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Victor Hess discovered in 1912 that the Earth is being bombarded constantly by particles from space, the cosmic rays. Many new types of fundamental particle were discovered among
the cosmic rays, including antimatter, the muon, the
pion, kaons and other strange particles. Ernest Lawrence and others realised that, in order to study
these new particles systematically, physicists had to accelerate
particles in their laboratories and examine their collisions. Many
new particles were found using these particle accelerators,
which enabled them to be understood in a well-tested Standard
Model. A comprehensive introduction to particle physics and
accelerators is available at CERN website. Matter particles can be grouped into two classes, those that
have strong nuclear forces, and those that do not. The former
are composed of point-like elementary particles called quarks,
of which six different types exist in the Universe. The particles
without strong nuclear forces are called leptons, and also come
in six varieties, including the electron, muon and a heavier but
otherwise similar electrically-charged particle (the tau), each of
which is accompanied by its own type of
neutrino. In addition to electromagnetism, gravity and the strong
nuclear forces, there are also weak nuclear forces
responsible for radioactivity. Each of these forces is due to the
exchange of other particles, the photon for electromagnetism, the
graviton (not yet seen) for gravity, the gluon for the strong nuclear
forces, and the W and Z particles for the weak nuclear forces. The Standard Model describing these forces has been verified and
tested in many experiments using particle accelerators around the
world, in particular the LEP accelerator at CERN, enabling
physicists to describe with confidence the history of the Universe
since it was about a tenth of a thousandth of a millionth of a second (10-10 sec.)
old. For example, experiments at CERN established that there exist
just three different types of neutrino, making possible accurate
calculations of the amounts of light elements created in
the first seconds of the history of the Universe. Present and future experiments at particle accelerators seek new
physics beyond the Standard Model. They search for particles that
might constitute the dark
matter in the Universe and they try to understand the small
difference between matter and antimatter, that might explain
the origin of the matter in the Universe and why it contains no large
amounts of antimatter. They also try to understand phase
transitions that might have occurred in the early Universe, and
might have analogies with cosmological
inflation. |
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Life in the Universe
Cosmology
The Big Bang
Cosmological Inflation
Cosmic Background (CMB) Radiation
Antimatter
Dark Matter
Creation of Light Elements
Particles and Accelerators
Telescopes
Missing Laws?
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Last updated August 5, 2001