math

cosine

A trigonometric function, the complement of sine, describing a smooth periodic oscillation.
6 formulas

Description

The cosine function, written cos(θ), is a fundamental trigonometric function that describes a smooth, periodic oscillation. It is defined as the ratio of the adjacent side to the hypotenuse in a right triangle, but its true power lies in its wave-like behavior: it repeats every 360° (or 2π radians) and oscillates between −1 and 1. Cosine is the complement of sine, meaning cos(θ) = sin(θ + 90°). It appears throughout physics, from the motion of pendulums and alternating currents to the interference patterns of light.

History

The cosine function was developed in ancient India and later formalized in Islamic mathematics. The modern notation 'cos' was introduced by Leonhard Euler in the 18th century, who also established its connection to complex exponentials via Euler's formula.

How it works

On the unit circle, the cosine of an angle θ is the x-coordinate of the point where the terminal side of the angle intersects the circle. As θ increases, this coordinate traces a smooth wave. In physics, cosine functions often describe the projection of circular motion onto a line, such as the horizontal position of a point on a rotating wheel. Its derivative is the negative sine, which links it to harmonic motion: the second derivative is proportional to the negative of the function itself, the hallmark of simple harmonic oscillators.

In practice

Cosine is used in signal processing (e.g., Fourier transforms), electrical engineering for AC circuits, and in physics to model wave phenomena like sound and light.

Fun fact

The cosine of an angle in radians is the real part of the complex exponential e^{iθ}, a relationship that underpins quantum mechanics and signal analysis.

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Formulas

$$1+z = rac{1}{ rac{ ext{v}}{c} ext{cos} heta ext{ sign} ext{ adjusted}}$$
Redshift due to relative motion between observer and source.
What is in the formula
zvariableredshift parameter — redshift
vvariablerelative velocity between source and observer — velocity metre per second
θvariableangle between velocity vector and line of sight — angle radian
cconstantspeed of light in vacuum — speed of light = 299792458 metre per second
cosoperatortrigonometric cosine function — cosine
$$e \cos \omega = \frac{\pi \Delta t}{2P}$$
Eccentricity and argument of periastron from eclipse timing.
What is in the formula
evariableOrbital eccentricity — eccentricity
ωvariableArgument of periastron — argument of periapsis radian
ΔtvariableTime offset in eclipse timing — time offset second
PvariableOrbital period — period second
cosoperatorComputes the cosine of an angle — cosine
$$F(\theta_1, \theta_2, C_{QE}, \phi) = F_0 (1 - C_{QE} A(\theta_1) A(\theta_2) \cos(2\phi))$$
Correlation function depends on entanglement degree and scattering angles.
What is in the formula
FvariableCorrelation function — correlation function
F_0variableNormalization constant — correlation function
C_QEvariableDegree of quantum entanglement — entanglement degree
A(\theta_1)variableAngular modulation factor at angle theta_1 — modulation factor
A(\theta_2)variableAngular modulation factor at angle theta_2 — modulation factor
\theta_1variableScattering angle for first particle — angle radian
\theta_2variableScattering angle for second particle — angle radian
\phivariableAzimuthal angle — angle radian
\cosoperatorTrigonometric cosine function — cosine
$$A(\theta) = \frac{\sin^{2}\theta (2-\cos\theta)}{2+(1-\cos\theta)^{3}}$$
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
$$B(k_1,k_2,k_3) \propto (k_1/k_2)^\Delta \cos(\omega \ln(k_1/k_2))$$
Bispectrum shows oscillations from additional fields.
What is in the formula
Bvariablebispectrum — bispectrum cubic metre
k_1variablefirst wavenumber — wavenumber reciprocal metre
k_2variablesecond wavenumber — wavenumber reciprocal metre
k_3variablethird wavenumber — wavenumber reciprocal metre
\Deltavariablespectral tilt — dimensionless
\omegavariableoscillation frequency in log space — dimensionless
\proptooperatorindicates the left side equals the right side times a constant factor — proportionality
\lnoperatorlogarithm to base e — natural logarithm
\cosoperatortrigonometric cosine — cosine

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