Gravitational Radiation Reaction

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Author(s)

Abstract

We give a short personally-biased review on the recent progress in our understanding of gravitational radiation reaction acting on a point particle orbiting a black hole. The main motivation of this study is to obtain sufficiently precise gravitational waveforms from inspiraling binary compact stars with a large mass ratio. For this purpose, various new concepts and techniques have been developed to compute the orbital evolution taking into account the gravitational self-force. Combining these ideas with a few supplementary new ideas, we try to outline a path to our goal here.

Journal

  • Progress of Theoretical Physics

    Progress of Theoretical Physics (163), 120-145, 2006-07-31

    Progress of Theoretical Physics

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Codes

  • NII Article ID (NAID)
    110004799241
  • NII NACSIS-CAT ID (NCID)
    AA00791466
  • Text Lang
    ENG
  • Article Type
    Journal Article
  • ISSN
    03759687
  • NDL Article ID
    7994349
  • NDL Source Classification
    ZM35(科学技術--物理学)
  • NDL Call No.
    Z53-A468
  • Data Source
    CJP  CJPref  NDL  NII-ELS  NDL-Digital 
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