| タイトル | Neutrinos from binary pulsars |
| 著者（英） | Eichler, D. |
| 著者所属（英） | Chicago Univ. |
| 発行日 | 1978-10-26 |
| 言語 | eng |
| 内容記述 | It is shown that binary systems containing moderately young pulsars may emit high-energy neutrinos (between 1 and 100 TeV) at detectable levels. The pulsars are assumed to have total luminosities of the order of 10 to the 38th erg/sec. The neutrinos are produced by high energy particles (e.g. protons) from the pulsar striking the companion. Cyg X3 may be detectable in high-energy neutrinos if it emits greater than about 10 to the 35th erg/sec in high-energy protons. There may be a whole class of objects like Cyg X3, but obscured by thick accretion clouds. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 79A13069 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/429579 |
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