math

sine

sine — from formula anatomy
4 formulas

Description

The sine function is a fundamental mathematical tool that describes smooth, repetitive oscillations. It maps an angle to the ratio of two sides of a right triangle, but its true power lies in modeling any periodic phenomenon — from sound waves and alternating current to the vibrations of a guitar string. In physics, sine waves are the building blocks of all waveforms: any complex signal can be decomposed into a sum of sine waves of different frequencies and amplitudes, a principle known as Fourier analysis.

History

The sine function was formalized in ancient India and later refined by Islamic mathematicians, but the modern notation and treatment as a function of a real variable emerged in the 17th century with Euler and others.

How it works

Imagine a point moving around a circle at constant speed. The sine of the angle it sweeps is the vertical coordinate of that point, plotted against time. This produces a smooth, wavy curve that repeats every 360 degrees (or 2π radians). The function takes an angle as input and outputs a value between -1 and 1, with the shape determined by the circle's radius and the speed of rotation.

In practice

Sine waves are used in signal processing, acoustics, electrical engineering (AC power), and even in medical imaging (MRI) to encode spatial information.

Fun fact

The sine of an angle in radians is also the length of the shadow cast by a vertical stick of unit length when the sun is at that angle above the horizon.

Concept graph →

Formulas

$$D_L(z) = \frac{c(1+z)}{H_0} \times \begin{cases} \frac{\sinh\left(\sqrt{\Omega_k}\chi(z)\right)}{\sqrt{\Omega_k}} & \Omega_k>0 \\ \chi(z) & \Omega_k=0 \\ \frac{\sin\left(\sqrt{-\Omega_k}\chi(z)\right)}{\sqrt{-\Omega_k}} & \Omega_k<0 \end{cases}$$
Luminosity distance depends on redshift and cosmological parameters.
What is in the formula
D_Lvariableluminosity distance — photometric distance metre
zvariableredshift — redshift
χvariablecomoving distance — comoving distance metre
Ω_kvariablecurvature density parameter — curvature density parameter
cconstantspeed of light in vacuum — speed of light = 299792458 metre per second
H_0constantcurrent expansion rate of the universe — hubble constant = 2.2e-18 per second
sinhoperatorhyperbolic sine function — hyperbolic sine
sinoperatorsine function — sine
√operatorsquare root — square root
$$\sin \theta = \frac{q}{r} \sqrt{ \frac{1 + 2GM/(q v_{\infty}^2)}{1 - 2GM/(r v_{\infty}^2)} }$$
Angle for gravitational scattering trajectories.
What is in the formula
thetavariabledeflection angle — angle radian
qvariabledistance of closest approach in absence of gravity — distance metre
rvariableradial distance from the gravitating body — distance metre
Mvariablemass of the gravitating body — mass kilogram
v_infinityvariablespeed of the test particle at infinity — velocity metre per second
GconstantUniversal constant of gravitation — gravitational constant = 6.67430e-11 cubic metre per kilogram per second squared
sinoperatortrigonometric sine function — sine
sqrtoperatortakes the square root of the argument — square root
$$A(\theta) = \frac{\sin^{2}\theta (2-\cos\theta)}{2+(1-\cos\theta)^{3}}$$
Modulation factor for Compton scattering at 511 keV photons.
What is in the formula
A(\theta)variableModulation factor — modulation factor
\thetavariableScattering angle — angle radian
\sinoperatorTrigonometric sine function — sine
\cosoperatorTrigonometric cosine function — cosine
$$x\cos\phi + y\sin\phi = p$$
A line's equation using normal distance and angle.
What is in the formula
xvariablex-coordinate of a point on the line — x coordinate metre
yvariabley-coordinate of a point on the line — y coordinate metre
\phivariableangle of the normal to the line with respect to the x-axis — angle radian
pvariableperpendicular distance from the origin to the line — distance metre
\cosoperatorcomputes the cosine of an angle — cosine
\sinoperatorcomputes the sine of an angle — sine

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