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著者: Albert Einstein

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We imagine a large portion of empty space, so far removed from
stars and other appreciable masses, that we have before us
approximately the conditions required by the fundamental law of
Galilei. It is then possible to choose a Galileian reference-body
for this part of space (world), relative to which points at rest
remain at rest and points in motion continue permanently in
uniform rectilinear motion. As reference-body let us imagine a
spacious chest resembling a room with an observer inside who is
equipped with apparatus. Gravitation naturally does not exist for
this observer. He must fasten himself with strings to the floor,
otherwise the slightest impact against the floor will cause him
to rise slowly towards the ceiling of the room.

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