网络太阳中微子问题 网络释义 1. 太阳中微子问题 太阳中微子问题(The Solar Neutrino Problem) 中微子是一种不带电、质量极小的亚原子粒子, 它几乎不与任何物质发生相互作 … wenku.baidu.com|基于7个网页
The "solar neutrino problem" is summarized. It is emphasized that there are really two solar neutrino problems — the most compelling being the difficulty in making a quantitatively consistent picture of the relative rates of the different reactions from current experimental data. In addition, ...
In the light of the solar neutrino problem we started the development of a new mathematical approach to the analytic representation of nuclear reaction rates, cp. HAUBOLD and JOHN [2]. The intention to come up with closed form representations of nuclear reaction rates is to take into account ...
What is the solar neutrino problem?Solar Neutrino Problem:Humans have made efforts to understand the nature and the astronomical objects around them. One such astronomical object of interest is the Sun. Scientists have made efforts to understand the Sun through theoretical models and experiments ...
Helioseismic Constraints on Solar Structure and the Solar Neutrino Problemdoi:10.1007/978-94-011-4497-1_15One of the major outstanding problems of solar (or particle) physics is that the measured flux of neutinos on earth (cf Kirsten 1996, 1997) is substantially less than that predicted by a...
The values of neutrino masses and mixing angles which are required by the Mikheyev-Smirnov-Wolfenstein (MSW) solution to the solar-neutrino problem are found from analytic solutions to the neutrino propagation equations in the Sun. They coincide with those obtained through extensive numerical computat...
LMA MSW solution of the solar neutrino problem and first KamLAND results The first KamLAND results are in a very good agreement with the predictions made on the basis of the solar neutrino data and the LMA realization of the MSW... PCD Holanda,AY Smirnov - 《Journal of Cosmology & Astropa...
the solar neutrino problem(s) evident. At present, such information is the main evidence for solar neutrino physics beyond the standard electroweak model; however, since the theoretical 3 The inclusion of the Kamiokande rate is currently not decisive in shaping the MSW solutions, ...
The Sudbury Neutrino Observatory has solved a 30-year-old mystery by showing that neutrinos from the sun change species en route to the earth
the neutrino oscillation formulas that we use in the analysis of solar neutrino data which take into account matter effects in the case of the MSW solution of the solar neutrino problem. We also present some improvement concerning the calculation of the regeneration of solar ν e ’s in the...