Fermi addressed this the next year in a paper " Concerning a contradiction between electrodynamic and the relativistic theory of electromagnetic mass " in which he showed that the apparent contradiction was a consequence of relativity.
32.
From 1921 to 1933, the physics theory group was led by Max Born, who, during this time, became one of the three discoverers of the non-relativistic theory of quantum mechanics.
33.
The document, in paragraph 4, pointed out the danger to the Church of " relativistic theories which seek to justify religious pluralism " by denying that God has revealed truth to humanity.
34.
The second remains of interest both as an important milestone on the road to the current theory of gravitation, general relativity, and as a simple example of a self-consistent relativistic theory of gravitation.
35.
A subset of these non-relativistic theories have been further embedded within relativistic theories, which are capable of making contact with non-classical phenomena ( e . g ., gravitational lensing ) and cosmology.
36.
A subset of these non-relativistic theories have been further embedded within relativistic theories, which are capable of making contact with non-classical phenomena ( e . g ., gravitational lensing ) and cosmology.
37.
When, on the other hand, we deduce on the presence of matter sources from gravitational lensing from the usual relativistic theory, we obtain the distribution of the matter sources in the sense of the Einstein frame.
38.
Nevertheless, RQM is only an approximation to a fully self-consistent relativistic theory of known particle interactions because it does not describe cases where the number of particles changes; for example in matter creation and annihilation.
39.
For instance, the motion of a spacecraft, regarding its orbit and attitude ( rotation ), is described by the relativistic theory of classical mechanics, while the analogous movements of an atomic nucleus are described by quantum mechanics.
40.
Therefore, it is established that the classical theory ( Poisson's equation ) is the limiting case ( weak field, low velocities with respect to the speed of light ) of a relativistic theory where the metric is time-independent.
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