Mathematical Methods for Physics and Engineering : A Comprehensive Guide

(lu) #1

TENSORS


components of a second-order tensorTare


δTij
δt

≡T

ij
;k

duk
dt

,

δTij
δt

≡Tij;k

duk
dt

,

δTij
δt

≡Tij;k

duk
dt

.

The derivative ofTalong the curver(t) may then be written in terms of, for


example, its contravariant components as


dT
dt

=

δTij
δt

ei⊗ej=Tij;k

duk
dt

ei⊗ej.

26.22 Geodesics

As an example of the use of the absolute derivative, we conclude this chapter


with a brief discussion of geodesics. A geodesic in real three-dimensional space


is a straight line, which has two equivalent defining properties. Firstly, it is the


curve of shortest length between two points and, secondly, it is the curve whose


tangent vector always points in the same direction (along the line). Although


in this chapter we have considered explicitly only our familiar three-dimensional


space, much of the mathematical formalism developed can be generalised to more


abstract spaces of higher dimensionality in which the familiar ideas of Euclidean


geometry are no longer valid. It is often of interest to find geodesic curves in


such spaces by using the defining properties of straight lines in Euclidean space.


We shall not consider these more complicated spaces explicitly but will de-

termine the equation that a geodesic in Euclidean three-dimensional space (i.e.


a straight line) must satisfy, deriving it in a sufficiently general way that our


method may be applied with little modification to finding the equations satisfied


by geodesics in more abstract spaces.


Let us consider a curver(s), parameterised by the arc lengthsfrom some point

on the curve, and choose as our defining property for a geodesic that its tangent


vectort=dr/dsalways points in the same direction everywhere on the curve, i.e.


dt
ds

= 0. (26.100)

Alternatively, we could exploit the property that the distance between two points


is a minimum along a geodesic and use the calculus of variations (see chapter 22);


this would lead to the same final result (26.101).


If we now introduce an arbitrary coordinate systemuiwith basis vectorsei,

i=1, 2 ,3, then we may writet=tiei, and from (26.99) we find


dt
ds

=ti;k

duk
ds

ei= 0.
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