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10 number 2007 year |
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1.
Title:
MODELING OF THE LORD (LUNAR ORBITAL RADIO DETECTOR) EXPERIMENT WITH REGARD TO THE ANTENNA DIRECTIVITY DIAGRAM,
RADIATION POLARIZATION, AND GALACTIC NOISE
Authors:
G.A. Gusev, I.A. Krol, V.A. Tsarev.
Abstract:
2.
Title:
RESULTS OF THE MONTE CARLO SIMULATION OF THE LORD EXPERIMENT WITH ALLOWANCE MADE FOR THE ANTENNA SYSTEM PARAMETERS
AND GALACTIC NOISE EFFECT
Authors:
G.A. Gusev, I.A. Krol, V.A. Tsarev.
Abstract:
3.
Title:
RELATIVISTIC NEUTRON FIREBALL FROM A SUPERNOVA EXPLOSION
AS A POSSIBLE SOURCE OF CHIRAL EFFECT.
THE ROLE OF BREMSSTRAHLUNG PHOTONS
Authors:
G.A. Gusev, V.A. Tsarev.
Abstract:
We develop the idea, proposed earlier, of a possible role of neutrons, released in a supernova (SN) explosion, as a source of polarized electrons that cause chiral asymmetry of organic molecules in interstellar gas-dust clouds. The neutrons are carried away from the dense SN shell by a relativistic neutron fireball with Lorentz factor ?? of order 100. At the early stage of this carrying away, the ejected polarized electrons generate circularly polarized photons as a result of bremsstrahlung in the fireball plasma. The photons of energy near 5 eV in the ultraviolet part of the spectrum show a high efficiency of the chiral effect. In the favorable case of low absorption in the interstellar medium this mechanism may appear to be more (by two orders of magnitude) efficient than the chiral effect of the polarized electrons from the same fireball.
4.
Title:
DETERMINATION OF THE CYCLOTRON GENERATION SUPPRESSION BAND WIDTH IN A PLASMA RELATIVISTIC MICROWAVE GENERATOR
Authors:
I.L. Bogdankevich, P.S. Strelkov, V.P. Tarakanov.
Abstract:
5.
Title:
TWO-CHANNEL SCHEME FOR DARK MATTER PARTICLE DETECTION BASED ON A LOW-TEMPERATURE MAGNETIC CALORIMETER
Authors:
A.I. Golovashkin, G.A. Gusev, L.N. Zherikhina, B.N. Lomonosov, V.A. Tsarev, A.M. Tskhovrebov.
Abstract:
6.
Title:
CARBON TETRACHLORIDE AS A LIQUID MATRIX FOR ORTHO-PARA DIAGNOSTICS OF WATER. CAPABILITIES OF IR AND NMR SPECTROSCOPY
Authors:
V.S. Parbuzin, M.V. Polyakova, V.P. Bystrov.
Abstract:
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