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101.
The interaction of microwave radiation with the plasma in photoionized semiconductor photocells (CdS, CdSe) placed in waveguide
measurement systems is investigated theoretically and experimentally. The interaction of the characteristic waveguide modes
with a photoexcited semiconductor plasma is investigated. The dependence of the reflection coefficient and phase of the microwave
radiation on the intensity of the optical radiation to be measured is obtained, and the influence of the surface of the semiconductor
photocells on these parameters is investigated. A microwave photodetector design based on a millimeter-wave interferometer
is developed.
Zh. Tekh. Fiz. 68, 94–98 (November 1998) 相似文献
102.
103.
V. A. Tsarev 《Bulletin of the Lebedev Physics Institute》2008,35(8):244-246
The chiral effect of the switch-on shock wave from the supernova (SN) on interstellar cloud organics was estimated. It was found that this effect is weak and cannot violate the chiral universality of the influence caused by left-polarized electrons and neutrino from the SN. 相似文献
104.
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 γ 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. 相似文献
105.
V. I. Galkin Yu. A. Garnushkin V. A. Matveev A. G. Olshevsky N. G. Polukhina T. M. Roganova O. G. Ryazhskaya V. A. Tsarev 《Bulletin of the Russian Academy of Sciences: Physics》2007,71(4):579-581
The main purpose of the OPERA experiment is the direct observation of neutrino oscillations (vμ → vτ) in the vμ beam from the CERN accelerator through the direct detection of τ leptons in nuclear emulsions at the Gran Sasso National Underground Laboratory. Some aspects of the use of the Russian PAVICOM facility for processing and analyzing the data obtained from the OPERA experiment are discussed. 相似文献
106.
G. A. Gusev N. G. Polukhina V. A. Tsarev A. V. Uryson 《Bulletin of the Lebedev Physics Institute》2007,34(7):204-207
The previously proposed idea about the possible role of neutrons released during the supernova (SN) outburst as a source of polarized electrons causing chiral asymmetry of organic molecules in interstellar gas—dust clouds is developed. A specific physical mechanism of removal of a large number of free neutrons beyond the dense SN shell via the relativistic neutron fireball with a Lorentz factor on the order of 100 is considered. Estimations show high efficiency of the chiral effect of electrons from the SN in the mechanism under consideration. 相似文献
107.
We prove that every law of the lattice of all formations of finite groups is fulfilled in the lattice of all n-multiply ω-composition formations of finite groups for every nonempty set of primes ω and every natural n. 相似文献
108.