The earth is constantly being bombarded by particles, cosmic rays, coming from space. They strike the top of the atmosphere giving rise to showers of particles raining down on us all the time. All over the world, several hundred of these particles pass through every square metre of the earth at sea level. Our atmosphere gives protection essential for life against most of the radiation that could bring about biological damage.
The particle composition of cosmic rays is rather diverse and includes neutrinos, photons, electrons, protons and atomic nuclei up to as heavy as lead.
The 1987A supernova
A possible black hole in the centre of the NGC4261C galaxy
Most cosmic ray particles have energies up to a few million electron Volts, 106 eV. Recently, however, very energetic ones with energies of 1020 eV have been observed! To explain these incredible energies we must imagine anything from super-powerful cosmic explosions, to super-massive black holes or perhaps some unkown giant relics from the origin of the Universe. It's very possible that these high-energy cosmic rays hold secrets of the evolution and perhaps even of the origin of the Universe.
The Universe is like a giant particle accelerator, driving particles to energies far higher than we can achieve in laboratories on earth. Such energies are of great interest to physicists. In fact, until the 1950s cosmic rays were behind most important particle physics discoveries.
But cosmic rays are unpredictable and with the advent of particle accelerators, most particle physics research transferred to laboratories like CERN. Cosmic ray physics, however, is still important for energies beyond the reach of accelerators. The highest energy cosmic rays, those that reach 1020 eV, some 100 million times higher than even the most powerful laboratory accelerators, are generating a new wave of interest in cosmic ray physics. However, while these sources provide energies far beyond those of our accelerators, the rates are extremely low. Above 1018 eV we expect only one particle per square kilometre of the earth's atmosphere per week. Above 1020 eV we expect just one particle to fall on each square kilometre in 100 years!
The primary goal of cosmic ray studies is to understand the sources, the acceleration mechanisms and propagation of cosmic particles through the galaxy. Physicists also hope that new particles might be discovered in high energy cosmic ray interactions, particles that require too much energy for laboratory accelerators to make. Another strand of cosmic ray research analyzes cosmic rays from particular sources to learn about what goes on inside them.
One specific goal is to identify the particles that make up the mysterious Dark Matter in the Universe. We know that visible matter accounts for just 10% of all the mass in the Universe, but so far we don't know what the other 90% is made of! Cosmic ray studies have indicated that the elusive neutrinos could have a tiny mass. If they do, they could account for a significant fraction of the Dark Matter simply because there are so many of them.
Yet another goal of cosmic ray physics is to investigate the belief that the Universe is made of matter, containing almost no antimatter at all. Just one atom of something like anti-oxygen detected in cosmic rays would be proof that large regions of antimatter do exist in space because an anti-star would have been needed to cook up that single anti-atom. So far no such anti-atoms have been found and physicists believe that the asymmetry between matter and antimatter arises from a slight preference that nature seems to have for matter.
In all of these questions, cosmic ray physics and laboratory-based accelerator studies play complementary roles.
|Introduction to Accelerators|
|Particle Physics Education CD-ROM ©1999 CERN|