# Sine

In mathematics, the sine is a trigonometric function of an angle. The sine of an acute angle is defined in the context of a right triangle: for the specified angle, it is the ratio of the length of the side that is opposite that angle to the length of the longest side of the triangle (the hypotenuse).

Sine
Basic features
Parity odd
Domain (−, +) a
Codomain [−1, 1] a
Period 2π

Specific values
At zero 0
Maxima (2kπ + π/2, 1)b
Minima (2kππ/2, −1)

Specific features
Root kπ
Critical point kπ + π/2
Inflection point kπ
Fixed point 0

More generally, the definition of sine (and other trigonometric functions) can be extended to any real value in terms of the length of a certain line segment in a unit circle. More modern definitions express the sine as an infinite series or as the solution of certain differential equations, allowing their extension to arbitrary positive and negative values and even to complex numbers.

The sine function is commonly used to model periodic phenomena such as sound and light waves, the position and velocity of harmonic oscillators, sunlight intensity and day length, and average temperature variations throughout the year.

The function sine can be traced to the jyā and koṭi-jyā functions used in Gupta period Indian astronomy (Aryabhatiya, Surya Siddhanta), via translation from Sanskrit to Arabic and then from Arabic to Latin.[1] The word "sine" comes from a Latin mistranslation of the Arabic jiba, which is a transliteration of the Sanskrit word for half the chord, jya-ardha.[2]

## Right-angled triangle definitionEdit

For the angle α, the sine function gives the ratio of the length of the opposite side to the length of the hypotenuse.

To define the sine function of an acute angle α, start with a right triangle that contains an angle of measure α; in the accompanying figure, angle A in triangle ABC is the angle of interest. The three sides of the triangle are named as follows:

• The opposite side is the side opposite to the angle of interest, in this case side a.
• The hypotenuse is the side opposite the right angle, in this case side h. The hypotenuse is always the longest side of a right-angled triangle.
• The adjacent side is the remaining side, in this case side b. It forms a side of (is adjacent to) both the angle of interest (angle A) and the right angle.

Once such a triangle is chosen, the sine of the angle is equal to the length of the opposite side divided by the length of the hypotenuse, or:

${\displaystyle \sin(\alpha )={\frac {\textrm {opposite}}{\textrm {hypotenuse}}}}$

The other trigonometric functions of the angle can be defined similarly; for example, the cosine of the angle is the ratio between the adjacent side and the hypotenuse, while the tangent gives the ratio between the opposite and adjacent sides.

As stated, the value ${\displaystyle \sin(\alpha )}$  appears to depend on the choice of right triangle containing an angle of measure α. However, this is not the case: all such triangles are similar, and so the ratio is the same for each of them.

## Unit circle definitionEdit

Illustration of a unit circle. The radius has a length of 1. The variable t is an angle measure.

In trigonometry, a unit circle is the circle of radius one centered at the origin (0, 0) in the Cartesian coordinate system.

Let a line through the origin, making an angle of θ with the positive half of the x-axis, intersect the unit circle. The x- and y-coordinates of this point of intersection are equal to cos(θ) and sin(θ), respectively. The point's distance from the origin is always 1.

Unlike the definitions with the right triangle or slope, the angle can be extended to the full set of real arguments by using the unit circle. This can also be achieved by requiring certain symmetries and that sine be a periodic function.

Animation showing how the sine function (in red) ${\displaystyle y=\sin(\theta )}$  is graphed from the y-coordinate (red dot) of a point on the unit circle (in green) at an angle of θ.

## IdentitiesEdit

These apply for all values of ${\displaystyle \theta }$ .

${\displaystyle \sin(\theta )=\cos \left({\frac {\pi }{2}}-\theta \right)={\frac {1}{\csc(\theta )}}}$

### ReciprocalEdit

The reciprocal of sine is cosecant, i.e., the reciprocal of sin(A) is csc(A), or cosec(A). Cosecant gives the ratio of the length of the hypotenuse to the length of the opposite side:

${\displaystyle \csc(A)={\frac {1}{\sin(A)}}={\frac {\textrm {hypotenuse}}{\textrm {opposite}}}={\frac {h}{a}}.}$

### InverseEdit

The usual principal values of the arcsin(x) function graphed on the cartesian plane. Arcsin is the inverse of sin.

The inverse function of sine is arcsine (arcsin or asin) or inverse sine (sin-1). As sine is non-injective, it is not an exact inverse function but a partial inverse function. For example, sin(0) = 0, but also sin(π) = 0, sin(2π) = 0 etc. It follows that the arcsine function is multivalued: arcsin(0) = 0, but also arcsin(0) = π, arcsin(0) = 2π, etc. When only one value is desired, the function may be restricted to its principal branch. With this restriction, for each x in the domain the expression arcsin(x) will evaluate only to a single value, called its principal value.

${\displaystyle \theta =\arcsin \left({\frac {\text{opposite}}{\text{hypotenuse}}}\right)=\sin ^{-1}\left({\frac {a}{h}}\right).}$

k is some integer:

{\displaystyle {\begin{aligned}\sin(y)=x\Leftrightarrow &y=\arcsin(x)+2\pi k,{\text{ or }}\\&y=\pi -\arcsin(x)+2\pi k\end{aligned}}}

Or in one equation:

${\displaystyle \sin(y)=x\Leftrightarrow y=(-1)^{k}\arcsin(x)+\pi k}$

Arcsin satisfies:

${\displaystyle \sin(\arcsin(x))=x\!}$

and

${\displaystyle \arcsin(\sin(\theta ))=\theta \quad {\text{for }}-{\frac {\pi }{2}}\leq \theta \leq {\frac {\pi }{2}}.}$

### CalculusEdit

For the sine function:

${\displaystyle f(x)=\sin(x)}$

The derivative is:

${\displaystyle f'(x)=\cos(x)}$

The antiderivative is:

${\displaystyle \int f(x)\,dx=-\cos(x)+C}$

C denotes the constant of integration.

### Other trigonometric functionsEdit

The sine and cosine functions are related in multiple ways. The two functions are out of phase by 90°: ${\displaystyle \sin(\pi /2-x)}$  = ${\displaystyle \cos(x)}$  for all angles x. Also, the derivative of the function sin(x) is cos(x).

It is possible to express any trigonometric function in terms of any other (up to a plus or minus sign, or using the sign function).

Sine in terms of the other common trigonometric functions:

f θ Using plus/minus (±) Using sign function (sgn)
f θ = ± per Quadrant f θ =
I II III IV
cos ${\displaystyle \sin(\theta )}$  ${\displaystyle =\pm {\sqrt {1-\cos ^{2}(\theta )}}}$  + + ${\displaystyle =\operatorname {sgn} \left(\cos \left(\theta -{\frac {\pi }{2}}\right)\right){\sqrt {1-\cos ^{2}(\theta )}}}$
${\displaystyle \cos(\theta )}$  ${\displaystyle =\pm {\sqrt {1-\sin ^{2}(\theta )}}}$  + + ${\displaystyle =\operatorname {sgn} \left(\sin \left(\theta +{\frac {\pi }{2}}\right)\right){\sqrt {1-\sin ^{2}(\theta )}}}$
cot ${\displaystyle \sin(\theta )}$  ${\displaystyle =\pm {\frac {1}{\sqrt {1+\cot ^{2}(\theta )}}}}$  + + ${\displaystyle =\operatorname {sgn} \left(\cot \left({\frac {\theta }{2}}\right)\right){\frac {1}{\sqrt {1+\cot ^{2}(\theta )}}}}$
${\displaystyle \cot(\theta )}$  ${\displaystyle =\pm {\frac {\sqrt {1-\sin ^{2}(\theta )}}{\sin(\theta )}}}$  + + ${\displaystyle =\operatorname {sgn} \left(\sin \left(\theta +{\frac {\pi }{2}}\right)\right){\frac {\sqrt {1-\sin ^{2}(\theta )}}{\sin(\theta )}}}$
tan ${\displaystyle \sin(\theta )}$  ${\displaystyle =\pm {\frac {\tan(\theta )}{\sqrt {1+\tan ^{2}(\theta )}}}}$  + + ${\displaystyle =\operatorname {sgn} \left(\tan \left({\frac {2\theta +\pi }{4}}\right)\right){\frac {\tan(\theta )}{\sqrt {1+\tan ^{2}(\theta )}}}}$
${\displaystyle \tan(\theta )}$  ${\displaystyle =\pm {\frac {\sin(\theta )}{\sqrt {1-\sin ^{2}(\theta )}}}}$  + + ${\displaystyle =\operatorname {sgn} \left(\sin \left(\theta +{\frac {\pi }{2}}\right)\right){\frac {\sin(\theta )}{\sqrt {1-\sin ^{2}(\theta )}}}}$
sec ${\displaystyle \sin(\theta )}$  ${\displaystyle =\pm {\frac {\sqrt {\sec ^{2}(\theta )-1}}{\sec(\theta )}}}$  + + ${\displaystyle =\operatorname {sgn} \left(\sec \left({\frac {4\theta -\pi }{2}}\right)\right){\frac {\sqrt {\sec ^{2}(\theta )-1}}{\sec(\theta )}}}$
${\displaystyle \sec(\theta )}$  ${\displaystyle =\pm {\frac {1}{\sqrt {1-\sin ^{2}(\theta )}}}}$  + + ${\displaystyle =\operatorname {sgn} \left(\sin \left(\theta +{\frac {\pi }{2}}\right)\right){\frac {1}{\sqrt {1-\sin ^{2}(\theta )}}}}$

Note that for all equations which use plus/minus (±), the result is positive for angles in the first quadrant.

The basic relationship between the sine and the cosine can also be expressed as the Pythagorean trigonometric identity:

${\displaystyle \cos ^{2}(\theta )+\sin ^{2}(\theta )=1\!}$

where sin2(x) means (sin(x))2.

## Properties relating to the quadrantsEdit

The four quadrants of a Cartesian coordinate system.

The table below displays many of the key properties of the sine function (sign, monotonicity, convexity), arranged by the quadrant of the argument. For arguments outside those in the table, one may compute the corresponding information by using the periodicity ${\displaystyle \sin(\alpha +360^{\circ })=\sin(\alpha )}$  of the sine function.

1st Quadrant ${\displaystyle 0^{\circ }  ${\displaystyle 0  ${\displaystyle 0<\sin(x)<1}$  ${\displaystyle +}$  increasing concave
2nd Quadrant ${\displaystyle 90^{\circ }  ${\displaystyle {\frac {\pi }{2}}  ${\displaystyle 0<\sin(x)<1}$  ${\displaystyle +}$  decreasing concave
3rd Quadrant ${\displaystyle 180^{\circ }  ${\displaystyle \pi   ${\displaystyle -1<\sin(x)<0}$  ${\displaystyle -}$  decreasing convex
4th Quadrant ${\displaystyle 270^{\circ }  ${\displaystyle {\frac {3\pi }{2}}  ${\displaystyle -1<\sin(x)<0}$  ${\displaystyle -}$  increasing convex

The quadrants of the unit circle and of sin(x), using the Cartesian coordinate system.

The following table gives basic information at the boundary of the quadrants.

Degrees Radians ${\displaystyle \sin(x)}$  Point type
${\displaystyle 0^{\circ }}$  ${\displaystyle 0}$  ${\displaystyle 0}$  Root, Inflection
${\displaystyle 90^{\circ }}$  ${\displaystyle {\frac {\pi }{2}}}$  ${\displaystyle 1}$  Maximum
${\displaystyle 180^{\circ }}$  ${\displaystyle \pi }$  ${\displaystyle 0}$  Root, Inflection
${\displaystyle 270^{\circ }}$  ${\displaystyle {\frac {3\pi }{2}}}$  ${\displaystyle -1}$  Minimum

## Series definitionEdit

The sine function (blue) is closely approximated by its Taylor polynomial of degree 7 (pink) for a full cycle centered on the origin.

This animation shows how including more and more terms in the partial sum of its Taylor series approaches a sine curve.

Using only geometry and properties of limits, it can be shown that the derivative of sine is cosine, and that the derivative of cosine is the negative of sine.

Using the reflection from the calculated geometric derivation of the sine is with the 4n + k-th derivative at the point 0:

${\displaystyle \sin ^{(4n+k)}(0)={\begin{cases}0&{\text{when }}k=0\\1&{\text{when }}k=1\\0&{\text{when }}k=2\\-1&{\text{when }}k=3\end{cases}}}$

This gives the following Taylor series expansion at x = 0. One can then use the theory of Taylor series to show that the following identities hold for all real numbers x (where x is the angle in radians) :[3]

{\displaystyle {\begin{aligned}\sin(x)&=x-{\frac {x^{3}}{3!}}+{\frac {x^{5}}{5!}}-{\frac {x^{7}}{7!}}+\cdots \\[8pt]&=\sum _{n=0}^{\infty }{\frac {(-1)^{n}}{(2n+1)!}}x^{2n+1}\\[8pt]\end{aligned}}}

If x were expressed in degrees then the series would contain factors involving powers of π/180: if x is the number of degrees, the number of radians is y = πx /180, so

{\displaystyle {\begin{aligned}\sin(x_{\mathrm {deg} })&=\sin(y_{\mathrm {rad} })\\&={\frac {\pi }{180}}x-\left({\frac {\pi }{180}}\right)^{3}{\frac {x^{3}}{3!}}+\left({\frac {\pi }{180}}\right)^{5}{\frac {x^{5}}{5!}}-\left({\frac {\pi }{180}}\right)^{7}{\frac {x^{7}}{7!}}+\cdots .\end{aligned}}}

The series formulas for the sine and cosine are uniquely determined, up to the choice of unit for angles, by the requirements that

{\displaystyle {\begin{aligned}\sin(0)=0&{\text{ and }}\sin(2x)=2\sin(x)\cos(x)\\\cos ^{2}(x)+\sin ^{2}(x)=1&{\text{ and }}\cos(2x)=\cos ^{2}(x)-\sin ^{2}(x)\\\end{aligned}}}

The radian is the unit that leads to the expansion with leading coefficient 1 for the sine and is determined by the additional requirement that

${\displaystyle \sin(x)\approx x{\text{ when }}x\approx 0.}$

The coefficients for both the sine and cosine series may therefore be derived by substituting their expansions into the pythagorean and double angle identities, taking the leading coefficient for the sine to be 1, and matching the remaining coefficients.

In general, mathematically important relationships between the sine and cosine functions and the exponential function (see, for example, Euler's formula) are substantially simplified when angles are expressed in radians, rather than in degrees, grads or other units. Therefore, in most branches of mathematics beyond practical geometry, angles are generally assumed to be expressed in radians.

A similar series is Gregory's series for arctan, which is obtained by omitting the factorials in the denominator.

### Continued fractionEdit

The sine function can also be represented as a generalized continued fraction:

${\displaystyle \sin(x)={\cfrac {x}{1+{\cfrac {x^{2}}{2\cdot 3-x^{2}+{\cfrac {2\cdot 3x^{2}}{4\cdot 5-x^{2}+{\cfrac {4\cdot 5x^{2}}{6\cdot 7-x^{2}+\ddots }}}}}}}}.}$

The continued fraction representation can be derived from Euler's continued fraction formula and expresses the real number values, both rational and irrational, of the sine function.

## Fixed pointEdit

The fixed point iteration xn+1 = sin(xn) with initial value x0 = 2 converges to 0.

Zero is the only real fixed point of the sine function; in other words the only intersection of the sine function and the identity function is sin(0) = 0.

## Arc lengthEdit

The arc length of the sine curve between ${\displaystyle a}$  and ${\displaystyle b}$  is ${\displaystyle \int _{a}^{b}\!{\sqrt {1+\cos ^{2}(x)}}\,dx}$  This integral is an elliptic integral of the second kind.

The arc length for a full period is ${\displaystyle {\frac {4{\sqrt {2\pi ^{3}}}}{\Gamma (1/4)^{2}}}+{\frac {\Gamma (1/4)^{2}}{\sqrt {2\pi }}}=7.640395578\ldots }$  where ${\displaystyle \Gamma }$  is the Gamma function.

The arc length of the sine curve from 0 to x is the above number divided by ${\displaystyle 2\pi }$  times x, plus a correction that varies periodically in x with period ${\displaystyle \pi }$ . The Fourier series for this correction can be written in closed form using special functions, but it is perhaps more instructive to write the decimal approximations of the Fourier coefficients. The sine curve arc length from 0 to x is

${\displaystyle 1.21600672x+0.10317093\sin(2x)-0.00220445\sin(4x)+0.00012584\sin(6x)-0.00001011\sin(8x)+\cdots }$

## Law of sinesEdit

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:

${\displaystyle {\frac {\sin A}{a}}={\frac {\sin B}{b}}={\frac {\sin C}{c}}.}$

This is equivalent to the equality of the first three expressions below:

${\displaystyle {\frac {a}{\sin A}}={\frac {b}{\sin B}}={\frac {c}{\sin C}}=2R,}$

where R is the triangle's circumradius.

It can be proven 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.

## Special valuesEdit

Some common angles (θ) shown on the unit circle. The angles are given in degrees and radians, together with the corresponding intersection point on the unit circle, (cos(θ), sin(θ)).

For certain integral numbers x of degrees, the value of sin(x) is particularly simple. A table of some of these values is given below.

x (angle) sin(x)
0 0g 0 0 0
180° π 200g 1/2
15° 1/12π 16 2/3g 1/24 ${\displaystyle {\frac {{\sqrt {6}}-{\sqrt {2}}}{4}}}$  0.258819045102521
165° 11/12π 183 1/3g 11/24
30° 1/6π 33 1/3g 1/12 1/2 0.5
150° 5/6π 166 2/3g 5/12
45° 1/4π 50g 1/8 ${\displaystyle {\frac {\sqrt {2}}{2}}}$  0.707106781186548
135° 3/4π 150g 3/8
60° 1/3π 66 2/3g 1/6 ${\displaystyle {\frac {\sqrt {3}}{2}}}$  0.866025403784439
120° 2/3π 133 1/3g 1/3
75° 5/12π 83 1/3g 5/24 ${\displaystyle {\frac {{\sqrt {6}}+{\sqrt {2}}}{4}}}$  0.965925826289068
105° 7/12π 116 2/3g 7/24
90° 1/2π 100g 1/4 1 1

90 degree increments:

 x in degrees 0° 90° 180° 270° 360° x in radians 0 π/2 π 3π/2 2π x in gons 0 100g 200g 300g 400g x in turns 0 1/4 1/2 3/4 1 sin x 0 1 0 -1 0

Other values not listed above:

${\displaystyle \sin({\frac {\pi }{60}})=\sin(3^{\circ })={\frac {(2-{\sqrt {12}}){\sqrt {5+{\sqrt {5}}}}+({\sqrt {10}}-{\sqrt {2}})({\sqrt {3}}+1)}{16}}}$
${\displaystyle \sin({\frac {\pi }{30}})=\sin(6^{\circ })={\frac {{\sqrt {30-{\sqrt {180}}}}-{\sqrt {5}}-1}{8}}}$
${\displaystyle \sin({\frac {\pi }{20}})=\sin(9^{\circ })={\frac {{\sqrt {10}}+{\sqrt {2}}-{\sqrt {20-{\sqrt {80}}}}}{8}}}$
${\displaystyle \sin({\frac {\pi }{15}})=\sin(12^{\circ })={\frac {{\sqrt {10+{\sqrt {20}}}}+{\sqrt {3}}-{\sqrt {15}}}{8}}}$
${\displaystyle \sin({\frac {\pi }{10}})=\sin(18^{\circ })={\frac {{\sqrt {5}}-1}{4}}={\tfrac {1}{2}}\varphi ^{-1}}$
${\displaystyle \sin({\frac {7\pi }{60}})=\sin(21^{\circ })={\frac {(2+{\sqrt {12}}){\sqrt {5-{\sqrt {5}}}}-({\sqrt {10}}+{\sqrt {2}})({\sqrt {3}}-1)}{16}}}$
${\displaystyle \sin({\frac {\pi }{8}})=\sin(22.5^{\circ })={\frac {\sqrt {2-{\sqrt {2}}}}{2}}}$
${\displaystyle \sin({\frac {2\pi }{15}})=\sin(24^{\circ })={\frac {{\sqrt {3}}+{\sqrt {15}}-{\sqrt {10-{\sqrt {20}}}}}{8}}}$
${\displaystyle \sin({\frac {3\pi }{20}})=\sin(27^{\circ })={\frac {{\sqrt {20+{\sqrt {80}}}}-{\sqrt {10}}+{\sqrt {2}}}{8}}}$
${\displaystyle \sin({\frac {11\pi }{60}})=\sin(33^{\circ })={\frac {({\sqrt {12}}-2){\sqrt {5+{\sqrt {5}}}}+({\sqrt {10}}-{\sqrt {2}})({\sqrt {3}}+1)}{16}}}$
${\displaystyle \sin({\frac {\pi }{5}})=\sin(36^{\circ })={\frac {\sqrt {10-{\sqrt {20}}}}{4}}}$
${\displaystyle \sin({\frac {13\pi }{60}})=\sin(39^{\circ })={\frac {(2-{\sqrt {12}}){\sqrt {5-{\sqrt {5}}}}+({\sqrt {10}}+{\sqrt {2}})({\sqrt {3}}+1)}{16}}}$
${\displaystyle \sin({\frac {7\pi }{30}})=\sin(42^{\circ })={\frac {{\sqrt {30+{\sqrt {180}}}}-{\sqrt {5}}+1}{8}}}$

## Relationship to complex numbersEdit

An illustration of the complex plane. The imaginary numbers are on the vertical coordinate axis.

Sine is used to determine the imaginary part of a complex number given in polar coordinates (r, φ):

${\displaystyle z=r(\cos(\varphi )+i\sin(\varphi ))}$

the imaginary part is:

${\displaystyle \operatorname {Im} (z)=r\sin(\varphi )}$

r and φ represent the magnitude and angle of the complex number respectively. i is the imaginary unit. z is a complex number.

Although dealing with complex numbers, sine's parameter in this usage is still a real number. Sine can also take a complex number as an argument.

### Sine with a complex argumentEdit

${\displaystyle \sin(z)}$

Domain coloring of sin(z) over (-π, π) on x- and y-axes. Brightness indicates absolute magnitude, saturation represents complex argument.

sin(z) as a vector field

${\displaystyle \sin(\theta )}$  is the imaginary part of ${\displaystyle \mathrm {e} ^{\mathrm {i} \theta }}$ .

The definition of the sine function for complex arguments z:

{\displaystyle {\begin{aligned}\sin(z)&=\sum _{n=0}^{\infty }{\frac {(-1)^{n}}{(2n+1)!}}z^{2n+1}\\&={\frac {e^{iz}-e^{-iz}}{2i}}\\&={\frac {\sinh \left(iz\right)}{i}}\end{aligned}}}

where i 2 = −1, and sinh is hyperbolic sine. This is an entire function. Also, for purely real x,

${\displaystyle \sin(x)=\operatorname {Im} (e^{ix}).}$

For purely imaginary numbers:

${\displaystyle \sin(iy)=i\sinh(y).}$

It is also sometimes useful to express the complex sine function in terms of the real and imaginary parts of its argument:

{\displaystyle {\begin{aligned}\sin(x+iy)&=\sin(x)\cos(iy)+\cos(x)\sin(iy)\\&=\sin(x)\cosh(y)+i\cos(x)\sinh(y).\end{aligned}}}

#### Partial fraction and product expansions of complex sineEdit

Using the partial fraction expansion technique in complex analysis, one can find that the infinite series

{\displaystyle {\begin{aligned}\sum _{n=-\infty }^{\infty }{\frac {(-1)^{n}}{z-n}}={\frac {1}{z}}-2z\sum _{n=1}^{\infty }{\frac {(-1)^{n}}{n^{2}-z^{2}}}\end{aligned}}}

both converge and are equal to ${\displaystyle {\frac {\pi }{\sin \pi z}}}$ . Similarly, one can show that

{\displaystyle {\begin{aligned}{\frac {\pi ^{2}}{\sin ^{2}(\pi z)}}=\sum _{n=-\infty }^{\infty }{\frac {1}{(z-n)^{2}}}.\end{aligned}}}

Using product expansion technique, one can derive

{\displaystyle {\begin{aligned}\sin(\pi z)=\pi z\prod _{n=1}^{\infty }{\Bigl (}1-{\frac {z^{2}}{n^{2}}}{\Bigr )}.\end{aligned}}}

#### Usage of complex sineEdit

sin(z) is found in the functional equation for the Gamma function,

${\displaystyle \Gamma (s)\Gamma (1-s)={\pi \over \sin(\pi s)},}$

which in turn is found in the functional equation for the Riemann zeta-function,

${\displaystyle \zeta (s)=2(2\pi )^{s-1}\Gamma (1-s)\sin(\pi s/2)\zeta (1-s).}$

As a holomorphic function, sin z is a 2D solution of Laplace's equation:

${\displaystyle \Delta u(x_{1},x_{2})=0.}$

It is also related with level curves of pendulum.[4]

### Complex graphsEdit

 real component imaginary component magnitude

 real component imaginary component magnitude

## HistoryEdit

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 discovered by Hipparchus of Nicaea (180–125 BCE) and Ptolemy of Roman Egypt (90–165 CE).

The function sine (and cosine) can be traced to the jyā and koṭi-jyā functions used in Gupta period (320 to 550 CE) Indian astronomy (Aryabhatiya, Surya Siddhanta), via translation from Sanskrit to Arabic and then from Arabic to Latin.[1]

The first published use of the abbreviations 'sin', 'cos', and 'tan' is by the 16th century French mathematician Albert Girard; these were further promulgated by Euler (see below). The Opus palatinum de triangulis of Georg Joachim Rheticus, a student of Copernicus, was probably the first in Europe to define trigonometric functions directly in terms of right triangles instead of circles, with tables for all six trigonometric functions; this work was finished by Rheticus' student Valentin Otho in 1596.

In a paper published in 1682, Leibniz proved that sin x is not an algebraic function of x.[5] Roger Cotes computed the derivative of sine in his Harmonia Mensurarum (1722).[6] Leonhard Euler's Introductio in analysin infinitorum (1748) was mostly responsible for establishing the analytic treatment of trigonometric functions in Europe, also defining them as infinite series and presenting "Euler's formula", as well as the near-modern abbreviations sin., cos., tang., cot., sec., and cosec.[7]

### EtymologyEdit

Etymologically, the word sine derives from the Sanskrit word for chord, jiva*(jya being its more popular synonym). This was transliterated in Arabic as jiba جــيــب, which however is meaningless in that language and abbreviated jb جــــب . Since Arabic is written without short vowels, "jb" was interpreted as the word jaib جــيــب, which means "bosom". When the Arabic texts were translated in the 12th century into Latin by Gerard of Cremona, he used the Latin equivalent for "bosom", sinus (which means "bosom" or "bay" or "fold").[8][9] Gerard was probably not the first scholar to use this translation, Robert of Chester appears to have preceded him and there is evidence of even earlier usage.[10] The English form sine was introduced in the 1590s.

## Software implementationsEdit

The sine function, along with other trigonometric functions, is widely available across programming languages and platforms. In computing, it is typically abbreviated to sin.

Some CPU architectures have a built-in instruction for sine, including the Intel x87 FPUs since the 80387.

In programming languages, sin is typically either a built-in function or found within the language's standard math library.

For example, the C standard library defines sine functions within math.h: sin(double), sinf(float), and sinl(long double). The parameter of each is a floating point value, specifying the angle in radians. Each function returns the same data type as it accepts. Many other trigonometric functions are also defined in math.h, such as for cosine, arc sine, and hyperbolic sine (sinh).

Similarly, Python defines math.sin(x) within the built-in math module. Complex sine functions are also available within the cmath module, e.g. cmath.sin(z). CPython's math functions call the C math library, and use a double-precision floating-point format.

There is no standard algorithm for calculating sine. IEEE 754-2008, the most widely used standard for floating-point computation, does not address calculating trigonometric functions such as sine.[11] Algorithms for calculating sine may be balanced for such constraints as speed, accuracy, portability, or range of input values accepted. This can lead to different results for different algorithms, especially for special circumstances such as very large inputs, e.g. sin(1022).

A once common programming optimization, used especially in 3D graphics, was to pre-calculate a table of sine values, for example one value per degree. This allowed results to be looked up from a table rather than being calculated in real time. With modern CPU architectures this method may offer no advantage.[citation needed]

The CORDIC algorithm is commonly used in scientific calculators.

## NotesEdit

1. ^ a b Uta C. Merzbach, Carl B. Boyer (2011), A History of Mathematics, Hoboken, N.J.: John Wiley & Sons, 3rd ed., p. 189.
2. ^ Victor J. Katz (2008), A History of Mathematics, Boston: Addison-Wesley, 3rd. ed., p. 253, sidebar 8.1. "Archived copy" (PDF). Archived (PDF) from the original on 2015-04-14. Retrieved 2015-04-09.
3. ^ See Ahlfors, pages 43–44.
4. ^
5. ^ Nicolás Bourbaki (1994). Elements of the History of Mathematics. Springer.
6. ^ "Why the sine has a simple derivative Archived 2011-07-20 at the Wayback Machine.", in Historical Notes for Calculus Teachers Archived 2011-07-20 at the Wayback Machine. by V. Frederick Rickey Archived 2011-07-20 at the Wayback Machine.
7. ^ See Merzbach, Boyer (2011).
8. ^ Eli Maor (1998), Trigonometric Delights, Princeton: Princeton University Press, p. 35-36.
9. ^ Victor J. Katz (2008), A History of Mathematics, Boston: Addison-Wesley, 3rd. ed., p. 253, sidebar 8.1. "Archived copy" (PDF). Archived (PDF) from the original on 2015-04-14. Retrieved 2015-04-09.
10. ^ Smith, D.E. (1958) [1925], History of Mathematics, I, Dover, p. 202, ISBN 0-486-20429-4
11. ^ Grand Challenges of Informatics, Paul Zimmermann. September 20, 2006 – p. 14/31 "Archived copy" (PDF). Archived (PDF) from the original on 2011-07-16. Retrieved 2010-09-11.