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Photon splitting in the field of the atomic nucleus
1 August 2002
Researchers at the Budker Institute of Nuclear Physics in
Novosibirsk, Russia, performed an experiment which for the first
time detected the splitting of photons in the field of the atomic
nucleus. The mechanism of this splitting differs in a fundamental
way from the nonlinear-optics effect of photon splitting in a
crystal. A high-energy photon in the field of a nucleus
transforms into a virtual electron-positron pair, one member of
this pair emits a new photon, and the annihilation of the pair
gives rise to a second photon. Although this process has been
sought since 1966, previous experiments have not produced
definitive results and disagreed with theoretical calculations.
The Novosibirsk experiment used a beam of photons with energies
in the range 120-450 MeV generated by the backward Compton
scattering of laser radiation by an accelerator-produced electron
beam. The photon beam was passed through a nuclear target. At the
exit side of the target specially designed detectors were placed
which, based on the correlation properties of the events
involved, detected photon pairs resulting from the splitting of
single photons in the field of target nuclei. Among the # photons
studied, about 400 such pairs were found, in exact agreement with
theoretical calculations. Source:
Phys. Rev.
Lett. 89 061802 (2002)
Chemical transformations in sonoluminescence
1 August 2002
Sonoluminescence refers to the emission of light due to the
collapse of gas bubbles in a liquid under the action of
ultrasound. While several explanations of this effect have been
proposed, the mechanism of the emission is not yet completely
understood. Yu Didenko and K Suslick at the University of
Illinois in the US performed an experiment in which they
carefully monitored the chemical composition of single collapsing
air bubbles in water. The results of the study point to the
conclusion that the emission is due to chemical reactions
occurring in bubbles. The gas in a collapsing bubble is heated to
a temperature of from 10,000 to 20,000 K. Under these conditions,
the rapid synthesis of NO2 radicals and OH occurs. It is part of the
energy involved in these chemical processes which transforms into
light. Source:
Nature 418 394 (2002)
Cosmological limit on the neutrino mass
1 August 2002
While neutrino oscillation experiments (see Physics-Uspekhi 45 700
(2002)) have provided evidence that neutrinos have rest mass, so
far only mass differences between various kinds of neutrinos
have been measured. Other experimental estimates do give the
upper limit of m<1-20eV but have poor accuracy. The most reliable
estimate yet follows from cosmology. When already out of
equilibrium with electromagnetic radiation, these particles
remained relativistic for some period of time and so managed to
travel a large distance l, which depends on its mass. Therefore
cosmological density perturbations at scales less than l have
smoothed out somewhat. This smoothing out affects the spatial
distribution of galaxies. A team of British, Australian, and
American scientists have performed an analysis of the largest 2dF
Galaxy Survey that catalogues 220,000 galaxies. The analysis of
the galaxies' correlation properties showed that the contribution
from the neutrino to the cosmological density of matter does not
exceed 13% and that sum of the three neutrino masses is at
most 1.8 eV. Source:
Phys. Rev. Lett. 89 061301 (2002)
Masses of black holes in quasars
1 August 2002
To date, astronomers have discovered several quasars with
redshifts z>5.8, i. e., quasars that existed at the epoch when
the age of the universe did not exceed one billion years.
Radiation emitted by a quasar is generated in the interior of an
accretion disk close to a black hole at the centre of a galaxy.
From the luminosity of the quasar one can estimate the mass of
the black hole, which in some cases is more than three billion
times the mass of the sun. Thus far theory has been unable to
convincingly explain how such massive black holes could possibly
form at an early epoch. Now, J S B Wyithe and A Loeb of Harvard
University have apparently settled the issue by showing that
black holes in distant quasars have masses 10 to 100 times less
than previously believed. The important factor which J S B Wyithe
and A Loeb have taken into account is the gravitational lensing
of quasars by foreground galaxies. According to Wyithe and Loeb's
calculations, about one third of all quasars at redshifts z>5.8
might have been lensed. When a quasar is lensed its apparent
luminosity increases. Therefore the real luminosity is less than
that observed, and black hole masses should be smaller than
estimated from the observed luminosity. By the same token, there
are fewer bright large-redshift quasars than previously thought.
In addition to increasing luminosity, gravitational lensing
produces several images of one and the same quasar. Such multiple
images have indeed been observed for a number of close quasars.
Searches for the multiple images of distant quasars using the
Hubble telescope and large ground-based telescopes are being
planned which will provide a check on the validity of Wyithe and
Loeb's calculations. Source:
http://www.arXiv.org/abs/astro-ph/0203116
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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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