附录 发表于 2025-3-25 06:00:15
http://reply.papertrans.cn/24/2389/238878/238878_21.pngOndines-curse 发表于 2025-3-25 10:38:55
http://reply.papertrans.cn/24/2389/238878/238878_22.png自爱 发表于 2025-3-25 13:13:03
http://reply.papertrans.cn/24/2389/238878/238878_23.png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 coCpr951 发表于 2025-3-25 20:23:22
http://reply.papertrans.cn/24/2389/238878/238878_25.pngMercurial 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 oscillationEVICT 发表于 2025-3-26 06:23:27
http://reply.papertrans.cn/24/2389/238878/238878_27.png中世纪 发表于 2025-3-26 11:50:59
http://reply.papertrans.cn/24/2389/238878/238878_28.png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.