A.6 Relativity-tensor notation
For relativistic calculation we use the Bjorken-Drell metric
↓↓
and the four-vector notation
↓
Lowered indices:
↓
where we use the full Einstein summation convention
↓ that “any index that appears as upper and lower index is summed over; indices can be raised and lowered by the metric tensor
↓”. Thus
and
In the same way
(
is the Dalembertian
↓).
We also find that
where the “Kronecker
”
↓ is one if both indices are equal, and zero otherwise.
We shall denote a Lorentz transformation
↓ by
, and as we change inertial frames
↓ a four vector transforms as
where the position of the indices on
is crucial. From
and the invariance of
we find
(Note the change of place of the indices). What it means is that the only difference is a minus sign for the components in the
and
entries of the matrix.