淡江大學機構典藏:Item 987654321/27892
English  |  正體中文  |  简体中文  |  Items with full text/Total items : 62830/95882 (66%)
Visitors : 4030793      Online Users : 992
RC Version 7.0 © Powered By DSPACE, MIT. Enhanced by NTU Library & TKU Library IR team.
Scope Tips:
  • please add "double quotation mark" for query phrases to get precise results
  • please goto advance search for comprehansive author search
    •  Adv. Search
    Home ‧ Login ‧ Upload ‧ Help ‧ About ‧ Administer Goto mobile version


    Please use this identifier to cite or link to this item: https://tkuir.lib.tku.edu.tw/dspace/handle/987654321/27892


    Title: A hydrodynamical analysis of the burning of a neutron star
    Other Titles: 中子星燃燒的流體力學分析
    Authors: Cho, Hing-tong;Ng, K. W.;Speliotopoulos, A. D.
    Contributors: 淡江大學物理學系
    Date: 1994-04-28
    Issue Date: 2009-12-31 10:50:55 (UTC+8)
    Publisher: Amsterdam : North-Holland Publishing
    Abstract: 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.
    Relation: Physics Letters B 326(1-2), pp.111-117
    DOI: 10.1016/0370-2693(94)91201-7
    Appears in Collections:[Graduate Institute & Department of Physics] Journal Article

    Files in This Item:

    File Description SizeFormat
    index.html0KbHTML490View/Open
    index.html0KbHTML243View/Open

    All items in 機構典藏 are protected by copyright, with all rights reserved.

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