Mathematical Methods for Physics and Engineering : A Comprehensive Guide

(Darren Dugan) #1

TENSORS


uito anotheru′i, we may define the Jacobian of the transformation (see chapter 6)


as the determinant of the transformation matrix [∂u′i/∂uj]: this is usually denoted


by


J=





∂u′
∂u




∣.

Alternatively, we may interchange the primed and unprimed coordinates to


obtain|∂u/∂u′|=1/J: unfortunately this also is often called the Jacobian of the


transformation.


Using the JacobianJ, we define a relative tensor of weightwas one whose

components transform as follows:


T′

ij···k
lm···n=

∂u′i
∂ua

∂u′j
∂ub

···

∂u′k
∂uc

∂ud
∂u′l

∂ue
∂u′m

···

∂uf
∂u′n

Tab···cde···f





∂u
∂u′





w
.
(26.74)

Comparing this expression with (26.71), we see that a true (orabsolute) general


tensor may be considered as a relative tensor of weightw=0.Ifw=−1, on the


other hand, the relative tensor is known as a generalpseudotensorand ifw=1


as atensor density.


It is worth comparing (26.74) with the definition (26.39) of a Cartesian pseu-

dotensor. For the latter, we are concerned only with its behaviour under a rotation


(proper or improper) of Cartesian axes, for which the JacobianJ=±1. Thus,


general relative tensors of weightw=−1andw= 1 would both satisfy the


definition (26.39) of a Cartesian pseudotensor.


If thegijare the covariant components of the metric tensor, show that the determinantg
of the matrix[gij]is a relative scalar of weightw=2.

The componentsgijtransform as


gij′=

∂uk
∂u′i

∂ul
∂u′j

gkl.

Defining the matricesU=[∂ui/∂u′j],G=[gij]andG′=[g′ij], we may write this expression
as


G′=UTGU.

Taking the determinant of both sides, we obtain


g′=|U|^2 g=



∣∣∂u
∂u′



∣∣


2
g,

which shows thatgis a relative scalar of weightw=2.


From the discussion in section 26.8, it can be seen thatijkis a covariant

relative tensor of weight−1. We may also define the contravariant tensorijk,


which is numerically equal toijkbut is a relative tensor of weight +1.


If two relative tensors have weightsw 1 andw 2 respectively then, from (26.74),
Free download pdf