-Caveat Lector-   <A HREF="http://www.ctrl.org/">
</A> -Cui Bono?-

http://www.nytimes.com/library/national/science/021900sci-dark-matter
.html


 Evidence of Mystery Particles Stirring
 Excitement and Doubt

 By JAMES GLANZ

 February 19, 2000

 A team of physicists based at the University of Rome
 has generated both intense excitement and profound
 skepticism among scientists around the world by
 presenting evidence that they may have detected a
 heavy particle that could solve a 70-year-old
 mystery in astronomy and lead to a conceptual
 breakthrough in physics.

 The presumed particles would weigh at least 50 times
 as much as a proton and would almost always pass
 through other matter without a trace because of an
 extremely weak ability to interact with it.  The new
 evidence, which so far has not been confirmed by
 other scientists, would suggest that space is
 swarming with enough of the particles to account for
 the long-sought "dark matter" that astronomers
 believe makes up some 80 percent of all the mass in
 the universe.

 Though astronomers have been measuring the
 gravitational pull of the dark matter since the
 1930's, they have never succeeded in detecting it
 directly.

 A particle like the one that may have been found
 could also be part of an entire family of
 still-undiscovered particles predicted by an
 advanced theory of physics called supersymmetry.
 Many physicists regard supersymmetry as a possible
 first step toward an ultimate theory that would
 account for all the known forces and particle
 behaviors in nature -- marrying quantum theory and
 gravity, for example.

 "If this is right, this is clearly one of the great
 discoveries of the last hundred years," said Dr.
 Michael Turner, a cosmologist at the University of
 Chicago.  "To discover that most of the matter in
 the universe is not what we're made of -- that's
 pretty spectacular."

 But a number of scientists, including Dr. Turner,
 said it was still unclear whether the finding was
 correct.

 A member of the team, Dr. Pierluigi Belli, is
 scheduled to present the results next Friday in
 Marina del Rey, Calif., at the Fourth International
 Symposium on Sources and Detection of Dark Matter in
 the Universe.  But this week, the team made a paper
 describing the possible detection of the particle,
 variously called a neutralino and a weakly
 interacting, massive particle, or WIMP, available on
 its public Web site (http://www.lngs.infn.it).

 According to the paper, whose lead author is Dr.
 Rita Bernabei, a "cumulative analysis" of data
 collected over three years in an underground
 experiment at the Gran Sasso National Laboratory
 east of Rome "favors the possible presence of a
 WIMP."  The group came to its conclusion by noting
 seasonal variations in the counts registered on
 their detector, as expected if Earth is passing
 through a cloud of the particles in its orbit.

 "They have, clearly, a seasonal variation," said Dr.
 Bernard Sadoulet, an astrophysicist at the
 University of California at Berkeley, who has read
 the team's paper.

 Dr. Sadoulet, with Dr. Blas Cabrera of Stanford
 University and Dr. David O. Caldwell of the
 University of California at Santa Barbara, leads
 another group that will make the first public
 presentation of the results of its own search for
 dark matter at the same conference.

 But Dr. Sadoulet added that "there is a lot of
 skepticism in the community" as to whether the Rome
 group has really detected the elusive WIMP.  He said
 that unrelated seasonal effects, such as temperature
 variations around the sensitive detectors or changes
 in levels of natural radioactivity, could still be
 mimicking the expected signal.

 In response to questions by e-mail, Dr. Bernabei
 wrote that "all known sources" of such effects had
 been thoroughly analyzed in the paper.  She also
 pointed out that the new results showed "full
 compatibility" with the team's earlier, published
 results, based on less data, which suggested a WIMP
 of about the same size.

 Dr. Frank Avignone, a physicist at the University of
 South Carolina who has visited the Gran Sasso
 laboratory, said that "the experiment, the
 apparatus, has been constructed very carefully."
 Dr. Avignone added, "I'm not willing to say, 'No, I
 don't believe it,' " although he also expressed
 doubt that the measurement could be considered
 definitive.

 Dr. Avignone said that if correct, the finding
 "would definitely be at the level of a Nobel Prize."

 Eight of the scientists listed as authors on the
 team's new paper, including Dr. Bernabei and Dr.
 Belli, are affiliated with both the University of
 Rome and the National Institute of Nuclear Physics
 in Italy.  In addition, four authors are identified
 as members of the Institute of High Energy Physics
 of the Chinese Academy of Sciences in Beijing.

 Based on decades of indirect evidence, astronomers
 are all but certain that dark matter makes up the
 vast majority of all matter in the universe.
 Without the gravitational pull of the dark matter,
 clusters of galaxies would fly apart, since the
 galaxies are generally orbiting around each other
 too quickly to be held by the gravity of observable
 matter.

 The gravity of the dark matter is also thought to
 prevent individual galaxies from breaking to pieces.

 Moreover, astronomers have noted the presence of the
 dark matter's powerful gravity by observing the way
 that it bends light rays, as it should according to
 Einstein's theory of relativity.

 But because the matter seems utterly invisible,
 astronomers believe that the dark matter is very
 different from the ordinary stuff of which stars,
 planets and people are made.  Cosmologists studying
 how all matter was presumably created in the Big
 Bang, the explosion in which the universe is thought
 to have been born, have come to similar conclusions
 about the dark matter.

 Interacting only weakly among each other and with
 ordinary matter, dark matter WIMPs are thought to
 clump like an immense cloud or gas around the
 visible, starry parts of galaxies.  Called a halo,
 this structure may extend for hundreds of thousands
 of light years into space beyond the visible disk of
 a galaxy like the Milky Way.

 About one WIMP of the kind possibly found by the
 Rome group would exist in a volume of space the size
 of a coffee cup.  But because the sun is orbiting
 around the center of the Milky Way at a speed of
 about 140 miles per second, through the clouds of
 WIMPs, "a billion of them would be passing through
 your body every second," said Dr. Leszek Roszkowski,
 a particle physicist at Lancaster University in
 England.  "And yet you would not be able to detect
 them."

 Rarely, however, a WIMP should interact with
 ordinary matter in a collision.  The Rome group set
 about trying to detect the WIMPs with a material
 called sodium iodide, which scintillates, or emits
 tiny flashes of light, when particles collide with
 it.  The detector is underground in order to shield
 it from showers ordinary particles from space called
 cosmic rays.

 And to be sure that they were seeing the WIMPs, the
 group looked for a rise and fall of the rate of
 detections over the course of the seasons.  Because
 of the way in which Earth is orbiting the sun, which
 is itself in orbit around the galactic center, the
 detectors should sense a "wind" of WIMPs that is
 slightly stronger in the summer than the winter.

 It is as if a child on a merry-go-round were
 whirling a ball on a string.  The wind resistance on
 the ball would be greatest when it was moving in the
 same direction as the merry-go-round, and the least
 when moving in the opposite direction.  In the WIMP
 experiments, the expected difference over a year
 would amount to "roughly 5 percent in the detection
 rate," Dr. Roszkowski said.

 It is an observation of this seasonal variation, or
 modulation, that the Rome group is reporting in its
 paper, he said.  The most likely WIMP mass indicated
 by the results is about equal to that of 60 protons,
 or an entire atom of nickel.

 But Dr. Roszkowski added that because many processes
 vary with the seasons on Earth, and because the
 expected modulation is so slight, minor errors in
 the analysis could produce a false signal.  "They
 are probing uncharted waters," he said.  "Skepticism
 is the most healthy attitude in this respect."

 He and other scientists pointed out that several
 other dark matter experiments, including those of
 the Berkeley group, have begun collecting data and
 the correctness of the result could be tested
 quickly.

 But there is no questioning the impact of the
 discovery if it holds water, said Dr. David B.
 Cline, the physicist at the University of California
 at Los Angeles who is organizing the conference in
 Marina del Rey.

 "The Copernican revolution told us we're not the
 center of the universe," Dr. Cline said.  "This
 tells us we're not the matter of the universe."
 Intellectually, he said, the development "is just
 the tip of an incredible iceberg, if this is right."



 Copyright 2000 The New York Times Company

<A HREF="http://www.ctrl.org/">www.ctrl.org</A>
DECLARATION & DISCLAIMER
==========
CTRL is a discussion & informational exchange list. Proselytizing propagandic
screeds are not allowed. Substance�not soap-boxing!  These are sordid matters
and 'conspiracy theory'�with its many half-truths, misdirections and outright
frauds�is used politically by different groups with major and minor effects
spread throughout the spectrum of time and thought. That being said, CTRL
gives no endorsement to the validity of posts, and always suggests to readers;
be wary of what you read. CTRL gives no credence to Holocaust denial and
nazi's need not apply.

Let us please be civil and as always, Caveat Lector.
========================================================================
Archives Available at:
http://home.ease.lsoft.com/archives/CTRL.html

http:[EMAIL PROTECTED]/
========================================================================
To subscribe to Conspiracy Theory Research List[CTRL] send email:
SUBSCRIBE CTRL [to:] [EMAIL PROTECTED]

To UNsubscribe to Conspiracy Theory Research List[CTRL] send email:
SIGNOFF CTRL [to:] [EMAIL PROTECTED]

Om

Reply via email to