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Titlebook: Neutrinos; Hans Volker Klapdor Textbook 1988 Springer-Verlag Berlin Heidelberg 1988 Lepton.Neutrino.Particle Physics.Supernova.astrophysic

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樓主: 人工合成
11#
發(fā)表于 2025-3-23 12:47:02 | 只看該作者
Neutrino Oscillations in Vacuum and Matter,Neutrino oscillations in vacuum have been discussed first by Pontecorvo [1]. Strong transformations of mixed neutrinos in matter [2–4] have three aspects:
12#
發(fā)表于 2025-3-23 17:24:46 | 只看該作者
978-3-642-46650-2Springer-Verlag Berlin Heidelberg 1988
13#
發(fā)表于 2025-3-23 19:12:25 | 只看該作者
14#
發(fā)表于 2025-3-24 02:16:41 | 只看該作者
Neutrino Properties,inued to be one of the most mysterious particles in physics. It took 26 years before it could be directly observed, via the inverse reaction of the β-decay,.by F. Reines and C.L. Cowan in 1956 [Rei59]. In addition to the experimental verification of the existence of the neutrino, the cross section f
15#
發(fā)表于 2025-3-24 05:23:54 | 只看該作者
Double Beta Decay Experiments and Searches for Dark Matter Candidates and Solar Axions,.Xe and .Nd are discussed. A brief review is given of published efforts to search for cosmic dark matter candidate particles and solar axions using the low background detector of a Ge double-beta-decay experiment.
16#
發(fā)表于 2025-3-24 07:38:51 | 只看該作者
Double Beta Decay, Neutrino Mass and Nuclear Structure, Hax 84, Doi 85, Kir 86, Ver 86, Gro 86, Ell 87, Mut 88a]. It can become observable only when a nucleus cannot undergo ordinary single β decay because of energy conservation, or of very strong suppression of energetically allowed transitions by a large spin difference between the parent and daughter
17#
發(fā)表于 2025-3-24 13:51:12 | 只看該作者
18#
發(fā)表于 2025-3-24 17:45:44 | 只看該作者
19#
發(fā)表于 2025-3-24 21:07:12 | 只看該作者
20#
發(fā)表于 2025-3-25 02:08:01 | 只看該作者
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