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
In all these corrections we are dealing with highly complex phenomena
involving Newton’s law of gravitation and the laws of mechanics. Our
astronomical time-computations have thus been adjusted so as to satisfy
the requirements of these laws, regarded as of absolute validity. We
may recall that it was this belief in the accuracy of Newton’s law that
led Römer in 1675 to the discovery of the finite velocity of light. He
noticed that Jupiter’s satellites appeared to emerge from behind the
planet’s disk several minutes later than was required by the law of
gravitation. Rather than cast doubts on the accuracy of this law, he
ascribed a finite velocity to the propagation of light. Needless to
say, his previsions have since been justified by direct terrestrial
measurements. The calculations leading to the discovery of the planet
Neptune were also based on the assumption that Newton’s law was correct.
And now let us suppose that we had elected to define time by entirely
different methods. We might, for instance, appeal to the vibrations of
the atoms of some element, such as cadmium. Then the intervals of time
marked out by the successive beats of the atom at rest in our Galilean
frame would be equal or congruent by definition. These successive
congruent intervals of time would be measured by the wave length of the
radiation, since a wave length is the distance covered by the luminous
perturbation during the interval separating two successive vibrations.
We might again proceed in still another way in terms of radioactive
processes. It is well known that, when measured by ordinary clocks,
the rate of disintegration of radium appears to follow an exponential
law. And it is a remarkable fact that this rate of disintegration does
not appear to be modified in the slightest degree by the surrounding
conditions of temperature or of pressure. Thus the phenomenon may be
regarded as being in an ideal state of isolation. Curie had therefore
suggested defining time in terms of this rate of disintegration.
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