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A substantial part of the research of Albert Einstein in the first half of the
20th century was devoted to a derivation of a unified field theory in the context of general relativity
(Sachs, 1982). This theory incorporates the explanation of the physical phenomena
of gravitation and electromagnetism under a single umbrella. It is well-known that he did
not succeed in this pursuit, though he was aware that the logical basis of the theory of
relativity implies such unification.
The unified field theory sought by Einstein (1955) and Schrödinger (1954) was meant
to reformulate the variables of the field theory into a single field that incorporates
the gravitational and the electromagnetic variables in a single (16-component) field. It is
well-known that their attempts were not successful. Still, it was clear to Einstein
and Schrodinger that the unified field theory is implied by the logical basis of the theory
of general relativity. Then, how was it to be formulated?
The spacetime points (the `words' of this language) form a continuous set. The principle of relativity then implies that the transformations of the expression of the laws from one perspective in spacetime (i.e., one reference frame) to another `continuously connected' spacetime point preserves the forms of the laws of nature. Thus the laws of nature must be continuously distributed-they are `field equations' rather than equations of the motion of point particles (as in classical physics). The first discovered set of such field equations was Maxwell's equations for electromagnetism. Thus, the variables which are the solutions of the laws of nature, are `continuous fields'. It is further postulated, according to Noether's theorem, that the inclusion of the laws of conservation (of energy, momentum and angular momentum), in the flat space limit, is that the transformations of the laws of nature between reference frames must be analytic. This is a necessary and sufficient condition. Thus, the field solutions of the laws of nature are `regular'-continuous functions, without any singularities `anywhere'.
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