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In mathematics, a partial derivative of a function of several variables is its derivative with respect to one of those variables, with the others held constant (as opposed to the total derivative, in which all variables are allowed to vary). Partial derivatives are used in vector calculus and differential geometry.

The partial derivative of a function f with respect to the variable x is variously denoted by

\( f^\prime_x,\ f_x,\ f_{,x},\ \partial_x f, \text{ or } \frac{\partial f}{\partial x} \)

The partial-derivative symbol is ∂. The notation was introduced by Adrien-Marie Legendre and gained general acceptance after its reintroduction by Carl Gustav Jacob Jacobi.[1]

Introduction

Suppose that ƒ is a function of more than one variable. For instance,

\( z = f(x, y) = \,\! x^2 + xy + y^2.\, \)

A graph of \( z = x^2 + xy + y^2 \) . For the partial derivative at (1, 1, 3) that leaves y constant, the corresponding tangent line is parallel to the xz-plane.
A slice of the graph above at y= 1

The graph of this function defines a surface in Euclidean space. To every point on this surface, there are an infinite number of tangent lines. Partial differentiation is the act of choosing one of these lines and finding its slope. Usually, the lines of most interest are those that are parallel to the xz-plane, and those that are parallel to the yz-plane.

To find the slope of the line tangent to the function at (1, 1, 3) that is parallel to the xz-plane, the y variable is treated as constant. The graph and this plane are shown on the right. On the graph below it, we see the way the function looks on the plane y = 1. By finding the derivative of the equation while assuming that y is a constant, the slope of ƒ at the point (x, y, z) is found to be:

\( \frac{\partial z}{\partial x} = 2x+y \)

So at (1, 1, 3), by substitution, the slope is 3. Therefore

\( \frac{\part z}{\part x} = 3 \)

at the point. (1, 1, 3). That is, the partial derivative of z with respect to x at (1, 1, 3) is 3.
Definition
Basic definition

The function f can be reinterpreted as a family of functions of one variable indexed by the other variables:

\( f(x,y) = f_x(y) = \,\! x^2 + xy + y^2.\, \)

In other words, every value of x defines a function, denoted fx, which is a function of one variable.[2] That is,

\( f_x(y) = x^2 + xy + y^2.\, \)

Once a value of x is chosen, say a, then f(x,y) determines a function fa which sends y to \( a^2 + ay + y^2 \) :

\( f_a(y) = a^2 + ay + y^2. \, \)

In this expression, a is a constant, not a variable, so fa is a function of only one real variable, that being y. Consequently, the definition of the derivative for a function of one variable applies:

\( f_a'(y) = a + 2y. \, \)

The above procedure can be performed for any choice of a. Assembling the derivatives together into a function gives a function which describes the variation of f in the y direction:

\( \frac{\part f}{\part y}(x,y) = x + 2y.\, \)

This is the partial derivative of f with respect to y. Here ∂ is a rounded d called the partial derivative symbol. To distinguish it from the letter d, ∂ is sometimes pronounced "del" or "partial" instead of "dee".

In general, the partial derivative of a function f(x1,...,xn) in the direction xi at the point (a1,...,an) is defined to be:

\( \frac{\part f}{\part x_i}(a_1,\ldots,a_n) = \lim_{h \to 0}\frac{f(a_1,\ldots,a_i+h,\ldots,a_n) - f(a_1,\ldots, a_i, \dots,a_n)}{h}. \)

In the above difference quotient, all the variables except xi are held fixed. That choice of fixed values determines a function of one variable \( f_{a_1,\ldots,a_{i-1},a_{i+1},\ldots,a_n}(x_i) = f(a_1,\ldots,a_{i-1},x_i,a_{i+1},\ldots,a_n) \) , and by definition,

\( \frac{df_{a_1,\ldots,a_{i-1},a_{i+1},\ldots,a_n}}{dx_i}(x_i) = \frac{\part f}{\part x_i}(a_1,\ldots,a_n). \)

In other words, the different choices of a index a family of one-variable functions just as in the example above. This expression also shows that the computation of partial derivatives reduces to the computation of one-variable derivatives.

An important example of a function of several variables is the case of a scalar-valued function f(x1,...xn) on a domain in Euclidean space Rn (e.g., on R2 or R3). In this case f has a partial derivative ∂f/∂xj with respect to each variable xj. At the point a, these partial derivatives define the vector

\( \nabla f(a) = \left(\frac{\partial f}{\partial x_1}(a), \ldots, \frac{\partial f}{\partial x_n}(a)\right). \)

This vector is called the gradient of f at a. If f is differentiable at every point in some domain, then the gradient is a vector-valued function ∇f which takes the point a to the vector ∇f(a). Consequently, the gradient produces a vector field.

A common abuse of notation is to define the del operator (∇) as follows in three-dimensional Euclidean space R3 with unit vectors \(\mathbf{\hat{i}}, \mathbf{\hat{j}}, \mathbf{\hat{k}} \) :

\( \nabla = \bigg[{\frac{\partial}{\partial x}} \bigg] \mathbf{\hat{i}} + \bigg[{\frac{\partial}{\partial y}}\bigg] \mathbf{\hat{j}} + \bigg[{\frac{\partial}{\partial z}}\bigg] \mathbf{\hat{k}} \)

Or, more generally, for n-dimensional Euclidean space Rn with coordinates (x1, x2, x3,...,xn) and unit vectors \( (\mathbf{\hat{e}_1}, \mathbf{\hat{e}_2}, \mathbf{\hat{e}_3}, \dots , \mathbf{\hat{e}_n}):

\( \nabla = \sum_{j=1}^n \bigg[{\frac{\partial}{\partial x_j}}\bigg] \mathbf{\hat{e}_j} = \bigg[{\frac{\partial}{\partial x_1}}\bigg] \mathbf{\hat{e}_1} + \bigg[{\frac{\partial}{\partial x_2}}\bigg] \mathbf{\hat{e}_2} + \bigg[{\frac{\partial}{\partial x_3}}\bigg] \mathbf{\hat{e}_3} + \dots + \bigg[{\frac{\partial}{\partial x_n}}\bigg] \mathbf{\hat{e}_n} \)

Formal definition

Like ordinary derivatives, the partial derivative is defined as a limit. Let U be an open subset of Rn and f : UR a function. The partial derivative of f at the point a = (a1, ..., an) ∈ U with respect to the i-th variable ai is defined as

\( \frac{ \partial }{\partial a_i }f(\mathbf{a}) = \lim_{h \rightarrow 0}{ f(a_1, \dots , a_{i-1}, a_i+h, a_{i+1}, \dots ,a_n) - f(a_1, \dots, a_i, \dots ,a_n) \over h } \)

Even if all partial derivatives ∂f/∂ai(a) exist at a given point a, the function need not be continuous there. However, if all partial derivatives exist in a neighborhood of a and are continuous there, then f is totally differentiable in that neighborhood and the total derivative is continuous. In this case, it is said that f is a C1 function. This can be used to generalize for vector valued functions (f : UR'm) by carefully using a componentwise argument.

The partial derivative \( \frac{\partial f}{\partial x} \) can be seen as another function defined on U and can again be partially differentiated. If all mixed second order partial derivatives are continuous at a point (or on a set), f is termed a C2 function at that point (or on that set); in this case, the partial derivatives can be exchanged by Clairaut's theorem:

\( \frac{\partial^2f}{\partial x_i\, \partial x_j} = \frac{\partial^2f} {\partial x_j\, \partial x_i}. \)

Examples
The volume of a cone depends on height and radius

The volume V of a cone depends on the cone's height h and its radius r according to the formula

\( V(r, h) = \frac{\pi r^2 h}{3}. \)

The partial derivative of V with respect to r is

\( \frac{ \partial V}{\partial r} = \frac{ 2 \pi r h}{3}, \)

which represents the rate with which a cone's volume changes if its radius is varied and its height is kept constant. The partial derivative with respect to h is

\( \frac{ \partial V}{\partial h} = \frac{\pi r^2}{3}, \)

which represents the rate with which the volume changes if its height is varied and its radius is kept constant.

By contrast, the total derivative of V with respect to r and h are respectively

\( \frac{\operatorname dV}{\operatorname dr} = \overbrace{\frac{2 \pi r h}{3}}^\frac{ \partial V}{\partial r} + \overbrace{\frac{\pi r^2}{3}}^\frac{ \partial V}{\partial h}\frac{\operatorname d h}{\operatorname d r} \)

and

\( \frac{\operatorname dV}{\operatorname dh} = \overbrace{\frac{\pi r^2}{3}}^\frac{ \partial V}{\partial h} + \overbrace{\frac{2 \pi r h}{3}}^\frac{ \partial V}{\partial r}\frac{\operatorname d r}{\operatorname d h} \)

The difference between the total and partial derivative is the elimination of indirect dependencies between variables in partial derivatives.

If (for some arbitrary reason) the cone's proportions have to stay the same, and the height and radius are in a fixed ratio k,

\( k = \frac{h}{r} = \frac{\operatorname d h}{\operatorname d r}. \)

This gives the total derivative with respect to r:

\( \frac{\operatorname dV}{\operatorname dr} = \frac{2 \pi r h}{3} + \frac{\pi r^2}{3}k \)

Which simplifies to:

\( \frac{\operatorname dV}{\operatorname dr} = k\pi r^2 \)

Similarly, the total derivative with respect to h is:

\( \frac{\operatorname dV}{\operatorname dh} = \pi r^2 \)

Equations involving an unknown function's partial derivatives are called partial differential equations and are common in physics, engineering, and other sciences and applied disciplines.
Notation

For the following examples, let f be a function in x, y and z.

First-order partial derivatives:

\( \frac{ \partial f}{ \partial x} = f_x = \partial_x f. \)

Second-order partial derivatives:

\( \frac{ \partial^2 f}{ \partial x^2} = f_{xx} = \partial_{xx} f. \)

Second-order mixed derivatives:

\( \frac{\partial^2 f}{\partial y \, \partial x} = \frac{\partial}{\partial y} \left( \frac{\partial f}{\partial x} \right) = f_{xy} = \partial_{yx} f. \)

Higher-order partial and mixed derivatives:

\( \frac{ \partial^{i+j+k} f}{ \partial x^i\, \partial y^j\, \partial z^k } = f^{(i, j, k)}. \)

When dealing with functions of multiple variables, some of these variables may be related to each other, and it may be necessary to specify explicitly which variables are being held constant. In fields such as statistical mechanics, the partial derivative of f with respect to x, holding y and z constant, is often expressed as

\( \left( \frac{\partial f}{\partial x} \right)_{y,z}. \)

Antiderivative analogue

There is a concept for partial derivatives that is analogous to antiderivatives for regular derivatives. Given a partial derivative, it allows for the partial recovery of the original function.

Consider the example of \( \frac{\partial z}{\partial x} = 2x+y \) . The "partial" integral can be taken with respect to x (treating y as constant, in a similar manner to partial derivation):

\( z = \int \frac{\partial z}{\partial x} \,dx = x^2 + xy + g(y) \)

Here, the "constant" of integration is no longer a constant, but instead a function of all the variables of the original function except x. The reason for this is that all the other variables are treated as constant when taking the partial derivative, so any function which does not involve x will disappear when taking the partial derivative, and we have to account for this when we take the antiderivative. The most general way to represent this is to have the "constant" represent an unknown function of all the other variables.

Thus the set of functions \( x^2 + xy + g(y) \) , where g is any one-argument function, represents the entire set of functions in variables x,y that could have produced the x-partial derivative 2x+y.

If all the partial derivatives of a function are known (for example, with the gradient), then the antiderivatives can be matched via the above process to reconstruct the original function up to a constant.
See also

d'Alembertian operator
Chain rule
Curl (mathematics)
Directional derivative
Divergence
Exterior derivative
Gradient
Jacobian matrix and determinant
Laplacian
Symmetry of second derivatives
Triple product rule, also known as the cyclic chain rule.

Notes

^ Jeff Miller (2009-06-14). "Earliest Uses of Symbols of Calculus". Earliest Uses of Various Mathematical Symbols. Retrieved 2010-02-20.
^ This can also be expressed as the adjointness between the product space and function space constructions.

Mathematics Encyclopedia

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