Einstein, the searcher : $b his work explained from dialogues with EinsteinMoszkowski, Alexander
Philosophy
Einstein, the searcher : $b his work explained from dialogues with Einstein
Moszkowski, Alexander
Einstein, Albert, 1879-1955; Relativity (Physics)
The Law of Inertia, according to our human standard, seems unsurpassable
in simplicity and completeness; it seems to us fundamental. But this
law, which prescribes uniform rectilinear motion to a body subject to no
external forces, selects only one possibility out of an infinite number
as being valid for us. It does not seem evident to a child, and it is
easy to imagine a good scholar in some branch of knowledge other than
physics, to whom it would likewise not seem evident. For it is by no
means necessary a priori that a body will move at all when all forces
are absent. If the law were self-evident, it would not need to have been
discovered by Galilei in 1638. Nevertheless, it appears to us, now, to
be absolutely self-evident, and we can scarcely imagine that it can ever
be otherwise. This is simply because we are bound to the current set of
ideas that cannot extend beyond the sum of sense-data and experiences
that have been inculcated into us by heredity and environment. At a very
distant date in the future the average mind may surpass that of Galilei
to the same extent as Galilei's surpasses that of a child, or of a
Papuan native. And of all the infinite possibilities one may occur to a
Galilei of the distant future, which, when formulated as a law, may
serve to describe motions of a body subject to no forces better than the
law of inertia, proposed in 1638.
These reflections are not mere hallucinations, but have to do with
scientific occurrences that we have observed in the twentieth century.
Newton's equation that gives the Law of Attraction is beyond doubt a
model of simplicity, and it would have occurred to no thinking person of
even the last generation to doubt its accuracy. The easily grasped
expression k (m.m^1⁄r^2) apparently expresses truth in a law which is
valid for all eternity. In this expression, he denotes a gravitational
constant, that is, a quantity which is invariable in the whole universe;
_m_ and _m_^1 are two masses that act attractively on one another; and
_r_ is the distance between them. But Newton has been followed by
Einstein, who has proved that this expression represents only an
approximate value, that leaves a small remainder as an error that may be
detected if the greatest refinement be made in our methods of
observation. The equations that have been set up by Einstein represent
the approximation that is to be considered final for the present, and
that may remain valid for thousands of years. They are certainly very
complicated, being included in a system of differential equations of
awe-inspiring length, and we may feel tempted to object with the
question: how do they agree with Kirchhoff's postulate that the simplest
description of the motions must be sought? But this objection falls to
the ground if we look carefully into the question. For simplicity
consists not merely in being brief or in excluding difficulty from a
formula, but rather in asserting the simplest relation to the universe
Public-domain text, read in full here on John Shaqi.
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