Copyright © 1999-2000 David E. Rutherford
All Rights Reserved
Until now, we have limited our study to four-dimensional rectangular coordinates in Euclidean spacetime. However, in order to describe our laws in general four-dimensional coordinate systems in Euclidean spacetime we must make several adjustments. We begin with the relation for the element of spacetime interval, which is the analog of (3.4)
where the
are the components of the metric tensor. In order to handle more general
coordinate systems, every previous occurrence of
must
be replaced by
. Our
formulations of the coordinate transformation equations, (6.2) and (6.4),
become
and
respectively. Where previously it was unnecessary to distinguish between covariant and contravariant components of tensors, since there is no distinction in rectangular coordinates, we must now specify which we are using. To comply with convention, superscripts will indicate contravariant components and subscripts will indicate covariant components.
In rectangular coordinates, the derivative of a tensor is, simply, the ordinary
derivative. But in general coordinates, we have terms which include nonzero
Christoffel symbols. These terms vanish in rectangular coordinates since
the components of the metric tensor are constants. In general coordinates,
however, the components of the metric tensor are not always constant, thus,
the Christoffel symbols do not always vanish. Because of this, all ordinary
derivatives of tensors must be replaced by their covariant derivatives, for
example,
becomes
where ";" indicates the covariant derivative of
with
respect to
.
Copyright © 1999-2000 David E. Rutherford
All Rights Reserved
E-mail: drutherford@softcom.net