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2Physics Quote:
"Stars with a mass of more than about 8 times the solar mass usually end in a supernova explosion. Before and during this explosion new elements, stable and radioactive, are formed by nuclear reactions and a large fraction of their mass is ejected with high velocities into the surrounding space. Most of the new elements are in the mass range until Fe, because there the nuclear binding energies are the largest. If such an explosion happens close to the sun it can be expected that part of the debris might enter the solar system and therefore should leave a signature on the planets and their moons." -- Thomas Faestermann, Gunther Korschinek (Read Full Article: "Recent Supernova Debris on the Moon" )

Tuesday, September 06, 2005

Bose-Einstein condensate













About 80 years ago, based on previous work by the Indian physicist
Satyendra Nath Bose, Einstein proposed that if a gas of neutral atoms is
cooled to a low enough temperature, all atoms of the gas would fall into the
same quantum state. In other words, all of the million or billion atoms in
the gas would end up in the same place at the same time, a weird quantum
state dubbed a Bose-Einstein condensate.

The supercold atoms are created from a hot gas of neutral atoms that is
laser cooled, collected in a magneto-optic trap, cooled further by evaporation,
and then spun off into a magnetic trap for a few seconds of study before it
warms up and dissipates.

A team of physicists at UC Berkeley has created a Bose-Einstein condensate
of rubidium atoms and nudged it into a circular racetrack 2 millimeters
across, creating a particle storage ring analogous to the accelerator storage
rings of high energy physics. This ring, the first to contain a Bose-Einstein gas,
is full of cold particles at a temperature of only one-millionth of a degree
above absolute zero (which is -273 degree centigrade), traveling with
energies a billion trillion times less than the particles in a high-energy storage
ring [The atoms circled the racetrack at a speed of about 50 to 150 millimeters
per second, which is equal to an energy of about one nano-electron volt (eV)
per atom, or one billionth of an electron volt. High-energy particle accelerators
routinely bump particles to energies of a few tera-electron volts, or a trillion
eV - a billion trillion times more energetic than the cold rubidium atoms].

Though such slow-moving rubidium atoms would be useless for producing
the exotic collision particles that are the bread and butter of high-energy
accelerators, cold collisions of such atoms might reveal new quantum physics,
said Dan Stamper-Kurn, assistant professor of physics at UC Berkeley and
leader of the study. Their paper was accepted for publication by Physical
Review Letters last week.

Useful Sites:
http://www.colorado.edu/physics/2000/bec/index.html
http://en.wikipedia.org/wiki/Bose-Einstein_condensate

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