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Anomalous magnetic moment of the muon
1 March 2001
Virtual photons which are produced in reactions involving
electrons and muons modify the Lorentzian structure of lepton
currents, giving particles an anomalous magnetic moment in
addition to Dirac's one. The anomalous moment, along with the
dominant contribution from the electromagnetic interaction, also
contains weak and strong interaction contributions. Until
recently, the Standard model of particle physics
(see
Physics-Usp. 42 1193 (1999) for a discussion) was in excellent agreement
with all the experimental data - the only exception being
neutrino oscillation experiments. Now, however, the high-
precision measurement of the anomalous magnetic moment of the
muon carried out at the Brookhaven National Laboratory, US,
unexpectedly have revealed a notable deviation from the Standard
model. The reason for choosing muons - rather than more abundant
electrons - for the experiment is that effects related to the
anomalous magnetic moment are proportional to the square of mass
and therefore are stronger in the muon which is about two hundred
times as massive as the electron. Based on millions of muon (more
precisely, antimuon) decays studied using intense particle
beams, new supersensitive detectors, and powerful superconducting
magnets, it is claimed that with probability of 99% the Standard
model underpredicts the anomalous magnetic moment. One
explanation - along with possible experimental errors - could be
some effects that are unaccountable by the Standard model and are
due to the supersymmetry of the muon or its having a
substructure. The experiment is an international collaboration in
which, among other institutions, the Novosibirsk Nuclear Physics
Institute, Russia, is involved.
Source:
http://xxx.lanl.gov/abs/hep-ex/0102017,
http://www.bnl.gov/bnlweb/pubaf/pr/bnlpr020801.htm
Superconductivity in MgB2
1 March 2001
A Japanese team led by J Akimitsa found that the intermetallic
compound MgB2
(magnesium diboride) has a superconducting transition
temperature Tc=39 K, nearly twice that of other known
intermetallic compounds. On the other hand, experiments carried
out at the Ames Laboratory in the US have shown that on replacing
the boron isotope B11 by B10 the value of Tc rises by about 1 K,
consistent with what the Bardeen-Cooper-Schrieffer theory
predicts. Thus although the BCS theory is inadequate for high-
temperature ceramic superconductors, it describes well the
superconducting properties of intermetallics. While cuprate high-
temperature superconductors have the advantage of Tc exceeding 90
K, magnesium diboride is far cheaper to manufacture and holds
promise for many applications.
Source:
Physics News Update, Number 526
Chiral varieties of nuclei
1 March 2001
K Starosta of the State University of New York and his colleagues
report their observation that some atomic nuclei can exist in two
varieties, one the mirror reflection of the other. This
phenomenon has been predicted theoretically. According to theory,
chiral varieties may exist in three-dimensionally non-spherical
nuclei with odd numbers of protons and neutrons, provided a
single outer-shell proton, a single neutron, and the core spin
about the nucleus' minor axis, major axis, and the intermediate-
length axis, respectively. Such nuclei, like a triple of vectors,
may be either left- or right-handed. The SUNY experiment reveals
doublet gamma-ray emission lines for the isotones (nuclei with
the same neutron number
N)
55Cs, 57La,
59Pr
and 61Pm
with N = 75. If the
observed doublets can be interpreted as chiral vibrations, then
this experiment provides the first evidence for the existence of
stable ellipsoidal nuclei.
Source:
Phys. Rev. Lett. 86 971 (2001)
A supernova at the centre of the Galaxy
1 March 2001
Chandra observations have provided first clear images of the
remnants of the supernova explosion Sgr A East against the
background of other complex structures in the centre of our
Galaxy. New observation support the idea that layers of hot gas
enriched with heavy elements were indeed ejected as a result of a
supernova explosion. Interestingly, another object, the so-called
Sgr A* thought to be a black hole, is located within the gas
layers left over from the explosion, implying that what we are
dealing with is an example of black hole-stellar explosion
interaction at the centre of the Galaxy.
Source:
http://chandra.harvard.edu
Cosmological parameters
1 March 2001
Recent advances in microwave background anisotropy measurements
and in particular the discovery of the Doppler (Sakharov) peaks
have made possible the independent estimation of the basic
cosmological parameters that describe the evolution of the
Universe. However, much higher accuracy is achieved if, in
addition to the anisotropy information, data on the large-scale
distribution of galaxies are employed in calculations. American
astrophysicists M Tegmark, M Zaldarriaga, and A S Hamilton,
applying a new effective calculation technique to the data on
14,677 galaxies from the IRAS satellite have determined the most
likely values for 11 cosmological parameters. It was found, in
particular, that with probability 95% the cosmological constant,
dark matter (hidden mass), and the baryon matter contributes
62%, about 33%, and only 5%, respectively, to the total
cosmological density.
Source:
Phys. Rev. D 63 043007 (2001)
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The Extracts from the Internet is a section of Uspekhi Fizicheskih Nauk (Physics Uspekhi) the monthly rewiew journal of the current state of the most topical problems in physics and in associated fields. The presented News is devoted to the fundamental discoveries of physics and astrophysics. Permanent editor is Yu.N. Eroshenko. It is compiled from a multitude of Internet sources.
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