Famous People in Astronomy for the CSET

Feb
19

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special relativity and idea of equivalence. Albert Einstein was taken seriously after rigorous testing of his theories. One example is the famous advance of Mercury’s perihelion. Because Newton’s law did not correctly predict this, Einstein’s theory gained approval for a new

revolution in science. Furthermore, the eclipse experiment of 1919 helped to prove his bending of light theory. These proofs helped him to gain wider acceptance of his theories. Einstein recieved the Nobel Prize in 1921, not for his research on relativity, but for his 1905 work on the photoelectric effect.

In the first of three papers, all written in 1905, Einstein examined the phenomenon discovered by Max Planck, according to which electromagnetic energy seemed to be emitted from radiating objects in discrete quantities. The energy of these quanta was directly proportional to the frequency of the radiation. This seemed to contradict classical electromagnetic theory, based on Maxwell’s equations and the laws of thermodynamics which assumed that electromagnetic energy consisted of waves which could contain any small amount of energy. Einstein used Planck’s quantum hypothesis to describe the electromagnetic radiation of light.

Einstein’s second 1905 paper proposed what is today called the special theory of relativity. He based his new theory on a reinterpretation of the classical principle of relativity, namely that the laws of physics had to have the same form in any frame of reference. As a second fundamental hypothesis, Einstein assumed that the speed of light remained constant in all frames of reference, as required by Maxwell’s theory.

Later in 1905 Einstein showed how mass and energy were equivalent: the famous e = mc2 . Einstein was not the first to propose all the components of special theory of relativity. His contribution is unifying important parts of classical mechanics and Maxwell’s electrodynamics.

The third of Einstein’s papers of 1905 concerned statistical mechanics, a field of that had been studied by Ludwig Boltzmann and Josiah Gibbs.

After 1905 Einstein continued working in the areas described above. He made important contributions to quantum theory, but he sought to extend the special theory of relativity to phenomena involving acceleration. The key appeared in 1907 with the principle of equivalence, in which gravitational acceleration was held to be indistinguishable from acceleration caused by mechanical forces. Gravitational mass was therefore identical with inertial mass.

In 1908 Einstein became a lecturer at the University of Bern after submitting his Habilitation

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