English  |  正體中文  |  简体中文  |  全文笔数/总笔数 : 49074/83178 (59%)
造访人次 : 6967391      在线人数 : 61
RC Version 7.0 © Powered By DSPACE, MIT. Enhanced by NTU Library & TKU Library IR team.
搜寻范围 查询小技巧:
  • 您可在西文检索词汇前后加上"双引号",以获取较精准的检索结果
  • 若欲以作者姓名搜寻,建议至进阶搜寻限定作者字段,可获得较完整数据
  • 进阶搜寻


    jsp.display-item.identifier=請使用永久網址來引用或連結此文件: http://tkuir.lib.tku.edu.tw:8080/dspace/handle/987654321/27892


    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

    文件中的档案:

    档案 描述 大小格式浏览次数
    index.html0KbHTML190检视/开启
    index.html0KbHTML40检视/开启

    在機構典藏中所有的数据项都受到原著作权保护.

    TAIR相关文章

    DSpace Software Copyright © 2002-2004  MIT &  Hewlett-Packard  /   Enhanced by   NTU Library & TKU Library IR teams. Copyright ©   - 回馈