| タイトル | Some astrophysical consequences of the existence of a heavy stable neutral lepton |
| 著者（英） | Lee, B. W.; Lerche, I.; Schramm, D. N.; Steigman, G.; Gunn, J. E. |
| 著者所属（英） | Yale Univ.|Chicago Univ. |
| 発行日 | 1978-08-01 |
| 言語 | eng |
| 内容記述 | It is suggested that a stable, massive, neutral lepton may dominate the present mass density in the universe. To investigate this assumption, attention is given to an analysis of extended gauge theories as they apply to a lepton with a mass of a few GeV/sq cm. A critical factor in the accuracy of the hypothesis is the actual mass of the lepton, and it is noted that the more massive the individual particle, the smaller the particle's aggregate contribution to the universal mass density. High energy accelerators could prove a useful tool in an empirical determination of the lepton's mass. It is further suggested that the lepton considered might provide the material in galactic halos, or supply the mass necessary to bind galactic clusters. A study of intergalactic annihilation radiation is expected to yield more data pertaining to the lepton's existence. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 78A45555 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/431717 |
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