Unified
Field Theory
Unified Field Theory, in physics, a theory that proposes to unify
the four known interactions, or forces—the strong, electromagnetic, weak, and
gravitational forces—by a simple set of general laws. Four distinct forces are
known to control all the observed interactions in matter: gravitation,
electromagnetism, the strong force (a short-range force that holds atomic
nuclei together), and the weak force (the force responsible for slow nuclear
processes, such as beta decay). The attempts to develop a unified field theory
are grounded in the belief that all physical phenomena should ultimately be
explainable by some underlying unity.
One of the first to attempt the development of such a
theory was Albert Einstein, whose work in relativity had led him to the
hypothesis that it should be possible to find a unifying theory for the
electromagnetic and gravitational forces. Einstein tried unsuccessfully during
the last 30 years of his life to develop a theory that would represent forces
and material particles by fields only, in which particles would be regions of
very high field intensity. The development of quantum theory, which Einstein
rejected, and the discovery of many new particles, however, precluded
Einstein's success in formulating a unifying theory based on relativity and
classical physics alone.
An important advance in this quest was made in 1967-68 by the
American physicist Steven Weinberg and the Pakistani physicist Abdus Salam. They succeeded in
unifying the weak interaction and the electromagnetic interaction by using a
mathematical technique known as gauge symmetry (see Elementary
Particles). According to this theory the electromagnetic interaction consists
of the exchange of a photon, and the weak interaction of the exchange of W and
Z intermediate bosons. These bosons are believed to belong to the same family
of particles as the photons. Theoretical physicists are currently attempting to
combine this so-called electroweak theory with the strong nuclear force, using
symmetry theories; such attempts are known as grand unification theories, or GUTs. The effort also continues to combine all four
fundamental interactions, including gravitation, in what are now known as supersymmetry theories. Thus far, however, such attempts
have not succeeded, although they are proving useful in current work in
cosmology (see Inflationary Theory).
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unified field theory
in particle physics, an attempt to
describe all fundamental forces and the relationships between elementary
particles in terms of a single theoretical framework. In physics, forces can be
described by fields that mediate interactions between separate objects. In the
mid-19th century James Clerk Maxwell formulated the first field theory
in his theory of electromagnetism. Then, in the early part of the 20th
century, Albert Einstein developed general
relativity, a field theory of gravitation. Later, Einstein and
others attempted to construct a unified field theory in
which electromagnetism and gravity would emerge as different aspects of a
single fundamental field. They failed, and to this day gravity remains
beyond attempts at a unified field theory.
At subatomic
distances, fields are described by quantum field theories, which apply
the ideas of quantum mechanics to the fundamental field. In the 1940s quantum electrodynamics (QED), the
quantum field theory of electromagnetism, became fully developed.
In QED, charged particles interact as they emit and absorb photons (minute
packets of electromagnetic radiation), in effect
exchanging the photons in a game of subatomic "catch." This theory
works so well that it has become the prototype for theories of the other
forces.
During the 1960s
and '70s particle physicists discovered that matter is composed of two types of
basic building block--the fundamental particles known as quarks and leptons. The quarks are always
bound together within larger observable particles, such as protons and
neutrons. They are bound by the short-range strong force, which overwhelms
electromagnetism at subnuclear distances. The
leptons, which include the electron, do not "feel" the strong force.
However, quarks and leptons both experience a second nuclear force, the weak force. This force, which is
responsible for certain types of radioactivity classed together as beta decay,
is feeble in comparison with electromagnetism.
At the same time
that the picture of quarks and leptons began to crystallize, major advances led
to the possibility of developing a unified theory. Theorists
began to invoke the concept of local gauge invariance, which postulates
symmetries of the basic field equations at each point in space and time
(see gauge theory). Both
electromagnetism and general relativity already involved such symmetries, but
the important step was the discovery that a gauge-invariant quantum field
theory of the weak force had to include an additional
interaction--namely, the electromagnetic interaction. Sheldon Glashow, Abdus Salam,
and Steven Weinberg independently
proposed a unified "electroweak" theory
of these forces based on the exchange of four particles: the photon for electromagnetic
interactions, and two charged W particles and a neutral Z
particle for weak interactions.
During the 1970s
a similar quantum field theory for the strong force, called quantum chromodynamics
(QCD), was developed. In QCD, quarks interact through the exchange of particles
called gluons. The aim of researchers now is to discover whether the strong
force can be unified with the electroweak force in a grand unified
theory (GUT). There is evidence that the strengths of the different
forces vary with energy in such a way that they converge at high energies.
However, the energies involved are extremely high, more than a million million times as great as the energy scale of electroweak
unification, which has already been verified by many experiments.
Grand unified
theories describe the interactions of quarks and leptons within the same
theoretical structure. This gives rise to the possibility that quarks can decay
to leptons and specifically that the proton can decay. Early attempts at
a GUT predicted that the proton's lifetime must be in the region of 1032
years. This prediction has been tested in experiments that monitor large
amounts of matter containing on the order of 1032 protons, but there
is no evidence that protons decay. If they do in fact decay, they must do so
with a lifetime greater than that predicted by the simplest GUTs.
There is also evidence to suggest that the strengths of the forces do not
converge exactly unless new effects come into play at higher energies. One such
effect could be a new symmetry called "supersymmetry."
A successful GUT
will still not include gravity. The problem here is that theorists do not yet
know how to formulate a workable quantum field theory of gravity
based on the exchange of a hypothesized graviton. See also quantum field theory.