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Marina Murzina 《Space Science Reviews》1995,74(3-4):493-497
Transport of energy and lepton charge by neutrino radiation in a uniform medium is investigated within neutrino-thermoconductivity approximation — as a neutrino heat wave. The process is described by a self-similar solution. The problem applies primarily to the cooling of young neutron stars. 相似文献
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We analyze here how solar neutrino experiments could detect time fluctuations of the solar neutrino flux due to magnetohydrodynamics
(MHD) perturbations of the solar plasma. We state that if such time fluctuations are detected, this would provide a unique
signature of the Resonant Spin-Flavor Precession (RSFP) mechanism as a solution to the Solar Neutrino Problem.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
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Astrophysical limitations do not exclude the possibility of some number of dark matter primordial Black Holes (BH) being seeded in the interiors of the Earth at the epoch of planet condensation in the young Solar System. We show that limitations on the neutrino radiation due to the BH quantum evaporation and accretion growth of BH mass completely forbid the existence of primordial BH of any mass in the Earth. 相似文献
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Y. Suzuki 《Space Science Reviews》1998,85(1-2):91-104
The current status of solar neutrino experiments is reviewed. All the experimental measurements show deficits of solar neutrinos.
Non monotonic suppression indicates that the problem may naturally be explained by neutrino oscillations, but not by modifying
solar models. A new experiment shows very promising results. We hope that a definite answer to the question of whether solar
neutrinos are oscillating will be obtained in the very near future.
This revised version was published online in June 2006 with corrections to the Cover Date. 相似文献
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