Ksiazka · Relativity
Strona 86 z 212
Autor: Albert Einstein
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Up to the present, however, we have by no means maintained the
equivalence of all bodies of reference K in connection with the
formulation of natural laws. Our course was more on the following
Iines. In the first place, we started out from the assumption
that there exists a reference-body K, whose condition of motion
is such that the Galileian law holds with respect to it: A
particle left to itself and sufficiently far removed from all
other particles moves uniformly in a straight line. With
reference to K (Galileian reference-body) the laws of nature were
to be as simple as possible. But in addition to K, all bodies of
reference K′ should be given preference in this sense, and they
should be exactly equivalent to K for the formulation of natural
laws, provided that they are in a state of uniform rectilinear
and non-rotary motion with respect to K; all these bodies of
reference are to be regarded as Galileian reference-bodies.
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