Gradient

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## Motivation

## Definition

### Cartesian coordinates

### Cylindrical and spherical coordinates

### General coordinates

## Gradient and the derivative or differential

### Linear approximation to a function

### Differential or (exterior) derivative

### Gradient as a derivative

#### Linearity

#### Product rule

#### Chain rule

## Further properties and applications

### Level sets

### Conservative vector fields and the gradient theorem

## Generalizations

### Gradient of a vector

### Riemannian manifolds

## See also

## Notes

## References

## Further reading

## External links

This article uses material from the Wikipedia page available here. It is released under the Creative Commons Attribution-Share-Alike License 3.0.

Gradient

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In vector calculus, the **gradient** is a multi-variable generalization of the derivative.^{[1]} Whereas the ordinary derivative of a function of a single variable is a scalar-valued function, the gradient of a function of several variables is a vector-valued function. Specifically, the gradient of a differentiable function of several variables, at a point , is the vector whose components are the partial derivatives of at .^{[2]}^{[3]}^{[4]}^{[5]}^{[6]}^{[7]}^{[8]}^{[9]}^{[10]}

Much as the derivative of a function of a single variable represents the slope of the tangent to the graph of the function,^{[11]} if at a point , the gradient of a function of several variables is not the zero vector, it has the direction of greatest increase of the function at , and its magnitude is the rate of increase in that direction.^{[12]}^{[13]}^{[14]}^{[15]}^{[16]}^{[17]}^{[18]}

The magnitude and direction of the gradient vector are independent of the particular coordinate representation.^{[19]}^{[20]}

The Jacobian is the generalization of the gradient for vector-valued functions of several variables and differentiable maps between Euclidean spaces or, more generally, manifolds.^{[21]}^{[22]} A further generalization for a function between Banach spaces is the Fréchet derivative.

Consider a room where the temperature is given by a scalar field, *T*, so at each point (*x*, *y*, *z*) the temperature is *T*(*x*, *y*, *z*). (Assume that the temperature does not change over time.) At each point in the room, the gradient of *T* at that point will show the direction in which the temperature rises most quickly. The magnitude of the gradient will determine how fast the temperature rises in that direction.

Consider a surface whose height above sea level at point (*x*, *y*) is *H*(*x*, *y*). The gradient of *H* at a point is a vector pointing in the direction of the steepest slope or grade at that point. The steepness of the slope at that point is given by the magnitude of the gradient vector.

The gradient can also be used to measure how a scalar field changes in other directions, rather than just the direction of greatest change, by taking a dot product. Suppose that the steepest slope on a hill is 40%. If a road goes directly up the hill, then the steepest slope on the road will also be 40%. If, instead, the road goes around the hill at an angle, then it will have a shallower slope. For example, if the angle between the road and the uphill direction, projected onto the horizontal plane, is 60°, then the steepest slope along the road will be 20%, which is 40% times the cosine of 60°.

This observation can be mathematically stated as follows. If the hill height function *H* is differentiable, then the gradient of *H* dotted with a unit vector gives the slope of the hill in the direction of the vector. More precisely, when *H* is differentiable, the dot product of the gradient of *H* with a given unit vector is equal to the directional derivative of *H* in the direction of that unit vector.

The gradient (or gradient vector field) of a scalar function *f*(*x*_{1}, *x*_{2}, *x*_{3}, ..., *x _{n}*) is denoted ?

When a function also depends on a parameter such as time, the gradient often refers simply to the vector of its spatial derivatives only (see Spatial gradient).

In the three-dimensional Cartesian coordinate system with a Euclidean metric, the gradient, if it exists, is given by:

where **i**, **j**, **k** are the standard unit vectors in the directions of the *x*, *y* and *z* coordinates, respectively. For example, the gradient of the function

is

In some applications it is customary to represent the gradient as a row vector or column vector of its components in a rectangular coordinate system.

In cylindrical coordinates with a Euclidean metric, the gradient is given by:^{[23]}

where *?* is the axial distance, *?* is the azimuthal or azimuth angle, *z* is the axial coordinate, and **e**_{?}, **e**_{?} and **e**_{z} are unit vectors pointing along the coordinate directions.

In spherical coordinates, the gradient is given by:^{[23]}

where *r* is the radial distance, *?* is the azimuthal angle and *?* is the polar angle, and **e**_{r}, **e**_{?} and **e**_{?} are again local unit vectors pointing in the coordinate directions (i.e. the normalized covariant basis).

For the gradient in other orthogonal coordinate systems, see Orthogonal coordinates (Differential operators in three dimensions).

We consider general coordinates, which we write as *x*^{1}, ..., *x*^{i}, ..., *x*^{n}, where n is the number of dimensions of the domain. Here, the upper index refers to the position in the list of the coordinate or component, so *x*^{2} refers to the second component--not the quantity *x* squared. The index variable *i* refers to an arbitrary element *x*^{i}. Using Einstein notation, the gradient can then be written as:

- ( Note that its dual is ),

where and refer to the unnormalized local covariant and contravariant bases respectively, is the inverse metric tensor, and the Einstein summation convention implies summation over *i* and *j*.

If the coordinates are orthogonal we can easily express the gradient (and the differential) in terms of the normalized bases, which we refer to as and , using the scale factors (also known as Lamé coefficients) :

- ( and ),

where we cannot use Einstein notation, since it is impossible to avoid the repetition of more than two indices. Despite the use of upper and lower indices, , , and are neither contravariant nor covariant.

The latter expression evaluates to the expressions given above for cylindrical and spherical coordinates.

The gradient of a function *f* from the Euclidean space **R**^{n} to **R** at any particular point *x*_{0} in **R**^{n} characterizes the best linear approximation to *f* at *x*_{0}. The approximation is as follows:

for *x* close to *x*_{0}, where (?*f* )_{x0} is the gradient of *f* computed at *x*_{0}, and the dot denotes the dot product on **R**^{n}. This equation is equivalent to the first two terms in the multivariable Taylor series expansion of *f* at *x*_{0}.

The best linear approximation to a differentiable function

at a point *x* in **R**^{n} is a linear map from **R**^{n} to **R** which is often denoted by *df _{x}* or

for any *v* ? **R**^{n}. The function *df*, which maps *x* to *df*_{x}, is called the differential or exterior derivative of *f* and is an example of a differential 1-form.

If **R**^{n} is viewed as the space of (dimension *n*) column vectors (of real numbers), then one can regard *df* as the row vector with components

so that *df*_{x}(*v*) is given by matrix multiplication. Assuming the standard Euclidean metric on **R**^{n}, the gradient is then the corresponding column vector, i.e.,

Let *U* be an open set in **R**^{n}. If the function *f* : *U* -> **R** is differentiable, then the differential of *f* is the (Fréchet) derivative of *f*. Thus ?*f* is a function from *U* to the space **R**^{n} such that

where · is the dot product.

As a consequence, the usual properties of the derivative hold for the gradient:

The gradient is linear in the sense that if *f* and *g* are two real-valued functions differentiable at the point *a* ? **R**^{n}, and ? and ? are two constants, then *?f* + *?g* is differentiable at *a*, and moreover

If *f* and *g* are real-valued functions differentiable at a point *a* ? **R**^{n}, then the product rule asserts that the product *fg* is differentiable at *a*, and

Suppose that *f* : *A* -> **R** is a real-valued function defined on a subset *A* of **R**^{n}, and that *f* is differentiable at a point *a*. There are two forms of the chain rule applying to the gradient. First, suppose that the function *g* is a parametric curve; that is, a function *g* : *I* -> **R**^{n} maps a subset *I* ? **R** into **R**^{n}. If *g* is differentiable at a point *c* ? *I* such that *g*(*c*) = *a*, then

where ? is the composition operator: ( *f* ? *g*)(*x*) = *f*(*g*(*x*)).

More generally, if instead *I* ? **R**^{k}, then the following holds:

where (*Dg*)^{T} denotes the transpose Jacobian matrix.

For the second form of the chain rule, suppose that *h* : *I* -> **R** is a real valued function on a subset *I* of **R**, and that *h* is differentiable at the point *f*(*a*) ? *I*. Then

A level surface, or isosurface, is the set of all points where some function has a given value.

If *f* is differentiable, then the dot product (?*f* )_{x} ? *v* of the gradient at a point *x* with a vector *v* gives the directional derivative of *f* at *x* in the direction *v*. It follows that in this case the gradient of *f* is orthogonal to the level sets of *f*. For example, a level surface in three-dimensional space is defined by an equation of the form *F*(*x*, *y*, *z*) = *c*. The gradient of *F* is then normal to the surface.

More generally, any embedded hypersurface in a Riemannian manifold can be cut out by an equation of the form *F*(*P*) = 0 such that *dF* is nowhere zero. The gradient of *F* is then normal to the hypersurface.

Similarly, an affine algebraic hypersurface may be defined by an equation *F*(*x*_{1}, ..., *x*_{n}) = 0, where *F* is a polynomial. The gradient of *F* is zero at a singular point of the hypersurface (this is the definition of a singular point). At a non-singular point, it is a nonzero normal vector.

The gradient of a function is called a gradient field. A (continuous) gradient field is always a conservative vector field: its line integral along any path depends only on the endpoints of the path, and can be evaluated by the gradient theorem (the fundamental theorem of calculus for line integrals). Conversely, a (continuous) conservative vector field is always the gradient of a function.

Since the total derivative of a vector field is a linear mapping from vectors to vectors, it is a tensor quantity.

In rectangular coordinates, the gradient of a vector field **f** = ( *f*^{1}, *f*^{2}, *f*^{3}) is defined by:

(where the Einstein summation notation is used and the tensor product of the vectors **e**_{i} and **e**_{k} is a dyadic tensor of type (2,0)). Overall, this expression equals the transpose of the Jacobian matrix:

In curvilinear coordinates, or more generally on a curved manifold, the gradient involves Christoffel symbols:

where *g*^{jk} are the components of the inverse metric tensor and the **e**_{i} are the coordinate basis vectors.

Expressed more invariantly, the gradient of a vector field **f** can be defined by the Levi-Civita connection and metric tensor:^{[24]}

where ?_{c} is the connection.

For any smooth function f on a Riemannian manifold (*M*, *g*), the gradient of *f* is the vector field ?*f* such that for any vector field *X*,

i.e.,

where *g*_{x}( , ) denotes the inner product of tangent vectors at *x* defined by the metric *g* and ?_{X} *f* is the function that takes any point *x* ? *M* to the directional derivative of *f* in the direction *X*, evaluated at *x*. In other words, in a coordinate chart *?* from an open subset of *M* to an open subset of **R**^{n}, (?_{X} *f* )(*x*) is given by:

where *X*^{j} denotes the *j*th component of *X* in this coordinate chart.

So, the local form of the gradient takes the form:

Generalizing the case *M* = **R**^{n}, the gradient of a function is related to its exterior derivative, since

More precisely, the gradient ?*f* is the vector field associated to the differential 1-form *df* using the musical isomorphism

(called "sharp") defined by the metric *g*. The relation between the exterior derivative and the gradient of a function on **R**^{n} is a special case of this in which the metric is the flat metric given by the dot product.

**^**Beauregard & Fraleigh (1973, p. 84)**^**Bachman (2007, p. 76)**^**Beauregard & Fraleigh (1973, p. 84)**^**Downing (2010, p. 316)**^**Harper (1976, p. 15)**^**Kreyszig (1972, p. 307)**^**McGraw-Hill (2007, p. 196)**^**Moise (1967, p. 683)**^**Protter & Morrey, Jr. (1970, p. 714)**^**Swokowski et al. (1994, p. 1038)**^**Protter & Morrey, Jr. (1970, pp. 21,88)**^**Bachman (2007, p. 77)**^**Downing (2010, pp. 316-317)**^**Kreyszig (1972, p. 309)**^**McGraw-Hill (2007, p. 196)**^**Moise (1967, p. 684)**^**Protter & Morrey, Jr. (1970, p. 715)**^**Swokowski et al. (1994, pp. 1036,1038-1039)**^**Kreyszig (1972, pp. 308-309)**^**Stoker (1969, p. 292)**^**Beauregard & Fraleigh (1973, pp. 87,248)**^**Kreyszig (1972, pp. 333,353,496)- ^
^{a}^{b}Schey 1992, pp. 139-142. **^**Dubrovin, Fomenko & Novikov 1991, pp. 348-349.

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*MathWorld*.

This article uses material from the Wikipedia page available here. It is released under the Creative Commons Attribution-Share-Alike License 3.0.

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