter. The cosine graph over the same interval begins at (0, 1), decreases to 0 at π/2\pi/2, to -1 at π\pi, back to 0 at 3π/23\pi/2, and to 1 at 2π2\pi, shifted horizontally by π/2\pi/2 from the sine wave. For tangent, one period from π/2-\pi/2 to π/2\pi/2 (excluding endpoints) shows a curve passing through (0, 0), approaching ++\infty as θ\theta nears π/2\pi/2 from the left, and -\infty from the right of π/2-\pi/2, with vertical asymptotes at odd multiples of π/2\pi/2. The cotangent graph over (0,π)(0, \pi) starts near ++\infty just after 0, passes through (π/2\pi/2, 0), and approaches -\infty near π\pi, with vertical asymptotes at integer multiples of π\pi. Symmetry properties further characterize these functions, classifying them as even or odd based on their behavior under negation of the argument. The cosine function is even, satisfying cos(θ)=cosθ\cos(-\theta) = \cos \theta, which implies its graph is symmetric about the y-axis; for example, the value at θ\theta matches that at θ-\theta. In contrast, the sine, tangent, and cotangent functions are odd, with sin(θ)=sinθ\sin(-\theta) = -\sin \theta, tan(θ)=tanθ\tan(-\theta) = -\tan \theta, and cot(θ)=cotθ\cot(-\theta) = -\cot \theta; their graphs exhibit rotational symmetry about the origin, such that the point (θ,f(θ))(\theta, f(\theta)) maps to (θ,f(θ))(-\theta, -f(\theta)). These symmetries are evident in the graphs: the cosine wave mirrors itself across the y-axis, while the sine wave rotates 180 degrees around the origin to coincide with itself, and similar point symmetry holds for tangent and cotangent within their periodic branches between asymptotes.

Pythagorean Identities

The Pythagorean identities form a cornerstone of trigonometric theory, expressing relationships between the squares of sine and cosine, and their reciprocals. The fundamental identity is
sin2θ+cos2θ=1, \sin^2 \theta + \cos^2 \theta = 1,
which holds for all real angles θ.[28][29] This identity derives directly from the unit circle definition of the trigonometric functions. On the unit circle centered at the origin with radius 1, any point corresponding to angle θ has coordinates (cosθ,sinθ)(\cos \theta, \sin \theta). The equation of the circle, x2+y2=1x^2 + y^2 = 1, substitutes to yield cos2θ+sin2θ=1\cos^2 \theta + \sin^2 \theta = 1.[28][29] The identity extends to the other pairs of cofunctions by algebraic manipulation. Dividing the primary identity by cos2θ\cos^2 \theta (where cosθ0\cos \theta \neq 0) gives
tan2θ+1=sec2θ. \tan^2 \theta + 1 = \sec^2 \theta.
Similarly, dividing by sin2θ\sin^2 \theta (where sinθ0\sin \theta \neq 0) yields
1+cot2θ=csc2θ. 1 + \cot^2 \theta = \csc^2 \theta.
These forms connect the tangent-secant and cotangent-cosecant pairs, respectively.[30][31] In practice, the Pythagorean identities simplify trigonometric expressions and aid in solving equations. For example, they allow rewriting sin2θ\sin^2 \theta as 1cos2θ1 - \cos^2 \theta to express one function in terms of another, which is useful in integration or verifying equalities. Another application involves simplifying ratios like sin2θcos2θ+1\frac{\sin^2 \theta}{\cos^2 \theta} + 1, which reduces to sec2θ\sec^2 \theta using the tangent-secant form.[28][32]

Sum and Difference Formulas

The sum and difference formulas for the sine and cosine functions express the trigonometric values of summed or differenced angles in terms of products of the individual functions. These identities are fundamental in trigonometry and originate from geometric considerations in the second century CE, as developed by Ptolemy in his Almagest using chord lengths in a circle.[33] The addition formula for sine is given by
sin(A+B)=sinAcosB+cosAsinB, \sin(A + B) = \sin A \cos B + \cos A \sin B,
and the subtraction formula by
sin(AB)=sinAcosBcosAsinB. \sin(A - B) = \sin A \cos B - \cos A \sin B.
Similarly, for cosine, the addition formula is
cos(A+B)=cosAcosBsinAsinB, \cos(A + B) = \cos A \cos B - \sin A \sin B,
and the subtraction formula is
cos(AB)=cosAcosB+sinAsinB. \cos(A - B) = \cos A \cos B + \sin A \sin B.
These formulas can be derived using the geometry of the unit circle. Consider points on the unit circle centered at the origin: let Q=(cosA,sinA)Q = (\cos A, \sin A) and S=(cos(B),sin(B))=(cosB,sinB)S = (\cos(-B), \sin(-B)) = (\cos B, -\sin B). The distance between QQ and SS is equated to the distance between the point at angle A+BA + B, R=(cos(A+B),sin(A+B))R = (\cos(A + B), \sin(A + B)), and the origin point P=(1,0)P = (1, 0). Applying the distance formula yields PR2=22cos(A+B)PR^2 = 2 - 2\cos(A + B) and QS2=22(cosAcosBsinAsinB)QS^2 = 2 - 2(\cos A \cos B - \sin A \sin B), leading directly to the cosine addition formula; the sine formulas follow by considering rotations or auxiliary angles.[34] An alternative geometric derivation employs Ptolemy's theorem for a cyclic quadrilateral inscribed in a unit circle with diameter BC=1BC = 1. For angles AA and BB, the sides and diagonals correspond to sines and cosines via the law of sines. Applying Ptolemy's theorem—stating that the product of the diagonals equals the sum of the products of opposite sides—reformulates to sin(A+B)=sinAcosB+cosAsinB\sin(A + B) = \sin A \cos B + \cos A \sin B. The subtraction formula arises similarly by adjusting the configuration with BCBC as the diameter. This approach, rooted in Euclidean geometry (Elements, Book III, Propositions 20 and 21), underscores the formulas' ancient origins.[35] The tangent addition and subtraction formulas are derived from the sine and cosine identities by division:
tan(A+B)=tanA+tanB1tanAtanB,tan(AB)=tanAtanB1+tanAtanB, \tan(A + B) = \frac{\tan A + \tan B}{1 - \tan A \tan B}, \quad \tan(A - B) = \frac{\tan A - \tan B}{1 + \tan A \tan B},
provided the denominators are nonzero. These follow immediately from tanθ=sinθ/cosθ\tan \theta = \sin \theta / \cos \theta and simplifying the quotients of the sum and difference formulas.[34] A notable special case occurs when AA and BB are complementary angles, satisfying A+B=π/2A + B = \pi/2. Substituting into the sine addition formula yields sin(π/2)=1=sinAcosB+cosAsinB\sin(\pi/2) = 1 = \sin A \cos B + \cos A \sin B, which, with B=π/2AB = \pi/2 - A, simplifies to sin2A+cos2A=1\sin^2 A + \cos^2 A = 1, confirming the Pythagorean identity.[35]

Multiple-Angle Formulas

Multiple-angle formulas express the trigonometric functions of multiple angles, such as 2θ, 3θ, or θ/2, in terms of functions of θ alone. These formulas are derived from the sum and difference formulas by substituting specific angles, enabling simplification of expressions involving repeated angles.[36]

Double-Angle Formulas

The double-angle formulas arise by applying the sum formulas with both angles equal to θ. For sine,
sin(2θ)=sin(θ+θ)=sinθcosθ+cosθsinθ=2sinθcosθ. \sin(2\theta) = \sin(\theta + \theta) = \sin \theta \cos \theta + \cos \theta \sin \theta = 2 \sin \theta \cos \theta.
This identity is fundamental for expanding products of sine and cosine.[36] For cosine, the derivation yields multiple equivalent forms:
cos(2θ)=cos(θ+θ)=cosθcosθsinθsinθ=cos2θsin2θ. \cos(2\theta) = \cos(\theta + \theta) = \cos \theta \cos \theta - \sin \theta \sin \theta = \cos^2 \theta - \sin^2 \theta.
Using the Pythagorean identity cos2θ+sin2θ=1\cos^2 \theta + \sin^2 \theta = 1, this can be rewritten as
cos(2θ)=2cos2θ1=12sin2θ. \cos(2\theta) = 2\cos^2 \theta - 1 = 1 - 2\sin^2 \theta.
The form 2cos2θ12\cos^2 \theta - 1 serves as a power-reduction formula, expressing cos2θ\cos^2 \theta as 1+cos(2θ)2\frac{1 + \cos(2\theta)}{2}, which reduces the power of the cosine in integrals or series expansions. Similarly, sin2θ=1cos(2θ)2\sin^2 \theta = \frac{1 - \cos(2\theta)}{2}. These power-reduction variants facilitate averaging over angles or simplifying polynomial expressions in trigonometry.[37][38]

Triple-Angle Formulas

Triple-angle formulas extend the double-angle results by adding another θ. For sine,
sin(3θ)=sin(2θ+θ)=sin(2θ)cosθ+cos(2θ)sinθ=2sinθcosθcosθ+(cos2θsin2θ)sinθ. \sin(3\theta) = \sin(2\theta + \theta) = \sin(2\theta) \cos \theta + \cos(2\theta) \sin \theta = 2 \sin \theta \cos \theta \cos \theta + (\cos^2 \theta - \sin^2 \theta) \sin \theta.
Simplifying further using cos2θ=1sin2θ\cos^2 \theta = 1 - \sin^2 \theta gives
sin(3θ)=3sinθ4sin3θ. \sin(3\theta) = 3 \sin \theta - 4 \sin^3 \theta.
This cubic form is particularly useful in solving equations like the triple-angle equation for sine, which relates to the geometry of trisecting angles.[39] A similar derivation for cosine yields cos(3θ)=4cos3θ3cosθ\cos(3\theta) = 4 \cos^3 \theta - 3 \cos \theta, though the focus here is on the sine variant as a direct extension.[39]

Half-Angle Formulas

Half-angle formulas solve for functions of θ/2 in terms of θ, derived by treating the double-angle formulas as equations in the half-angle. For sine, starting from cosθ=12sin2(θ/2)\cos \theta = 1 - 2 \sin^2(\theta/2), rearranging gives
sin2(θ/2)=1cosθ2, \sin^2(\theta/2) = \frac{1 - \cos \theta}{2},
so
sin(θ/2)=±1cosθ2. \sin(\theta/2) = \pm \sqrt{\frac{1 - \cos \theta}{2}}.
The sign depends on the quadrant of θ/2. This formula is essential for integrating expressions like 1cosθdθ\int \sqrt{1 - \cos \theta} \, d\theta or computing exact values for angles like 22.5°.[37] Analogously, from cosθ=2cos2(θ/2)1\cos \theta = 2 \cos^2(\theta/2) - 1,
cos(θ/2)=±1+cosθ2. \cos(\theta/2) = \pm \sqrt{\frac{1 + \cos \theta}{2}}.
These identities, along with the tangent half-angle formula tan(θ/2)=sinθ1+cosθ\tan(\theta/2) = \frac{\sin \theta}{1 + \cos \theta}, support substitutions in rational functions of sine and cosine.[38]

Differentiation and Integration Formulas

The derivatives of the basic trigonometric functions are fundamental results in calculus, assuming the argument is in radians. The derivative of the sine function is given by
ddxsinx=cosx, \frac{d}{dx} \sin x = \cos x,
while the derivative of the cosine function is
ddxcosx=sinx. \frac{d}{dx} \cos x = -\sin x.
These formulas can be derived using the limit definition of the derivative, relying on the standard limits limθ0sinθθ=1\lim_{\theta \to 0} \frac{\sin \theta}{\theta} = 1 and limθ01cosθθ=0\lim_{\theta \to 0} \frac{1 - \cos \theta}{\theta} = 0. For the tangent function, defined as tanx=sinxcosx\tan x = \frac{\sin x}{\cos x}, the derivative follows from the quotient rule:
ddxtanx=sec2x. \frac{d}{dx} \tan x = \sec^2 x.
This is obtained by differentiating the numerator and denominator separately and applying the quotient rule formula (uv)=uvuvv2\left( \frac{u}{v} \right)' = \frac{u' v - u v'}{v^2}, yielding cosxcosxsinx(sinx)cos2x=cos2x+sin2xcos2x=1cos2x=sec2x\frac{\cos x \cdot \cos x - \sin x \cdot (-\sin x)}{\cos^2 x} = \frac{\cos^2 x + \sin^2 x}{\cos^2 x} = \frac{1}{\cos^2 x} = \sec^2 x. Higher-order derivatives of sinx\sin x and cosx\cos x exhibit a cyclic pattern with period four. Specifically, the first derivative of sinx\sin x is cosx\cos x, the second is sinx-\sin x, the third is cosx-\cos x, and the fourth is sinx\sin x, after which the pattern repeats. Similarly, for cosx\cos x, the derivatives cycle as sinx-\sin x, cosx-\cos x, sinx\sin x, and cosx\cos x. This periodicity arises directly from repeated application of the basic derivative rules and is useful for computing nth-order derivatives without exhaustive differentiation. The indefinite integrals of the basic trigonometric functions are the antiderivatives, which reverse the differentiation process. Thus,
sinxdx=cosx+C, \int \sin x \, dx = -\cos x + C,
and
cosxdx=sinx+C. \int \cos x \, dx = \sin x + C.
For the tangent function, the integral is derived using the substitution u=cosxu = \cos x, so du=sinxdxdu = -\sin x \, dx and tanx=sinxcosx\tan x = \frac{\sin x}{\cos x}, leading to
tanxdx=sinxcosxdx=duu=lnu+C=lncosx+C, \int \tan x \, dx = \int \frac{\sin x}{\cos x} \, dx = -\int \frac{du}{u} = -\ln |u| + C = -\ln |\cos x| + C,
which is equivalent to lnsecx+C\ln |\sec x| + C. For integrals of powers of sine, such as sinnxdx\int \sin^n x \, dx where n>1n > 1 is an integer, a reduction formula allows recursive computation by lowering the power. The formula is
sinnxdx=sinn1xcosxn+n1nsinn2xdx. \int \sin^n x \, dx = -\frac{\sin^{n-1} x \cos x}{n} + \frac{n-1}{n} \int \sin^{n-2} x \, dx.
This is proved using integration by parts: let u=sinn1xu = \sin^{n-1} x and dv=sinxdxdv = \sin x \, dx, so du=(n1)sinn2xcosxdxdu = (n-1) \sin^{n-2} x \cos x \, dx and v=cosxv = -\cos x. Then, udv=uvvdu\int u \, dv = uv - \int v \, du yields the relation, which can be rearranged to the reduction form. Similar reduction formulas exist for powers of cosine and other trigonometric functions, facilitating evaluation of higher-power integrals.

Advanced Definitions

Power Series and Infinite Products

The power series expansions, also known as Maclaurin series, provide analytic definitions of the sine and cosine functions that are valid for all real numbers. These series arise from the repeated differentiation of the functions and evaluation at zero, reflecting their smooth, entire nature in the complex plane restricted to real arguments. The convergence radius is infinite, ensuring representation everywhere on the real line without singularities. The Taylor series for sine is given by
sinx=n=0(1)nx2n+1(2n+1)!=xx33!+x55!x77!+, \sin x = \sum_{n=0}^{\infty} \frac{(-1)^n x^{2n+1}}{(2n+1)!} = x - \frac{x^3}{3!} + \frac{x^5}{5!} - \frac{x^7}{7!} + \cdots,
which converges absolutely for all real xx. Similarly, the series for cosine is
cosx=n=0(1)nx2n(2n)!=1x22!+x44!x66!+, \cos x = \sum_{n=0}^{\infty} \frac{(-1)^n x^{2n}}{(2n)!} = 1 - \frac{x^2}{2!} + \frac{x^4}{4!} - \frac{x^6}{6!} + \cdots,
also converging for all real xx. These expansions encode the periodic and oscillatory behavior through alternating signs and factorial denominators that grow rapidly, enabling efficient computation for small to moderate x|x|. These series can be derived systematically by solving the second-order linear differential equation y+y=0y'' + y = 0, which both sine and cosine satisfy. Assume a power series solution y(x)=n=0anxny(x) = \sum_{n=0}^{\infty} a_n x^n. Differentiating twice and substituting yields the recurrence an+2=an/((n+1)(n+2))a_{n+2} = -a_n / ((n+1)(n+2)) for n0n \geq 0. For sine, the initial conditions y(0)=0y(0) = 0 and y(0)=1y'(0) = 1 fix a0=0a_0 = 0, a1=1a_1 = 1, producing only odd-powered terms. For cosine, y(0)=1y(0) = 1 and y(0)=0y'(0) = 0 yield a0=1a_0 = 1, a1=0a_1 = 0, resulting in even powers. This method confirms the coefficients without relying on geometric definitions. An alternative perspective on the series emerges from basic Fourier analysis, where sine and cosine serve as basis functions for expansions of periodic functions, and their own series align with the orthogonality properties over intervals like [π,π][-\pi, \pi]. The sine function also possesses an elegant infinite product representation, first derived by Leonhard Euler in 1748 by analogy to the factorization of polynomials. Considering sinx/x\sin x / x as an "infinite-degree polynomial" with zeros at x=±nπx = \pm n\pi for positive integers nn, Euler expressed it as
sinxx=n=1(1x2n2π2), \frac{\sin x}{x} = \prod_{n=1}^{\infty} \left(1 - \frac{x^2}{n^2 \pi^2}\right),
or equivalently,
sinx=xn=1(1x2n2π2). \sin x = x \prod_{n=1}^{\infty} \left(1 - \frac{x^2}{n^2 \pi^2}\right).
This product converges uniformly on compact subsets of the real line excluding the zeros at integer multiples of π\pi. The derivation involves comparing the Taylor series coefficients of the product to those of sinx/x\sin x / x, leveraging the known roots and leading coefficient to match the expansions term by term. This form highlights the function's zeros and connects to broader analytic number theory, such as evaluations of the Riemann zeta function at even integers.

Exponential and Complex Definitions

One of the most elegant ways to define the trigonometric functions sine and cosine analytically is through their relationship with the exponential function, particularly via Euler's formula, which states that for a real number θ\theta,
eiθ=cosθ+isinθ. e^{i\theta} = \cos \theta + i \sin \theta.
This formula links the exponential function with purely imaginary exponents to the trigonometric functions on the unit circle in the complex plane.[40] From this, the trigonometric functions can be expressed explicitly as
sinθ=eiθeiθ2i,cosθ=eiθ+eiθ2. \sin \theta = \frac{e^{i\theta} - e^{-i\theta}}{2i}, \quad \cos \theta = \frac{e^{i\theta} + e^{-i\theta}}{2}.
These definitions provide a unified view of sine and cosine as the imaginary and real parts, respectively, of the complex exponential eiθe^{i\theta}.[41] The exponential definitions extend naturally to complex arguments, allowing trigonometric functions to be defined for any complex number zz. Thus, the complex sine and cosine are given by
sinz=eizeiz2i,cosz=eiz+eiz2. \sin z = \frac{e^{iz} - e^{-iz}}{2i}, \quad \cos z = \frac{e^{iz} + e^{-iz}}{2}.
These functions are entire, meaning they are holomorphic everywhere in the complex plane, and they satisfy many of the same identities as their real counterparts, though with periodic strips rather than full periodicity.[42] A notable connection arises between these complex trigonometric functions and the hyperbolic functions, where the hyperbolic sine relates to the complex sine via sinhx=isin(ix)\sinh x = -i \sin(ix) for real xx. This relation highlights the analogy between trigonometric and hyperbolic functions through imaginary arguments.[43]

Differential and Integral Definitions

Trigonometric functions can be defined as the solutions to the second-order linear differential equation $ y'' + y = 0 $. The cosine function is the unique solution satisfying the initial conditions $ \cos 0 = 1 $ and $ \cos' 0 = 0 $, while the sine function is the unique solution satisfying $ \sin 0 = 0 $ and $ \sin' 0 = 1 $.[44] The general solution to this equation is a linear combination $ y(x) = A \cos x + B \sin x $, where the constants $ A $ and $ B $ are determined by the initial conditions.[44] The uniqueness of these solutions follows from the existence and uniqueness theorem for linear ordinary differential equations with continuous coefficients, which applies here since the coefficients are constants.[45] For the second-order equation, it can be rewritten as a first-order system $ \begin{cases} y' = z \ z' = -y \end{cases} $, to which the Picard–Lindelöf theorem applies, guaranteeing a unique solution on the real line given the Lipschitz condition on the right-hand side. An alternative definition uses integrals in a mutually recursive manner: $ \sin x = \int_0^x \cos t , dt $ and $ \cos x = 1 - \int_0^x \sin t , dt $. These definitions are consistent because differentiating them yields $ \cos x = \frac{d}{dx} \sin x $ and $ -\sin x = \frac{d}{dx} \cos x $, which imply that both functions satisfy the differential equation $ y'' + y = 0 $ with the appropriate initial conditions. This differential and integral approach parallels the definition of exponential functions as solutions to $ y' = y $, with sine and cosine emerging as the real and imaginary parts of the complex exponential $ e^{ix} $. Complex extensions of these definitions are explored further in exponential formulations.[44]

Functional Equation Definitions

Trigonometric functions can be axiomatized through functional equations that capture their additive properties, independent of geometric or analytic definitions. Consider real-valued functions SS and CC defined on R\mathbb{R} satisfying the Pythagorean identity S(x)2+C(x)2=1S(x)^2 + C(x)^2 = 1 for all xRx \in \mathbb{R}, along with initial conditions S(0)=0S(0) = 0 and C(0)=1C(0) = 1, and the additive relations
C(x+y)=C(x)C(y)S(x)S(y),S(x+y)=S(x)C(y)+C(x)S(y) C(x + y) = C(x)C(y) - S(x)S(y), \quad S(x + y) = S(x)C(y) + C(x)S(y)
for all x,yRx, y \in \mathbb{R}. These equations resemble a Cauchy-type addition formula tailored to the unit circle constraint. If SS or CC is continuous at a single point, then there exists a constant a0a \neq 0 such that C(x)=cos(ax)C(x) = \cos(ax) and S(x)=sin(ax)S(x) = \sin(ax) for all xRx \in \mathbb{R}.[46] The additive formula for sine specifically, S(x+y)=S(x)C(y)+C(x)S(y)S(x + y) = S(x)C(y) + C(x)S(y), extends the classical Cauchy functional equation f(x+y)=f(x)+f(y)f(x + y) = f(x) + f(y) by incorporating the auxiliary function CC, reflecting the interdependent nature of sine and cosine. Without continuity, pathological solutions exist using Hamel bases, but regularity conditions like continuity, monotonicity, or measurability guarantee uniqueness up to the scaling parameter aa. Analyticity further ensures the solutions are entire functions, aligning with their periodic behavior.[46] For cosine alone, d'Alembert's functional equation provides a standalone characterization: a function f:RRf: \mathbb{R} \to \mathbb{R} satisfies f(x+y)+f(xy)=2f(x)f(y)f(x + y) + f(x - y) = 2f(x)f(y) for all x,yRx, y \in \mathbb{R}, with f(0)=1f(0) = 1. Under continuity, the solutions are f(x)=cos(ax)f(x) = \cos(ax) for some constant aRa \in \mathbb{R}. This equation originates from studies in wave propagation and has been generalized to groups, where continuous solutions on R\mathbb{R} remain trigonometric. Boundedness or periodicity assumptions also yield the same uniqueness.[47] These functional equations connect to group theory, as the pair (C(x),S(x))(C(x), S(x)) represents a continuous group homomorphism from the additive group (R,+)(\mathbb{R}, +) to the special orthogonal group SO(2)SO(2), the group of 2D rotations, via the matrix (C(x)S(x)S(x)C(x))\begin{pmatrix} C(x) & -S(x) \\ S(x) & C(x) \end{pmatrix}. The kernel is 2πZ/a2\pi \mathbb{Z}/|a|, ensuring the covering map property. This perspective unifies the algebraic relations with the geometric interpretation of rotations.[48]

Inverse Functions

Definitions and Principal Values

The inverse trigonometric functions, also known as arcus functions, provide the angles whose trigonometric ratios equal a given value, reversing the action of the standard trigonometric functions. Due to the periodic nature of trigonometric functions, which results in multiple angles yielding the same ratio, these inverses are defined with specific restrictions on their ranges to ensure they are single-valued and bijective, producing a unique principal value for each input in their domain.[49][50] The arcsine function, denoted arcsin(y)\arcsin(y), is defined as the angle θ\theta such that sinθ=y\sin \theta = y and π/2θπ/2-\pi/2 \leq \theta \leq \pi/2. Its domain is the closed interval [1,1][-1, 1], corresponding to the range of the sine function over its principal interval. Similarly, the arccosine function, arccos(y)\arccos(y), satisfies cosθ=y\cos \theta = y with 0θπ0 \leq \theta \leq \pi, also defined on [1,1][-1, 1]. The arctangent function, arctan(y)\arctan(y), is the angle θ\theta where tanθ=y\tan \theta = y and π/2<θ<π/2-\pi/2 < \theta < \pi/2, with a domain of all real numbers R\mathbb{R}, reflecting the unbounded range of the tangent function in its principal interval.[49][50] These restrictions ensure bijectivity: the sine function is one-to-one and onto from [π/2,π/2][-\pi/2, \pi/2] to [1,1][-1, 1], the cosine from [0,π][0, \pi] to [1,1][-1, 1], and the tangent from (π/2,π/2)(-\pi/2, \pi/2) to R\mathbb{R}. The graph of arcsin(y)\arcsin(y) is an increasing S-shaped curve, symmetric about the origin, starting at (1,π/2)( -1, -\pi/2 ) and ending at (1,π/2)( 1, \pi/2 ). The graph of arccos(y)\arccos(y) decreases from (1,π)( -1, \pi ) to (1,0)( 1, 0 ), while arctan(y)\arctan(y) approaches π/2-\pi/2 as yy \to -\infty and π/2\pi/2 as yy \to \infty, passing through the origin.[49][51] Reciprocal inverse functions are defined analogously using the reciprocals of the trigonometric functions. The arcsecant, \arcsec(y)\arcsec(y), is the angle θ\theta such that secθ=y\sec \theta = y (or cosθ=1/y\cos \theta = 1/y) with 0θ<π/20 \leq \theta < \pi/2 or π/2<θπ\pi/2 < \theta \leq \pi, defined for y1y \leq -1 or y1y \geq 1. The arccosecant, \arccsc(y)\arccsc(y), satisfies cscθ=y\csc \theta = y (or sinθ=1/y\sin \theta = 1/y) with π/2θ<0-\pi/2 \leq \theta < 0 or 0<θπ/20 < \theta \leq \pi/2, also on y1y \leq -1 or y1y \geq 1. The arccotangent, \arccot(y)\arccot(y), is the angle θ\theta where cotθ=y\cot \theta = y (or tanθ=1/y\tan \theta = 1/y) with 0<θ<π0 < \theta < \pi, defined for all real yy. These ranges make the functions bijective over their respective domains, with graphs that are decreasing for \arcsec\arcsec and \arccsc\arccsc (except at discontinuities) and decreasing for \arccot\arccot.[49][52]

Properties and Identities

The inverse sine function, arcsin, is an odd function, satisfying arcsin(-x) = -arcsin(x) for all x in the domain [-1, 1].[53] This property follows from the oddness of the sine function and the principal branch definition of the inverse.[54] The derivatives of the principal inverse trigonometric functions are fundamental for calculus applications. The derivative of arcsin x is given by
ddxarcsinx=11x2,x<1. \frac{d}{dx} \arcsin x = \frac{1}{\sqrt{1 - x^2}}, \quad |x| < 1.
This result is obtained via implicit differentiation from the relation sin(y) = x, where y = arcsin x.[55] Similarly, the derivative of arctan x is
ddxarctanx=11+x2,xR. \frac{d}{dx} \arctan x = \frac{1}{1 + x^2}, \quad x \in \mathbb{R}.
This follows from implicit differentiation of tan(y) = x, yielding a secant expression that simplifies using the Pythagorean identity.[56] Key identities include the complementary property for arctangent: arctan x + arctan(1/x) = π/2 for x > 0.[57] For x < 0, the sum is -π/2, reflecting the odd nature of arctan.[58] More generally, the addition formula for arctangent states that
arctana+arctanb=arctan(a+b1ab) \arctan a + \arctan b = \arctan\left( \frac{a + b}{1 - ab} \right)
when ab < 1, with adjustments by ±π when ab > 1 to account for the principal range (-π/2, π/2).[58] This formula derives from the tangent addition rule applied to the angles whose tangents are a and b. Indefinite integrals involving these functions often yield inverse trigonometric expressions. For instance,
dx1x2=arcsinx+C,x<1. \int \frac{dx}{\sqrt{1 - x^2}} = \arcsin x + C, \quad |x| < 1.
This antiderivative is verified by differentiation, confirming its consistency with the arcsin derivative.[59] Similarly,
dx1+x2=arctanx+C,xR, \int \frac{dx}{1 + x^2} = \arctan x + C, \quad x \in \mathbb{R},
arising directly from the arctan derivative.[60] These integrals are essential in evaluating definite forms and solving differential equations.

Applications

Geometry and Triangles

Trigonometric functions are fundamentally applied in geometry to determine unknown angles and side lengths in right triangles, where the sine, cosine, and tangent ratios relate the sides opposite, adjacent to, and opposite over adjacent to a given acute angle, respectively. In a right triangle with acute angle θ, opposite side a, adjacent side b, and hypotenuse c, these are defined as sin θ = a/c, cos θ = b/c, and tan θ = a/b. To solve for missing elements, one can use these ratios inversely: for example, if the hypotenuse and an acute angle are known, the opposite side is found via a = c sin θ. Such applications allow computation of all sides and angles when at least one side and one acute angle (or two sides) are given, leveraging the Pythagorean theorem for verification.[61] For non-right triangles, the law of sines extends these ratios to relate all three sides and opposite angles: a / sin A = b / sin B = c / sin C = 2R, where R is the circumradius. This equality holds for any triangle and enables solving for unknown angles or sides when two angles and any side (AAS or ASA) or two sides and an angle opposite one of them (SSA) are known. However, the SSA case can be ambiguous, potentially yielding zero, one, or two triangles depending on the height relative to the given side and angle; specifically, if the given angle is acute and the opposite side is shorter than the adjacent side but longer than the adjacent side times the sine of the angle, two triangles may exist.[62][63] The law of cosines generalizes the Pythagorean theorem to any triangle, providing c² = a² + b² - 2ab cos C for the side opposite angle C, and cyclic permutations for the others. This formula is particularly useful for solving triangles when two sides and the included angle (SAS) or all three sides (SSS) are known, allowing computation of the opposite angle via the inverse cosine. It directly relates side lengths to the cosine of the included angle, facilitating solutions where the law of sines alone is insufficient.[64][65] A complementary relation, the law of tangents, connects differences and sums of sides to tangents of half-angles: (a - b) / (a + b) = tan((A - B)/2) / tan((A + B)/2). This identity, derived from the laws of sines and cosines, aids in solving for angles when sides are known, especially in cases involving half-angle computations, though it is less commonly used than the primary laws.[66] Trigonometric functions also provide a direct formula for the area of any triangle: (1/2)ab sin C, where a and b are two sides and C is the included angle. This expression, equivalent to (1/2)bc sin A or (1/2)ac sin B, derives from the height interpretation of the sine and is applicable even without knowing the third side, making it valuable for geometric computations.[67]

Calculus and Periodic Functions

Trigonometric functions play a central role in the analysis of periodic phenomena through Fourier series, which allow the representation of any sufficiently smooth periodic function as an infinite sum of sine and cosine terms. This decomposition exploits the orthogonality of these functions over one period, enabling the approximation of complex waveforms by superpositions of simpler harmonic components. The general form is $ f(x) = \frac{a_0}{2} + \sum_{n=1}^{\infty} (a_n \cos(nx) + b_n \sin(nx)) $, where the coefficients $ a_n $ and $ b_n $ are determined by integrals involving the function and the basis functions. This method, introduced by Joseph Fourier in his seminal work on heat conduction, revolutionized the study of periodic functions in mathematics.[68] In differential equations, trigonometric functions provide the natural solutions to second-order linear homogeneous equations modeling oscillatory behavior, such as the simple harmonic oscillator. The equation $ \frac{d^2x}{dt^2} + \omega^2 x = 0 $ has the general solution $ x(t) = A \cos(\omega t + \phi) $, where $ A $ is the amplitude and $ \phi $ is the phase shift, determined by initial conditions. This form arises from the characteristic equation $ r^2 + \omega^2 = 0 $, yielding complex roots $ r = \pm i\omega $, whose real and imaginary parts correspond to cosine and sine functions via Euler's formula. Such solutions highlight the periodic nature inherent in undamped oscillatory systems.[69] Trigonometric substitution is a powerful integration technique for handling integrals involving square roots of quadratic expressions, particularly those resembling trigonometric identities. For the integral $ \int \frac{dx}{\sqrt{x^2 + a^2}} $, the substitution $ x = a \tan \theta $ simplifies the expression, as $ \sqrt{x^2 + a^2} = a \sec \theta $ and $ dx = a \sec^2 \theta , d\theta $, leading to $ \int \sec \theta , d\theta = \ln |\sec \theta + \tan \theta| + C $. Back-substituting yields $ \sinh^{-1}(x/a) + C $ or equivalently $ \ln |x + \sqrt{x^2 + a^2}| + C $, demonstrating how trigonometric functions facilitate the evaluation of otherwise intractable integrals.[70] For small-angle approximations, the Taylor series expansions of sine and cosine provide essential simplifications in calculus applications. The series for $ \sin x $ is $ x - \frac{x^3}{3!} + \frac{x^5}{5!} - \cdots $, so for small $ x $, $ \sin x \approx x $; similarly, $ \cos x = 1 - \frac{x^2}{2!} + \frac{x^4}{4!} - \cdots \approx 1 - \frac{x^2}{2} $. These linear and quadratic approximations are derived by evaluating the function and its derivatives at zero, offering high accuracy for angles near zero radians and aiding in numerical computations and asymptotic analyses.[71]

Physics and Engineering

Trigonometric functions play a pivotal role in modeling dynamic systems across physics and engineering, where they describe periodic behaviors, resolve forces, and analyze signals in real-world applications. In physics, sine and cosine functions capture the oscillatory nature of phenomena like waves, while in engineering, they enable precise calculations for circuits and mechanical systems. These applications leverage the periodic properties of trigonometric functions to represent time-varying quantities accurately. In waves and oscillations, trigonometric functions model sinusoidal variations essential for understanding sound, light, and mechanical vibrations. For instance, the displacement in simple harmonic motion or a transverse wave is often expressed as $ y = A \sin(2\pi f t + \phi) $, where $ A $ is the amplitude, $ f $ is the frequency, $ t $ is time, and $ \phi $ is the phase angle; this form describes the periodic up-and-down motion in sound waves propagating through air or light waves in electromagnetic spectra.[72][73] Sound waves, for example, are modeled this way to predict pressure variations that the human ear perceives as pitch and volume, while light waves use similar sinusoidal profiles to explain interference patterns in optics.[74] Trigonometric functions are crucial for resolving vectors and forces in mechanics, particularly in projectile motion, where initial velocity components are decomposed using sine and cosine. The horizontal component is $ v_x = v \cos \theta $, and the vertical component is $ v_y = v \sin \theta $, with $ v $ as the launch speed and $ \theta $ as the angle relative to the horizontal; this allows engineers to predict trajectories for applications like ballistics or satellite launches.[75] In projectile motion under gravity, these components separate the motion into independent horizontal (constant velocity) and vertical (accelerated) parts, enabling calculations of range and maximum height without solving coupled equations.[76] In signal processing, the Fast Fourier Transform (FFT) relies on trigonometric functions to decompose complex signals into their frequency components, facilitating analysis in fields like audio engineering and telecommunications. The FFT computes the discrete Fourier transform efficiently, expressing a time-domain signal as a sum of sines and cosines at various frequencies, which reveals dominant periodic elements in noisy data.[77] This technique is widely used to filter signals or identify vibrations in machinery, transforming raw sensor data into interpretable spectra for fault detection.[78] Electrical engineering employs trigonometric functions to analyze alternating current (AC) circuits, where phase shifts between voltage and current are quantified using tangent. In a resistive-inductive (RL) circuit, the phase angle $ \phi $ satisfies $ \tan \phi = X_L / R $, with $ X_L $ as inductive reactance and $ R $ as resistance; this determines power factor and efficiency in power distribution systems.[79] Similarly, in RC circuits, $ \tan \phi = -X_C / R $ accounts for capacitive effects, guiding the design of filters and oscillators in electronics.[80]

Historical and Linguistic Aspects

Historical Development

The origins of trigonometric functions trace back to ancient astronomy and geometry, where early mathematicians developed tables to solve practical problems in celestial navigation and measurement. In the 2nd century BCE, the Greek astronomer Hipparchus compiled the first known tables of chords, which measured the length of a chord subtending an angle in a circle of fixed radius, laying the foundational work for what would become trigonometry.[3] These tables, though not surviving intact, influenced subsequent Hellenistic and later traditions by providing a systematic approach to angular calculations. The Alexandrian astronomer Ptolemy (c. 100–170 CE) advanced this by establishing key identities, such as the Pythagorean theorem in trigonometric form (sin²θ + cos²θ = 1, expressed in chords), and providing an equivalent of the law of sines: a / sin A = b / sin B = c / sin C.[3] Around 500 CE, the Indian mathematician Aryabhata advanced this further by introducing the sine function, denoted as "jya" (meaning chord), and computing sine tables for astronomical purposes in his text Aryabhatiya, marking the first explicit use of sine as a distinct trigonometric ratio.[3] During the Islamic Golden Age (8th–13th centuries CE), scholars refined and expanded trigonometric methods, integrating Greek and Indian knowledge with original innovations driven by advancements in astronomy. Al-Battani (c. 858–929 CE), a prominent astronomer from Mesopotamia, produced highly accurate sine tables and was the first to express trigonometric functions as lengths rather than proportions, while also contributing to spherical trigonometry by refining Ptolemaic models for planetary motion.[81][82] In the 9th–10th centuries, Islamic mathematicians introduced the tangent function, initially conceptualized as the "extended shadow" (the shadow cast by a horizontal rod on a vertical wall), which Al-Battani employed in his calculations; this was later formalized by Al-Biruni (973–1048 CE) alongside the cotangent.[81] Abu al-Wafa (940–998 CE) further derived addition formulas, including the double-angle identity sin(2x) = 2 sin(x) cos(x).[3] The European Renaissance (15th–16th centuries) saw the revival and systematization of trigonometry as a standalone mathematical discipline, spurred by printing technology and astronomical needs. Regiomontanus (Johannes Müller, 1436–1476) authored De triangulis omnimodis around 1464 (published 1533), the first comprehensive European treatise on trigonometry, which emphasized sines and their inverses in plane and spherical contexts, drawing from Islamic sources like Jabir ibn Aflah.[83] His student Georg Rheticus (1514–1574) advanced computational aspects in 1542 by publishing extensive tables of sines and cosines to 10 decimal places, defining functions geometrically in terms of right triangles with unit hypotenuse, and assisting in the trigonometric sections of Copernicus's De revolutionibus.[3] In the 18th century, Leonhard Euler (1707–1783) propelled trigonometric functions into analytic mathematics by treating sine, cosine, and others as standalone functions rather than geometric ratios, introducing key identities and the complex exponential representation in his Introductio in analysin infinitorum (1748).[84] In the 19th and early 20th centuries, trigonometric functions gained deeper theoretical foundations through complex analysis and series expansions. Joseph Fourier (1768–1830) revolutionized their application in the 1820s by developing Fourier series, which decompose arbitrary periodic functions into infinite sums of sines and cosines, as detailed in his Théorie analytique de la chaleur (1822) while solving the heat equation.[85] Bernhard Riemann (1826–1866) extended this in his 1854 habilitation dissertation by investigating the conditions under which functions could be represented by trigonometric series, linking them to integrability and complex variable theory, thereby bridging Fourier analysis with Riemann surfaces and holomorphic functions.[86]

Etymology

The term "sine" originates from the Latin sinus, meaning "a bend, curve, fold in a garment, or bosom," which entered mathematical usage in the mid-12th century through Gherardo of Cremona's Medieval Latin translation of Arabic geometrical texts.[87] The Arabic jiba, denoting the "chord of an arc" or sine, derived from the Sanskrit jya ("bowstring"), but was mistranslated from jaib ("pocket" or "bosom"), leading to the adoption of sinus as a fitting equivalent due to its connotation of a fold or inlet.[87] This linguistic path reflects the transmission of trigonometric concepts from Indian astronomy through Arabic scholarship to Europe, where the term first appeared in English in the 1590s.[87] The name "cosine," introduced in the 1630s, is a contraction of "co. sinus," abbreviating the Medieval Latin complementi sinus ("sine of the complement").[88] Here, the prefix "co-" stems from Latin complementum ("that which fills up or completes"), referring to the complementary angle in a right triangle, as the cosine of an angle equals the sine of its complement (90° minus the angle).[88] This nomenclature, popularized by English mathematician Edmund Gunter around 1620, underscores the relational symmetry between sine and cosine in early trigonometric tables and calculations.[88] "Tangent" derives from the Latin tangentem (nominative tangens), the present participle of tangere ("to touch"), introduced as a trigonometric term in 1583 by Danish mathematician Thomas Fincke in his work Geometria Rotundi.[89] The name evokes the geometric construction where the tangent represents the length of a line from the origin touching the unit circle at one point, emphasizing contact without crossing.[89] Similarly, "cotangent," a 17th-century contraction of "co. tangent," applies the "co-" prefix to denote the tangent of the complementary angle, mirroring the structure of cosine.[90] The terms "secant" and "cosecant" trace to Latin secantem (nominative secans), from secare ("to cut"), also coined by Fincke in 1583 to describe a line intersecting a circle at two points.[91] "Cosecant," analogously, combines the "co-" prefix with secant, signifying the secant of the complementary angle.[91] "Cotangent," as noted, follows the same complementary pattern with tangent. These names, rooted in classical Latin geometry, highlight the functions' roles as reciprocals of cosine and sine, respectively, in extending basic ratios beyond the unit circle.[90]

References

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