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저자: Albert Einstein

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Since the publication of the first edition of this little book,
our knowledge about the structure of space in the large
("cosmological problem") has had an important development, which
ought to be mentioned even in a popular presentation of the
subject.
My original considerations on the subject were based on two
hypotheses:
(1) There exists an average density of matter in the whole of
space which is everywhere the same and different from zero.
(2) The magnitude ("radius") of space is independent of time.
Both these hypotheses proved to be consistent, according to the
general theory of relativity, but only after a hypothetical term
was added to the field equations, a term which was not required
by the theory as such nor did it seem natural from a theoretical
point of view ("cosmological term of the field equations").
Hypothesis (2) appeared unavoidable to me at the time, since I
thought that one would get into bottomless speculations if one
departed from it.

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