|
Nobelium-254
1 November 1998
Atoms with atomic numbers above 92 (trans-uranian elements) are all but
absent in nature. Researchers at Argonne National Laboratory produce heavy
atoms by directing calcium nuclei at a lead target in the ATLAS
accelerator. In this process a small fraction of nobelium-254 is obtained,
whose nucleus consists of 102 protons and 152 neutrons and has a relatively
long lifetime of 55 sec. The nuclei are created within a so-called `Gamma
sphere,' a spherically shaped device lined by gamma detectors which sample
gamma photons from newly created, highly excited and spinning nuclei.
Having passed a mass analyzer, nuclei go to a silicon detector, to be
identified by the way they decay into lighter fragments. The nobelium-254
is the heaviest nucleus whose gamma spectrum has been studied in detail so
far. A 20% non-sphericity of the nuclei is reported, and the possibility
for this heavy nuclei to sustain an angular moment of ≈14h by is shown.
Source:
Physics News Update, Number 397
Electron diffraction on a fullerene
1 November 1998
A. Solov'ev and his colleagues in St. Petersburg developed a new techniques
for the study of large molecules and atomic clusters by means of electron
diffraction. Using a 809 eV electron beam, a gas of spherical C60 fullerenes
was investigated. The effective electron wavelength was chosen to be
smaller than the size of the fullerene molecule but larger than the
intercarbon atom spacing. The angular and energy distributions of scattered
electrons were studied. The technique proved very useful for the study of
the molecule's surface electrons. In particular, a number of plasmon modes
were detected, of which only one had been previously reported. In the
authors' opinion, in such experiments also the surface charge distribution
and polarizability of the C60 molecule as well as the properties of more
complex molecules, e. g., proteins, can be examined.
Source:
http://publish.aps.org/FOCUS/
Photon molecule
1 November 1998
In 1997, A Forchel, T. Reinecke and their colleagues created a
‘photonic atom’, a quantum system consisting of a single photon in a micron-size
semiconductor cavity. By connecting two such ‘atom’ by a microscopic
bridge, a `photonic molecule' was obtained in more recent experiments. As
is the case with the hydrogen molecule, also the energy levels of the
photonic molecule are observed to shift and split. The `photonic molecule'
is the first step towards the creation of more complex structures of a
larger number of `photonic atoms,' to which desired properties may be
given.
Source: http://ojps.aip.org/prlo/top.html
Gamma radiation blast
1 November 1998
On August 27, 1998, for the first time, significant changes in the Earth's
ionosphere were detected, caused by an energy flow from outside of the
solar system. A 5-min high-power blast of gamma radiation caused an effect
comparable to oscillations normally observed during a day in ionospheric
activities. The phenomenon caused a partial violation of radio
communication. A similar situation is observed during solar blasts. A blast
of gamma and X-ray radiation was also detected by a number of space
vehicles. The radiation source is believed to be a neutron star which was
detected earlier due to its pulsed X-ray radiation. Such neutron stars are
called magnetars due to their high magnetic field of 1015Gauss, 100 times
that in ordinary neutron stars. The blast presumably occurred during the
fault of the neutron star's core which caused charged particles to
accelerate in a magnetic field. Source: http://unisci.com/
Distant galaxies
1 November 1998
Extremely weak galaxies about 12×109 light years away have been detected using
an infrared chamber and a multi-object spectrometer mounted on the Hubble
telescope. The large red shift due to the expansion of the Universe make
these galaxies invisible in the optical range. Some galaxies have blue
colored knots in their structure, which were earlier considered as separate
galaxies but turned out to be in fact regions of active star formation.
Possibly, the detected galaxies are still at very early stages of their
formation. A new generation telescope, to be launched in 2007, seems to
hold particular promise for progress in the study of such objects. Source:
http://www.stsci.edu/
|
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.
|