Since the 1800s, some physicists have attempted to develop a single theoretical
framework that can account for the fundamental
forces of nature – a unified field theory. Classical unified
field theories are attempts to create a unified field theory based on classical physics.
In particular, unification of gravitation and electromagnetism was actively pursued by
several physicists and mathematicians in the years between World War I and World War II. This work
spurred the purely mathematical development of differential geometry. Albert Einstein is the
best known of the many physicists who attempted to develop a classical unified
field theory.When the equivalent of Maxwell's equations for electromagnetism
is formulated within the framework of Einstein's theory of general
relativity, the electromagnetic field energy (being equivalent to mass as
one would expect from Einstein's famous equation E=mc2) contributes
to the stress tensor and thus to the curvature of space-time, which is the
general-relativistic representation of the gravitational field; or putting it
another way, certain configurations of curved space-time incorporate
effects of an electromagnetic field. This suggests that a purely geometric
theory ought to treat these two fields as different aspects of the same basic
phenomenon. However, ordinary Riemannian geometry is unable to describe
the properties of the electromagnetic field as a purely geometric
phenomenon.
Einstein tried to form a generalized theory of gravitation that would unify
the gravitational and electromagnetic forces (and perhaps others), guided by a
belief in a single origin for the entire set of physical laws. These attempts
initially concentrated on additional geometric notions such as vierbeins and
"distant parallelism", but eventually centered around treating both the metric tensor and the affine connection
as fundamental fields. (Because they are not independent, the metric-affine
theory was somewhat complicated.) In general relativity, these fields are symmetric (in the
matrix sense), but since antisymmetry seemed essential for electromagnetism, the
symmetry requirement was relaxed for one or both fields. Einstein's proposed
unified-field equations (fundamental laws of physics) were generally derived
from a variational principle expressed in terms
of the Riemann curvature tensor for the
presumed space-time manifold.
In field theories of this kind, particles appear as limited regions in
space-time in which the field strength or the energy density are particularly
high. Einstein and coworker Leopold Infeld managed to demonstrate that, in
Einstein's final theory of the unified field, true singularities of the field did have
trajectories resembling point particles. However, singularities are places where
the equations break down, and Einstein believed that in an ultimate theory the
laws should apply everywhere, with particles being soliton-like solutions to the (highly nonlinear) field
equations. Further, the large-scale topology of the universe should impose
restrictions on the solutions, such as quantization or discrete symmetries.
The degree of abstraction, combined with a relative lack of good mathematical
tools for analyzing nonlinear equation systems, make it hard to connect such
theories with the physical phenomena that they might describe. For example, it
has been suggested that the torsion (antisymmetric part of the affine
connection) might be related to isospin rather than electromagnetism; this is related
to a discrete (or "internal") symmetry known to Einstein as "displacement
field duality".
Einstein became increasingly isolated in his research on a generalized theory
of gravitation, and most physicists consider his attempts ultimately
unsuccessful. In particular, his pursuit of a unification of the fundamental
forces ignored developments in quantum physics (and vice versa), most notably
the discovery of the strong nuclear force and weak nuclear force.
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