| タイトル | Nucleosynthesis, neutrino bursts and gamma-rays from coalescing neutron stars |
| 著者（英） | Schramm, David N.; Livio, Mario; Eichler, David; Piran, Tsvi |
| 著者所属（英） | Princeton Univ. Observatory|NASA Lewis Research Center|Fermi National Accelerator Lab.|Ben Gurion Univ. of the Negev|Chicago Univ.|Hebrew Univ.|Maryland Univ.|Technion - Israel Inst. of Tech. |
| 発行日 | 1989-07-13 |
| 言語 | eng |
| 内容記述 | It is pointed out here that neutron-star collisions should synthesize neutron-rich heavy elements, thought to be formed by rapid neutron capture (the r-process). Furthermore, these collisions should produce neutrino bursts and resultant bursts of gamma rays; the latter should comprise a subclass of observable gamma-ray bursts. It is argued that observed r-process abundances and gamma-ray burst rates predict rates for these collisions that are both significant and consistent with other estimates. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 89A46577 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/362379 |
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