17.02.2014 Views

Mathematical Methods for Physicists: A concise introduction - Site Map

Mathematical Methods for Physicists: A concise introduction - Site Map

Mathematical Methods for Physicists: A concise introduction - Site Map

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

TENSOR ANALYSIS<br />

Proof: In Gauss' theorem (1.78), let A ˆ B C where C is a constant vector. We<br />

then have<br />

Z<br />

Z<br />

r…B C†dV ˆ …B C†^nda:<br />

V<br />

S<br />

Since r…B C† ˆC …rB† and …B C†^n ˆ B …C ^n† ˆ…C ^n†B ˆ<br />

C …^n B†;<br />

Z<br />

Z<br />

C …rB†dV ˆ C …^n B†da:<br />

V<br />

S<br />

Taking C outside the integrals<br />

Z<br />

Z<br />

C …r B†dV ˆ C …^n B†da<br />

V<br />

S<br />

and since C is an arbitrary constant vector, we have<br />

Z<br />

Z<br />

rBdV ˆ ^n Bda:<br />

V<br />

S<br />

Tensor analysis<br />

Tensors are a natural generalization of vectors. The beginnings of tensor analysis<br />

can be traced back more than a century to Gauss' works on curved surfaces.<br />

Today tensor analysis ®nds applications in theoretical physics (<strong>for</strong> example, general<br />

theory of relativity, mechanics, and electromagnetic theory) and to certain<br />

areas of engineering (<strong>for</strong> example, aerodynamics and ¯uid mechanics). The general<br />

theory of relativity uses tensor calculus of curved space-time, and engineers<br />

mainly use tensor calculus of Euclidean space. Only general tensors are<br />

considered in this section. The general de®nition of a tensor is given, followed<br />

by a <strong>concise</strong> discussion of tensor algebra and tensor calculus (covariant di€erentiation).<br />

Tensors are de®ned by means of their properties of trans<strong>for</strong>mation under<br />

coordinate trans<strong>for</strong>mation. Let us consider the trans<strong>for</strong>mation from one coordinate<br />

system …x 1 ; x 2 ; ...; x N † to another …x 01 ; x 02 ; ...; x 0N † in an N-dimensional<br />

space V N . Note that in writing x , the index is a superscript and should not<br />

be mistaken <strong>for</strong> an exponent. In three-dimensional space we use subscripts. We<br />

now use superscripts in order that we may maintain a `balancing' of the indices in<br />

all the general equations. The meaning of `balancing' will become clear a little<br />

later. When we trans<strong>for</strong>m the coordinates, their di€erentials trans<strong>for</strong>m according<br />

to the relation<br />

dx ˆ @x<br />

@x 0 dx 0 :<br />

…1:94†<br />

47

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!