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Volumn 68, Issue 2, 2003, Pages

Computing gravitational waves from slightly nonspherical stellar collapse to a black hole: Odd-parity perturbation

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; COSMOLOGICAL PHENOMENA; GRAVITY; MATHEMATICAL ANALYSIS; MOLECULAR DYNAMICS; THEORY; WAVEFORM;

EID: 3843088326     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.68.024002     Document Type: Article
Times cited : (20)

References (71)
  • 7
    • 33750354739 scopus 로고    scopus 로고
    • B.F. Schutz, gr-qc/0111095
    • B.F. Schutz, gr-qc/0111095.
  • 10
    • 0004229909 scopus 로고
    • edited by J.M. Centrella (Cambridge University Press, Cambridge, England)
    • in Dynamical Spacetimes and Numerical Relativity, edited by J.M. Centrella (Cambridge University Press, Cambridge, England, 1986), p. 40.
    • (1986) Dynamical Spacetimes and Numerical Relativity , pp. 40
  • 14
    • 0002926667 scopus 로고    scopus 로고
    • edited by R.M. Wald (Chicago University Press, Chicago)
    • M.J. Rees, in Black Holes and Relativistic Stars, edited by R.M. Wald (Chicago University Press, Chicago, 1998), p. 79.
    • (1998) Black Holes and Relativistic Stars , pp. 79
    • Rees, M.J.1
  • 15
    • 0042349593 scopus 로고    scopus 로고
    • edited by L. Kaper, E.P.J. van den Geurel, and P.A. Woudt (Springer-Verlag, New York)
    • M.J. Rees, in Black Holes in Binaries and Galactic Nuclei, edited by L. Kaper, E.P.J. van den Geurel, and P.A. Woudt (Springer-Verlag, New York, 2001), p. 351.
    • (2001) Black Holes in Binaries and Galactic Nuclei , pp. 351
    • Rees, M.J.1
  • 24
    • 0036005462 scopus 로고    scopus 로고
    • Prog. Theor. Phys. 107, 265 (2002);
    • (2002) Prog. Theor. Phys. , vol.107 , pp. 265
  • 25
  • 59
  • 63
    • 18144414653 scopus 로고    scopus 로고
    • See, the following references for concrete application of the formula in [46]: M. Shibata, Phys. Rev. D 60, 104052 (1999).
    • (1999) Phys. Rev. D , vol.60 , pp. 104052
    • Shibata, M.1
  • 70
    • 33750333380 scopus 로고    scopus 로고
    • note
    • i are the initial central density and average density of the dust cloud at t=0, respectively. It is obvious that the former can be earlier than the latter for the initial data with certain central concentration.
  • 71
    • 33750336907 scopus 로고    scopus 로고
    • note
    • The similar results were obtained for linearized gravitational waves during the spherically symmetric homogeneous dust collapse [22] and for scalar waves during the neutron star collapse in the fully nonlinear spherically symmetric Einstein-fluid-Klein-Gordon system [43].


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.