完整後設資料紀錄
DC 欄位 | 值 | 語言 |
---|---|---|
dc.contributor.author | Athar, H | en_US |
dc.contributor.author | Lin, GL | en_US |
dc.contributor.author | Tseng, JL | en_US |
dc.date.accessioned | 2019-04-03T06:39:28Z | - |
dc.date.available | 2019-04-03T06:39:28Z | - |
dc.date.issued | 2001-10-01 | en_US |
dc.identifier.issn | 0556-2821 | en_US |
dc.identifier.uri | http://dx.doi.org/10.1103/PhysRevD.64.071302 | en_US |
dc.identifier.uri | http://hdl.handle.net/11536/29369 | - |
dc.description.abstract | The cross section for muon pair productions by electrons scattering over photons, sigma (MPP), is calculated analytically in the leading order. It is pointed out that for the center-of-mass energy range s greater than or equal to 5m(mu)(2), the cross section sigma (MPP) is less than 1 mub. The differential energy spectrum for either of the resulting muons is given for the purpose of high-energy neutrino astronomy. An implication of our result for a recent suggestion concerning the high-energy cosmic neutrino generation through this muon pair is discussed. | en_US |
dc.language.iso | en_US | en_US |
dc.title | Muon pair production by electron-photon scatterings | en_US |
dc.type | Article | en_US |
dc.identifier.doi | 10.1103/PhysRevD.64.071302 | en_US |
dc.identifier.journal | PHYSICAL REVIEW D | en_US |
dc.citation.volume | 64 | en_US |
dc.citation.issue | 7 | en_US |
dc.citation.spage | 0 | en_US |
dc.citation.epage | 0 | en_US |
dc.contributor.department | 物理研究所 | zh_TW |
dc.contributor.department | Institute of Physics | en_US |
dc.identifier.wosnumber | WOS:000171280300003 | en_US |
dc.citation.woscount | 3 | en_US |
顯示於類別: | 期刊論文 |