Page:Relativity (1931).djvu/160

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140
APPENDIX I

relative to the system will be represented by the analogous formula

(2).

Those space-time points (events) which satisfy (1) must also satisfy (2). Obviously this will be the case when the relation

(3).

is fulfilled in general, where indicates a constant; for, according to (3), the disappearance of involves the disappearance of . If we apply quite similar considerations to light rays which are being transmitted along the negative -axis, we obtain the condition

(4).

By adding (or subtracting) equations (3) and (4), and introducing for convenience the constants and in place of the constants and where

and

we obtain the equations

(5).

We should thus have the solution of our problem, if the constants and were known. These result from the following discussion.

For the origin of we have permanently , and hence according to the first of the equations (5)