SETI bioastro: FW: Physics News Update 841

From: LARRY KLAES (ljk4_at_msn.com)
Date: Wed Oct 03 2007 - 12:14:14 PDT

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    >From: physnews_at_aip.org
    >Reply-To: physnews_at_aip.org
    >To: ljk4_at_MSN.COM
    >Subject: Physics News Update 841
    >Date: Tue, 2 Oct 2007 11:18:56 -0400
    >
    >PHYSICS NEWS UPDATE
    >The American Institute of Physics Bulletin of Physics News
    >Number 841 October 2, 2007 by Phillip F. Schewe www.aip.org/pnu
    >
    >THE VACUUM STRIKES BACK. Modern physics has shown that the vacuum,
    >previously thought of as a state of total nothingness, is really a
    >seething background of virtual particles springing in and out of
    >existence until they can seize enough energy to materialize as
    >*real* particles. In high energy collisions at accelerator labs,
    >some of the original beam energy can be consumed by ripping
    >particle-antiparticle pairs out of the vacuum. Sometimes this
    >process is the very reason for doing the experiment, but sometimes
    >it is only a detriment. For example, in the Large Hadron Collider
    >(LHC), under construction at the CERN lab in Geneva, a major source
    >of beam losses (particles exiting from the usable beam) for
    >heavy-ion collisions is expected to be a class of event in which the
    >counter-moving ions pass each other and don*t interact except to
    >spawn a pair of particles---an electron and positron---one of which
    >(the positron) goes off to oblivion while the other (the electron)
    >latches onto one of the ions. This ion, bearing an extra electric
    >charge, will now behave slightly differently as it races through the
    >chain of powerful magnets that normally steer the particles around
    >the accelerator. Going a certain distance, the modified ion will
    >leave its fellows and smash into the beam pipe carrying the beams,
    >thus heating up the pipe and surrounding magnet coils.
    >Fearing these future beam losses, accelerator physicists have sought
    >to observe this effect at an existing machine, the Relativistic
    >Heavy Ion Collider (RHIC) at the Brookhaven Lab on Long Island. And
    >they found what they were looking for, a tiny splash of energy
    >amounting to about
    >.0002 watts, or about what a firefly puts out. The RHIC beam for
    >these tests consisted of copper ions each carrying 6.3 TeV of energy
    >(about 100 GeV per nucleon). According to CERN scientist John
    >Jowett (john.jowett_at_cern.ch, 41-22-7676-643) this troublesome class
    >of events, referred to as bound-free-pair production (or BFPP, the
    >bound referring to the electron and the free to the positron), will
    >be much more formidable at LHC than at RHIC. First of all, the pair
    >production scales as the atomic number of the nucleus (or the charge
    >of the nucleus, denoted by the letter Z) raised to the seventh
    >power. The LHC heavy-ion collisions will use beams composed of lead
    >ions. The more highly charged nucleus and the larger energies (574
    >TeV per lead nucleus) mean the BFPP process should be some 100,000
    >times more prominent than in the test at RHIC. This would amount to
    >about 25 watts, the equivalent of a reading lamp. That doesn't
    >sound like much but, when deposited in the ultra-cold (1.9 K)
    >magnets of the LHC, it could bring them to the brink of "quenching"
    >out of their superconducting state, interrupting the
    >operation of the huge machine. (Bruce et al., Physical Review
    >Letters, 5 October 2007;
    >journalists can obtain the text from www.aip.org/physnews/select;
    >other background material at arxiv.org/abs/0706.3356v2),
    >http://cern.ch/AccelConf/e04/PAPERS/MOPLT020.PDF, Vol. I, Chapter 21
    >of the LHC Design Report, available at
    >http://ab-div.web.cern.ch/ab-div/Publications/LHC-DesignReport.html
    >)
    >
    >GAMMA RAYS FROM THUNDERCLOUDS have been observed by ground-based
    >detectors, providing new insights into mechanisms for accelerating
    >electrons to high energies, as high as 10 MeV, in the atmosphere.
    >Ground observations of thundercloud gammas has been made before as
    >part of monitoring regular nuclear plant operations. The new
    >measurements, ho
    >wever, represent the first time that such gamma
    >studies were made with detailed scientific objectives in mind,
    >including determinations of particle species, arrival direction, and
    >energy spectrum. On the night of 6 January 2007 two powerful
    >low-pressure air masses collided over the Sea of Japan. A nearby
    >array of gamma detectors provided information on the energy and the
    >timing of the gammas, which are the highest-category of
    >electromagnetic radiation. The array is operated by the University
    >of Tokyo and the Cosmic Radiation Laboratory of RIKEN in Japan. The
    >gamma production, the researchers believe, works like this: an
    >energetic seed electron, perhaps liberated from an atom by an
    >intruding cosmic ray, ionizes many air molecules, which in turn are
    >accelerated by the high electric fields present in the
    >thunderclouds. This flock of fast electrons can then emit gamma
    >radiation (bremsstrahlung, or *braking radiation*) as they are
    >slowed by surrounding air. The gamma production actually occurs
    >before the eventual lightning strike, says Teruaki Enoto of the
    >University of Tokyo (enoto_at_amalthea.phys.s.u-tokyo.ac.jp,
    >81-3-5841-4173), and the reason for this is not entirely known.
    >Previous thundercloud-related gammas were studied by satellite and
    >only measured very brief bursts, with durations of msec. By
    >contrast, the Tokyo-RIKEN work indicates bursting behavior that
    >could last for minutes, testifying to the quasi-static nature of the
    >acceleration mechanism at work in the clouds. The electric fields
    >in the clouds might be as high as 10 million volts. (Tsuchiya et
    >al., Physical Review Letters, upcoming article; text can be obtained
    >from www.aip.org/physnews/select )
    >
    >***********
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