The evolution of scientific thought from Newton to EinsteinD'Abro, A. (Aram)
Science
The evolution of scientific thought from Newton to Einstein
D'Abro, A. (Aram)
Relativity (Physics); Science -- Methodology
Now when we say that a theory of mathematical physics is correct, all
we mean is that the various mathematical consequences we can extract
from its equations call for the existence of physical phenomena which
experiment has succeeded in verifying. On the other hand, if our
mathematical anticipations do not tally with experimental verification,
we must recognise that our theory is incorrect. This does not mean that
it is incorrect from a purely mathematical point of view, for in any
case it exemplifies a possible rational world; but it is incorrect in
that it does not exemplify our real world. We must then assume that
our initial equations were in all probability bad translations of the
physical phenomena they were supposed to represent.
In a number of cases, however, it has been found unnecessary to
abandon a theory merely because one of its anticipations happened to
be refuted by experiment. Instead, it is often possible to assume that
the discrepancy between the mathematical anticipation and the physical
result may be due to some contingent physical influence, which,
owing to the incompleteness of the physical data furnished us by the
experimenters, our equations have failed to take into consideration. A
case in point is afforded by the discovery of Neptune.
The Newtonian mathematical treatment of planetary motions assigned a
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definite motion to the planet Uranus. Astronomical observation then
proved that the actual motion of Uranus did not tally with these
mathematical anticipations. Yet it was not deemed necessary to abandon
Newton’s law; Adams and Leverrier suggested the possibility that an
unknown planet lying beyond the orbit of Uranus might be responsible
for the deviations in Uranus’ motion. Taking the existence of this
unknown planet into consideration in his mathematical calculations,
Leverrier succeeded in determining the exact position which it would
have to occupy in the heavens at an assigned date. As is well known,
at the precise spot calculated, the elusive planet (presently named
Neptune) was discovered with a powerful telescope.
Public-domain text, read in full here on John Shaqi.
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