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Vacuum Stability
Vacuum Stability
In the distant past, deep within the very first second after the start
of the big bang, the vacuum state of the universe has had a higher
energy than it has now. During the phase transitions that have
occurred since then, this extra energy was converted into thermal
radiation. It is conceivable that our current vacuum is still not the
lowest vacuum possible. If that is the case, a transition to a lower
vacuum state will be catastrophic: not only will it liberate enormous
amounts of energy, it will also alter the very properties of the
particles that make up all known forms of matter. Given this
dramatic, if remote, possibility, it is worthwhile to ask under which
conditions such a vacuum phase transition could be triggered.
Limits from Highest Energy Cosmic Rays
On Earth, the most energetic reactions between elementary particles
take place in collisions between the highest energy cosmic rays and
nucleons in the upper atmosphere. In the center of mass frame, such
collisions can have energies up to 1 Pev. At present, these are far
more energetic than the collisions that are produced in laboratory
accelerators, where collisions barely exceed 1 TeV. However, in
future generations of particle accelerators, energies beyond 1 PeV
could be attained, later in this century. If so, such experiments
would create conditions that have never before been achieved naturally
on Earth. Would it be possible, in principle at least, that such
experiments would threatened the vacuum as we know it?
It was this question that Martin Rees and I addressed in our paper:
Our conclusion was that there was no need to worry: plenty of
collisions between two of the highest energy cosmic ray particles have
taken place in our past light cone, with energies up to 100 Eev (100,000 Pev).
Limits from Heaviest Cosmic Rays
Although our analysis made a convincing case against the possibility
that elementary particles in accelerators could trigger a vacuum
transition, it did not directly address what would happen in
laboratories accelerating much more complex objects, such as heavy
ions. I extended our analysis to this case, in the paper:
-
Is It Safe to Disturb the Vacuum?
by Hut, P., 1984, Invited
Talk at Quark Matter '83, the Third International Conference
on Ultra-Relativistic Nucleus-Nucleus Collisions, Brookhaven, NY, September
1983, ed. T.W. Ludlam and H. Wegner (Amsterdam: North Holland Publ.); in
Nuclear Physics A418, 301c-311c.
My conclusion was that there was still no reason to worry, but that it
would be interesting to probe the composition of the highest energy
cosmic rays, in order to sharpen the limits even further.
Many years later, our results were quoted in a report commissioned by
John Marburger, then Director of Brookhaven National Laboratories, to
address various `disaster scenarios' that had been put forward, ours
being one of them. See
Review of Speculative
``Disaster Scenarios'' at RHIC, by Jaffe, R.L., Busza, W.,
Sandweiss, J., and Wilczek, F, 2000, Rev. Mod. Phys. 72, 1125-1140.
On a lighter note, around the same time physicist Gregory Benson
published a science fiction story,
Cosm
(1999, Avon Eos), about the creation of a whole new universe
through a vacuum phase transition triggered in a particle accelerator.
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