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In mathematics, the total derivative of a function is the best linear approximation of the value of the function with respect to its arguments. Unlike partial derivatives, the total derivative approximates the function with respect to all of its arguments, not just a single one. In many situations, this is the same as considering all partial derivatives simultaneously. The term "total derivative" is primarily used when is a function of several variables, because when is a function of a single variable, the total derivative is the same as the derivative of the function.[1]:198–203

"Total derivative" is sometimes also used as a synonym for the material derivative in fluid mechanics.

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The total derivative as a linear mapEdit

Let   be an open subset. Then a function   is said to be (totally) differentiable at a point   if there exists a linear transformation   such that

 

The linear map   is called the (total) derivative or (total) differential of   at  . Other notations for the total derivative include   and  . A function is (totally) differentiable if its total derivative exists at every point in its domain.

Conceptually, the definition of the total derivative expresses the idea that   is the best linear approximation to   at the point  . This can be made precise by quantifying the error in the linear approximation determined by  . To do so, write

 

where   equals the error in the approximation. To say that the derivative of   at   is   is equivalent to the statement

 

where   is little-o notation and indicates that   is much smaller than   as  . The total derivative   is the unique linear transformation for which the error term is this small, and this is the sense in which it is the best linear approximation to  .

The function   is differentiable if and only if each of its components   is differentiable, so when studying total derivatives, it is often possible to work one coordinate at a time in the codomain. However, the same is not true of the coordinates in the domain. It is true that if   is differentiable at  , then each partial derivative   exists at  . The converse is false: It can happen that all of the partial derivatives of   at   exist, but   is not differentiable at  . This means that the function is very "rough" at  , to such an extreme that its behavior cannot be adequately described by its behavior in the coordinate directions. When   is not so rough, this cannot happen. More precisely, if all the partial derivatives of   at   exist and are continuous in a neighborhood of  , then   is differentiable at  . When this happens, then in addition, the total derivative of   is the linear transformation corresponding to the Jacobian matrix of partial derivatives at that point.[2]

The total derivative as a differential formEdit

When the function under consideration is real-valued, the total derivative can be recast using differential forms. For example, suppose that   is a differentiable function of variables  . The total derivative of   at   may be written in terms of its Jacobian matrix, which in this instance simplifies to the gradient:

 

The linear approximation property of the total derivative implies that if

 

is a small vector (where the   denotes transpose, so that this vector is a column vector), then

 

Heuristically, this suggests that if   are infinitesimal increments in the coordinate directions, then

 

The theory of differential forms is one way to give a precise meaning to infinitesimal increments such as  . In this theory,   is a linear functional on the vector space  . Evaluating   at a vector   in   measures how much   points in the  th coordinate direction. The total derivative   is a linear combination of linear functionals and hence is itself a linear functional. The evaluation   measures how much   points in the direction determined by   at  , and this direction is the gradient. This point of view makes the total derivative an instance of the exterior derivative.

Suppose now that   is a vector-valued function, that is,  . In this case, the components   of   are real-valued functions, so they have associated differential forms  . The total derivative   amalgamates these forms into a single object and is therefore an instance of a vector-valued differential form.

The chain rule for total derivativesEdit

The chain rule has a particularly elegant statement in terms of total derivatives. It says that, for two functions   and  , the total derivative of the composite   at   satisfies

 

If the total derivatives of   and   are identified with their Jacobian matrices, then the composite on the right-hand side is simply matrix multiplication. This is enormously useful in applications, as it makes it possible to account for essentially arbitrary dependencies among the arguments of a composite function.

Example: Differentiation with direct dependenciesEdit

Suppose that f is a function of two variables, x and y. If these two variables are independent, so that the domain of f is  , then the behavior of f may be understood in terms of its partial derivatives in the x and y directions. However, in some situations, x and y may be dependent. For example, it might happen that f is constrained to a curve  . In this case, we are actually interested in the behavior of the composite function  . The partial derivative of f with respect to x does not give the true rate of change of f with respect to changing x because changing x necessarily changes y. However, the chain rule for the total derivative takes such dependencies into account. Write  . Then chain rule says

 

By expressing the total derivative using Jacobian matrices, this becomes:

 

Suppressing the evaluation at   for legibility, we may also write this as

 

This gives a straightforward formula for the derivative of   in terms of the partial derivatives of   and the derivative of  .

For example, suppose

 

The rate of change of f with respect to x is usually the partial derivative of f with respect to x; in this case,

 

However, if y depends on x, the partial derivative does not give the true rate of change of f as x changes because the partial derivative assumes that y is fixed. Suppose we are constrained to the line

 

Then

 

and the total derivative of f with respect to x is

 

which we see is not equal to the partial derivative  . Instead of immediately substituting for y in terms of x, however, we can also use the chain rule as above:

 

Example: Differentiation with indirect dependenciesEdit

While one can often perform substitutions to eliminate indirect dependencies, the chain rule provides for a more efficient and general technique. Suppose   is a function of time   and   variables   which themselves depend on time. Then, the time derivative of   is

 

The chain rule expresses this derivative in terms of the partial derivatives of   and the time derivatives of the functions  :

 

This expression is often used in physics for a gauge transformation of the Lagrangian, as two Lagrangians that differ only by the total time derivative of a function of time and the   generalized coordinates lead to the same equations of motion. An interesting example concerns the resolution of causality concerning the Wheeler–Feynman time-symmetric theory. The operator in brackets (in the final expression above) is also called the total derivative operator (with respect to  ).

For example, the total derivative of   is

 

Here there is no   term since   itself does not depend on the independent variable   directly.

Total differential equationEdit

A total differential equation is a differential equation expressed in terms of total derivatives. Since the exterior derivative is coordinate-free, in a sense that can be given a technical meaning, such equations are intrinsic and geometric.

Application to equation systemsEdit

In economics, it is common for the total derivative to arise in the context of a system of equations.[1]:pp. 217–220 For example, a simple supply-demand system might specify the quantity q of a product demanded as a function D of its price p and consumers' income I, the latter being an exogenous variable, and might specify the quantity supplied by producers as a function S of its price and two exogenous resource cost variables r and w. The resulting system of equations

 
 

determines the market equilibrium values of the variables p and q. The total derivative   of p with respect to r, for example, gives the sign and magnitude of the reaction of the market price to the exogenous variable r. In the indicated system, there are a total of six possible total derivatives, also known in this context as comparative static derivatives: dp / dr, dp / dw, dp / dI, dq / dr, dq / dw, and dq / dI. The total derivatives are found by totally differentiating the system of equations, dividing through by, say dr, treating dq / dr and dp / dr as the unknowns, setting dI = dw = 0, and solving the two totally differentiated equations simultaneously, typically by using Cramer's rule.

ReferencesEdit

  1. ^ a b Chiang, Alpha C. (1984). Fundamental Methods of Mathematical Economics (Third ed.). McGraw-Hill. ISBN 0-07-010813-7.
  2. ^ Abraham, Ralph; Marsden, J. E.; Ratiu, Tudor (2012). Manifolds, Tensor Analysis, and Applications. Springer Science & Business Media. p. 78.
  • A. D. Polyanin and V. F. Zaitsev, Handbook of Exact Solutions for Ordinary Differential Equations (2nd edition), Chapman & Hall/CRC Press, Boca Raton, 2003. ISBN 1-58488-297-2
  • From thesaurus.maths.org total derivative

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