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| subject: | PhysNews 642 01/02 |
PHYSICS NEWS UPDATE The American Institute of Physics Bulletin of Physics News Number 642 June 18, 2003 by Phillip F. Schewe, Ben Stein, and James Riordon INTRIGUING ODDITIES IN HIGH-ENERGY NUCLEAR COLLISIONS. Missing debris in the smashup between gold nuclei going at close to the speed of light suggests the creation of a highly unusual plasma environment, researchers have announced at Brookhaven National Laboratory. By smashing together gold ions at Brookhaven's Relativistic Heavy Ion Collider (RHIC), scientists are attempting to make and study a state of matter that existed only millionths of a second after the big bang. Called a quark-gluon plasma (QGP), it is a hot, dense soup of individual quarks and gluons. In today's universe, by contrast, quarks come in groups of twos and threes, held together by gluons. This spring, Brookhaven researchers performed a "control" experiment, in which they collided a gold nucleus with a deuteron, a light nucleus consisting of just a proton and neutron. In these and other kinds of nuclear collisions, a pair of quarks from a proton or neutron occasionally gets ejected. In turn each ejected quark produces a stream or "jet" of particles in its wake. In some of the gold-deuteron collisions, the researchers indeed observed pairs of jets flying in opposite directions. But in head-to-head collisions between two gold nuclei, researchers observed only one, rather than two, jets. This property, called jet quenching, suggests that the particle jet traveling in the direction of the collision region is getting absorbed by a hot, dense state of matter. Jet quenching is predicted to occur in the correspondingly hot, dense environment of a quark-gluon plasma, but RHIC experimentalists are not ready to claim the QGP prize quite yet. To verify its presence and rule out rival scenarios, they are planning numerous other experiments for finding other signatures of a QGP. However, the new data has convinced Columbia theorist Miklos Gyulassy that the RHIC team is already seeing a QGP (see http://www-cunuke.phys.columbia.edu/people/gyulassy/Welcome.html). The gold-gold collisions, he and his colleagues calculate, produce an environment 100 times denser than ordinary nuclear matter and display properties predicted in QGP models based on quantum chromodynamics (QCD), the theory of the strong force which holds nuclei together. On June 18, three of the four RHIC experimental groups have submitted papers on the new results to Physical Review Letters and researchers discussed these new results at a special Brookhaven colloquium today. (Brookhaven press release, June 11, http://www.bnl.gov/bnlweb/pubaf/pr/2003/bnlpr061103.htm.) SOLAR FLARES AND GLOBAL WARMING. A recent study by researchers at Duke University and the Army Research Office has found new evidence of a link between solar flare activity and the earth's temperature. The work is another contribution to the ongoing debate over global warming and its causes. A strong link between solar flares and our climate, if it exists, could override the influence humans have on the temperature of our environment. One of the challenges of determining the connection between solar flare activity and the atmosphere stems from the fact that the motion of the air that blankets our planet is turbulent and complex. A sudden burst of solar activity would, in effect, be smeared out by moving air and its interaction with the earth's surface. Any temperature increase caused by a given period of solar flare activity would be difficult to determine, at best. Rather than focus on such challenging one-to-one correlations, the new study compares the form of the statistical fluctuations in solar flare activity with the form of the statistical fluctuations of the earth's temperature. The researchers (contact: Bruce J. West, Bruce.J.West{at}us.army.mil, 919-549-4257) explain that solar flare activity can be characterized by a type of statistics described by a Levy distribution, which is generated by a "Levy-walk." (Many natural phenomena, from foraging patterns of spider monkeys to complex hydrodynamic flows, are well described by Levy walks, although the coefficients in the relevant equations typically vary from one phenomenon to another. See Update 510-3 for one example.) Analyses of global and local temperature fluctuations are also well described by a Levy-walk. In fact, a comparison of the mathematical coefficients that describe the fluctuations suggest to the researchers that the atmosphere directly inherits its temperature fluctuations from the variation in solar flare activity. Unless some other underlying cause is responsible for the unlikely correspondence between solar flares and the earth's temperature, the research suggests that for the large part variations in global temperatures are beyond our control and are instead at the mercy of the sun's activity. (Nicola Scafetta and Bruce J. West, Physical Review Letters, 20 June 2003) STAR OUT OF ROUND. The Very Large Telescope Interferometer (VLTI), an array of 2 telescopes which combine their light signals to achieve a higher angular resolution than is possible with any one scope, has determined that the star Achernar is the flattest star ever studied. The VLTI, which does not provide an actual image of the star but can provide an accurate estimate of the star's profile, has determined that Achernar's equatorial radius is 50% larger than its polar radius. This is quite oblate compared to most other celestial bodies, such as our Earth, whose equatorial radius is only 0.3% larger than its polar radius. Theorists do not yet know how to explain how a star like this could turn fast enough to adopt with such a shape without flying apart. Achernar is about 145 light years (Continued to next message) --- þ OLXWin 1.00b þ Error number 324656: Program has too many comments.* Origin: Try Our Web Based QWK: DOCSPLACE.ORG (1:123/140) SEEN-BY: 633/267 270 @PATH: 123/140 500 106/2000 633/267 |
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