附录 发表于 2025-3-25 06:00:15

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Ondines-curse 发表于 2025-3-25 10:38:55

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自爱 发表于 2025-3-25 13:13:03

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缩短 发表于 2025-3-25 17:49:56

Conservation and Efficiency Issues, observations were important, pride of place must be given to the detection of neutrinos from the SN (the SN being denoted SN 1987A; its location was the Large Magellanic Cloud)..The neutrino detection was important from a number of standpoints, not least for the confirmation given to the general co

Cpr951 发表于 2025-3-25 20:23:22

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Mercurial 发表于 2025-3-26 03:04:18

Conservation and Efficiency Issues,ons involving the three flavour neutrinos is considered without simplifying assumptions. The T-violating asymmetry in three-neutrino oscillations in matter with constant density is discussed and it is shown that this asymmetry can be much larger than the corresponding asymmetry in vacuum oscillation

EVICT 发表于 2025-3-26 06:23:27

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中世纪 发表于 2025-3-26 11:50:59

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专心 发表于 2025-3-26 16:29:54

Student Elicitation for Estimation, pointing accuracy of better than 1.5° to look at point sources. From April 1986-87 muon detectors of total area 200 m. have also been in operation. We present upper limits on the flux of gamma rays from CYGNUS-X3 and demonstrate the usefulness of our muon detectors in improving the signal to noise

鲁莽 发表于 2025-3-26 18:18:23

Petter Gottschalk,Lars Gunnesdal of the absorption regions, the accretion disk corona, causes very strong attenuation of TeV γ-rays produced near to its centre, and suggests that a more likely method for their creation would be the dumping of a proton beam into some outlying matter, such as the rim of the accretion disk.
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查看完整版本: Titlebook: Cosmic Gamma Rays, Neutrinos, and Related Astrophysics; Maurice M. Shapiro,John P. Wefel Book 1989 Kluwer Academic Publishers 1989 Superno