Adapted from P. Coles, 1999, The Routledge Critical
Dictionary of the New Cosmology, Routledge Inc., New York. Reprinted
with the author's permission. To order this book click here:
http://www.routledge-ny.com/books.cfm?isbn=0415923549
The four ways in which the various elementary
particles interact with one another: electromagnetism, the weak
nuclear force, the strong nuclear force and gravity. They vary in
strength (gravity is the weakest, and the strong nuclear force is the
strongest) and also in the kinds of elementary particle that take
part.
The electromagnetic interaction is what causes particles of opposite
charge to attract each other, and particles of the same charge to
repel each other, according to the Coulomb law of
electrostatics. Moving charges also generate magnetic fields which, in
the early history of physics, were thought to be a different kind of
phenomenon altogether, but which are now realised to be merely a
different aspect of the electromagnetic force. James Clerk Maxwell was
the first to elucidate the character of the electromagnetic
interactions. In this sense, Maxwell's equations were the first
unified physical theory, and the search for laws of physics that unify
the other interactions is still continuing (see grand unified
theories, theory of everything).
The theory of electromagnetism was also an important step in another
direction. Maxwell's equations show that light can be regarded as a
kind of electromagnetic radiation, and demonstrate that light should
travel at a finite speed. The electromagnetic theory greatly impressed
Albert Einstein, and his theory of special relativity was
constructed
specifically from the requirement that Maxwell's theory should hold
for observers regardless of their velocity. In particular, the speed
of light had to be identical for all observers, whatever the relative
motion between emitter and receiver.
The electromagnetic force holds electrons in orbit around atomic
nuclei, and is thus responsible for holding together all the material
with which we are familiar. However, Maxwell's theory is a classical
theory, and it was realised early in the 20th century that, in order
to apply it in detail to atoms, ideas from quantum physics would have
to be incorporated. It was not until the work of Richard Feynman that
a full quantum theory of the electromagnetic force, called quantum
electrodynamics, was developed. In this theory, which is usually
abbreviated to QED, electromagnetic radiation in the form of photons
is responsible for carrying the electromagnetic interaction between
particles.
The next force to come under the spotlight was the weak nuclear
force, which is responsible for the so-called beta decay of certain
radioactive isotopes. It involves elementary particles belonging to
the lepton family (which includes electrons). As with
electromagnetism, weak forces between particles are mediated by other
particles - not photons, in this case, but massive particles called
the W and Z bosons. The fact that these particles have
mass (unlike
the photon) is the reason why the weak nuclear force has such a short
range. The W and Z particles otherwise play the same role in this
context as the photon does in QED: they are all examples of gauge
bosons (see gauge theory). In this context, the particles that
interact are always fermions, while the particles that carry the
interaction are always bosons.
A theory that unifies the electromagnetic force with the weak
nuclear force was developed in the 1960s by Sheldon Glashow, Abdus
Salam and Steven Weinberg. Called the electroweak theory, it
represents these two distinct forces as being the low-energy
manifestations of a single force. At high enough energies, all the
gauge bosons involved change character and become massless entities
called intermediate vector bosons. That electromagnetism and the weak
force appear so different at low energies is a consequence of
spontaneous symmetry-breaking.
The strong nuclear interaction (or strong force) involves the hadron
family of elementary particles, which includes the baryons (protons
and neutrons). The theory of these interactions is called quantum
chromodynamics (QCD) and it is built upon similar lines to the
electroweak theory. In QCD there is another set of gauge bosons to
mediate the force: these are called gluons. There are eight of them,
and they are even more massive than the W and Z particles. The strong
force is thus of even shorter range than the weak force, Playing the
role of electric charge in QED is a property called `colour'. The
hadrons are represented as collections of particles called quarks,
which have a fractional electrical charge and come in six different
`flavours': up, down, strange, charmed, top and bottom. Each distinct
hadron species is a different combination of the quark flavours.
The electroweak and strong interactions coexist in a combined theory
of the fundamental interactions called the standard model. This model
is, however, not really a unified theory of all three interactions,
and it leaves many questions unanswered. Physicists hope eventually to
unify all three of the forces discussed so far in a single grand
unified theory. There are many contenders for such a theory, but it is
not known which (if any) is correct.
The fourth fundamental interaction is gravity, and the best theory
of it is general relativity. This force has proved extremely resistant
to efforts to make it fit into a unified scheme of things. The first
step in doing so would involve incorporating quantum physics into the
theory of gravity in order to produce a theory of quantum
gravity. Despite strenuous efforts, this has not yet been achieved. If
this is ever done, the next task will be to unify quantum gravity with
the grand unified theory. The result of this endeavour would be a
theory of everything. The difficulty of putting the theory of
interactions between elementary particles (grand unified theories)
together with the theory of space and time (general relativity) is the
fundamental barrier to understanding the nature of the initial stages
of the Big Bang theory.
FURTHER READING:
Roos, M., Introduction to Cosmology, 2nd edition (John Wiley,
Chichester, 1997), Chapter 6.
Davies, P.C.W., The Forces of Nature (Cambridge University Press,
Cambridge, 1979).
Pagels, H.R., Perfect Symmetry (Penguin, London, 1992).
FUNDAMENTAL INTERACTIONS