math

partial derivative

partial derivative — from formula anatomy
1 related articles · 6 formulas

Description

A partial derivative measures how a function changes when only one of its multiple variables is varied, while all others are held constant. It is a cornerstone of multivariable calculus and appears throughout physics, from thermodynamics (where pressure, volume, and temperature are interdependent) to field theories (where fields depend on space and time). The notation ∂f/∂x denotes the partial derivative of f with respect to x.

History

The concept was developed in the 18th century by mathematicians such as Leonhard Euler and Joseph-Louis Lagrange, who extended differential calculus to functions of several variables. The modern notation ∂ was introduced by Marquis de Condorcet in 1770 and popularized by Carl Gustav Jacob Jacobi in the 19th century.

How it works

To compute a partial derivative, treat all variables except the one of interest as constants and differentiate as in ordinary calculus. For example, if f(x, y) = x²y + sin(y), then ∂f/∂x = 2xy, and ∂f/∂y = x² + cos(y). Partial derivatives are used to build gradients, divergences, and curls in vector calculus, and they appear in differential equations like the wave equation and the Schrödinger equation.

In practice

Partial derivatives are used in optimization (e.g., gradient descent in machine learning), in solving partial differential equations for fluid dynamics and electromagnetism, and in error propagation analysis in experimental physics.

Fun fact

In thermodynamics, the four Maxwell relations are derived from the equality of mixed partial derivatives, linking quantities like temperature, pressure, entropy, and volume.

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Formulas

$$c_s^2 = \frac{P_X}{P_X + 2X P_{XX}}$$
Speed of perturbations in a scalar field with kinetic term.
What is in the formula
c_svariablesound speed — sound speed metre per second
Pvariablepressure of the scalar field — pressure pascal
Xvariablekinetic term, -1/2 (∂φ)^2 — kinetic energy density joule per cubic metre
P_Xvariablepartial derivative of P with respect to X — partial derivative
P_XXvariablesecond partial derivative of P with respect to X — second partial derivative
$$\partial_v r = 0$$
Condition defining a black hole horizon in null coordinates.
What is in the formula
vvariablenull coordinate (e.g., advanced time) — null coordinate metre
rvariableradial coordinate — radial coordinate metre
∂_voperatordifferentiates with respect to the null coordinate — partial derivative
$$P = i \left( \Psi^* \frac{\partial\Psi}{\partial t} - \frac{\partial\Psi^*}{\partial t} \Psi \right)$$
Defines probability density in relativistic quantum mechanics.
What is in the formula
PvariableProbability density — probability density per metre cubed
\PsivariableWave function — wave function per metre cubed half
\Psi^*variableComplex conjugate of wave function — wave function conjugate per metre cubed half
tvariableTime — time second
\frac{\partial}{\paroperatorPartial derivative with respect to time — partial derivative
$$i\hbar\frac{\partial\psi}{\partial t} = -\frac{\hbar^2}{2m}\nabla^2\psi + V\psi$$
Describes quantum particles with self-gravitating potential.
What is in the formula
ψvariablewave function of the quantum particle — wave function metre to the minus 3 over 2
tvariabletime — time second
Vvariablepotential energy (here self-gravitating) — potential energy joule
mvariablemass of the particle — mass kilogram
ħconstantReduced Planck constant, fundamental quantum of action — reduced planck constant = 1.054571817e-34 joule second
∂/∂toperatorpartial derivative with respect to time — partial derivative
∇²operatorLaplacian (spatial second derivative) — laplacian operator
$$\beta_{\rho} = M \frac{\partial \rho}{\partial M}$$
Beta function describes scale dependence of a parameter.
What is in the formula
β_ρvariablebeta function for ρ joule per cubic metre
Mvariablerenormalization scale — energy joule
ρvariablerunning parameter joule per cubic metre
∂/∂Moperatorpartial derivative with respect to scale M — partial derivative
$$\Delta T = -\frac{T}{C_p} \left( \frac{\partial S}{\partial P} \right)_T \Delta P$$
Temperature change under adiabatic pressure variation.
What is in the formula
ΔTvariabletemperature change — temperature kelvin
Tvariableabsolute temperature — temperature kelvin
C_pvariableheat capacity at constant pressure — heat capacity joule per kelvin
Svariableentropy — entropy joule per kelvin
ΔPvariablepressure change — pressure pascal
∂/∂Poperatorpartial derivative with respect to pressure at constant temperature — partial derivative

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