論文

査読有り
2015年

No rotating star solutions of a perfect fluid in projectable Horava-Lifshitz gravity

The 13th Marcel Grossmann Meeting: On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories - Proceedings of the MG13 Meeting on General Relativity, 2012
  • Naoki Tsukamoto
  • ,
  • Tomohiro Harada

210699
開始ページ
1131
終了ページ
1133
記述言語
英語
掲載種別
研究論文(国際会議プロシーディングス)
DOI
10.1142/9789814623995_0099
出版者・発行元
World Scientific

Horava-Lifshitz gravity has covariance only under the foliation-preserving diffeomorphism. This implies that the quantities on the constant-time hypersurfaces should be regular. In the original theory, the projectability condition which strongly restricts the lapse function is proposed. We assume that a star is filled with a perfect fluid, that it has the reflection symmetry about the equatorial plane. As a result, we find a no-go theorem for stationary axisymmetric star solutions in projectable Horava-Lifshitz gravity under the physically reasonable assumptions on the matter sector.

リンク情報
DOI
https://doi.org/10.1142/9789814623995_0099
ID情報
  • DOI : 10.1142/9789814623995_0099
  • SCOPUS ID : 85045346728

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