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Superheavy hydrogen
1 October 2001
For over forty years physicists have searched for nuclei of
superheavy hydrogen 5H, consisting of four neutrons and one proton.
Now, for the first time, these nuclei have been reliably detected
in an experiment conducted by Russian scientists from the Joint
Institute for Nuclear Research in Dubna and Kurchatov Institute
in collaboration with their colleagues from France and Japan.
Produced in the reaction 1H(6He,2He)5H,
the nuclei of the isotope 5H were
identified by the kinetics of the decay of 2He into two protons.
The energy spectrum of the protons shows a resonance which,
according to calculations, corresponds with the nucleus of
superheavy hydrogen as the second reaction product. The discovery
became possible thanks to a combination of a cryogenic target,
special kinds of detectors, and a unique source of 6He nuclei
developed at Dubna.
Source:
Phys. Rev. Lett. 87 092501 (2001)
Cancellation of magnetic moments
1 October 2001
H Adachi and his colleagues in Japan have discovered that the
compound Sm0,976Gd0,024Al2
may have zero macroscopic magnetization even with the
spins (and intrinsic magnetic moments) of its electrons all
aligned in a single direction as in a common ferromagnet. Spin
magnetization and that due to the orbital motion of atomic
electrons are different in their temperature dependence. At a
temperature of 67.5 K the perfect cancellation of the two
magnetizations occurs, although both above and below this
temperature the substance does have a magnetic moment. The
alignment of electron spins was discovered by studying the
Compton scattering of polarized X rays from a sample. The effect
was predicted theoretically by the Australian physicist A Stewart
in 1972. It may prove useful in experiments which require spin
polarization but in which the effect of a macroscopic magnetic
field is undesirable.
Source:
Phys. Rev. Lett. 87 127202 (2001)
An anomalous acoustoelectric effect
1 October 2001
The normal acoustoelectric effect is the appearance in a material
of an electric current parallel to the sound wave propagation
direction. The study of this effect may be useful in
understanding interactions between electrons and the vibrations
of the crystal lattice. A collaboration of scientists from Russia
(Ioffe Physical Technical Institute, St. Petersburg), Ukraine,
and Poland studied the propagation of acoustic surface waves in a
thin film of La0,67Ca0,33MnO3 laid onto a substrate of piezodielectric material
LiNbO3. It is found that, along with the ordinary current, an
additional current is generated in a material, which does not
depend on the direction of the sound wave and which in a certain
temperature range exceeds the current due to the normal
acoustoelectric effect. A detailed study showed that the
additional current is due to the properties of the
piezodielectric substrate and is produced by the electric fields
resulting from the compressions and rarefactions in the field of
the acoustic wave.
Source:
Physics News Update, Number 557
Superconductivity in the fullerene
1 October 2001
In a pure crystal of fullerene C60 the distance between the
molecules is 1.415 nm, and the temperature at which such a
crystal becomes superconducting is Tc= 18 K. It is known that
inducing hole superconductivity (hole injection) and doping the
crystal with certain substances may lead to a higher transition
temperature. A record high transition temperature of Tc=117 K was
achieved by B Battlog and his colleagues from Lucent Technologies
by doping a C60 crystal with molecules of tribromo-methane Br3CH.
Placed in the space between fullerene molecules, the Br3CH molecules
increase the lattice parameter to 1.445 nm, causing Tc to rise to
a temperature characteristic of high-temperature superconductors.
Source:
www.science.com
An X-ray burst
1 October 2001
For the first time, a short powerful burst of X-ray radiation
from the object Sgr A* at the centre of our galaxy has been
detected by the space-based Chandra Observatory. Within a few
minutes the source's brightness increased 45 times, then
decreased by a factor of 5 within the next ten minutes, and then
returned to its normal level over a period of several hours.
According to the infrared telescope data on the kinematics of
stars at the centre of the Galaxy, the location of the source Sgr A*
coincides with the supposed location of the central black hole
with a mass of about 2,6.106 solar mass. Previously, only weak constant-brightness
radiation at radio and X-ray wavelengths has been observed to
come from this object. The burst can be explained either by the
infall of a comet head into the black hole, or alternatively by
the reconnection of magnetic field lines in the black hole's
magnetosphere. Either scenario leads to the formation of shock
waves and also involves the acceleration of electrons to
subrelativistic speeds - and thereby X-ray radiation. Powerful
variable-brightness radiation is characteristic of quasars, where
it is due to the intense unsteady accretion on supermassive black
holes. Modern galaxies also may have passed through a quasar
stage in the dim past, but today their central black holes are
calm - except for rare events one of which was presumably
detected by Chandra.
Source:
http://unisci.com
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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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