淡江大學機構典藏:Item 987654321/27892
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    题名: A hydrodynamical analysis of the burning of a neutron star
    其它题名: 中子星燃燒的流體力學分析
    作者: Cho, Hing-tong;Ng, K. W.;Speliotopoulos, A. D.
    贡献者: 淡江大學物理學系
    日期: 1994-04-28
    上传时间: 2009-12-31 10:50:55 (UTC+8)
    出版者: Amsterdam : North-Holland Publishing
    摘要: The burning of a neutron star by strange matter is analyzed using relativistic combustion theory with a planar geometry. It is shown that such burning is probably neither slow combustion nor simple detonation. Fast combustion without detonation is possible under certain circumstances, but would involve very efficient heat transfer mechanisms. It is found, however, that the burning is most likely absolutely unstable with no well defined burn front.
    關聯: Physics Letters B 326(1-2), pp.111-117
    DOI: 10.1016/0370-2693(94)91201-7
    显示于类别:[物理學系暨研究所] 期刊論文

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