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Volumn 71, Issue 2, 2005, Pages

Massive scalar field instability in Kerr spacetime

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; CALCULATION; DYNAMICS; MATHEMATICAL ANALYSIS; SPACE; TIME;

EID: 84927760257     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.71.024034     Document Type: Article
Times cited : (79)

References (15)
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  • 3
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    • V. Cardoso, O. J. C. Dias, J. P. S. Lemos, and S. Yoshida, Phys. Rev. D 70, 044039 (2004); V. Cardoso and O. J. C. Dias, Phys. Rev. D 70, 084011 (2004); H. Furuhashi and Y. Nambu, gr-qc/0402037 [Prog. Theor. Phys. (to be published)]. H. R. Beyer, Commun. Math. Phys. 221, 659 (2001); R. A. Konoplya and A. V. Zhidenko, gr-qc/0411059.
    • (2004) Phys. Rev. D , vol.70 , pp. 084011
    • Cardoso, V.1    Dias, O.J.C.2
  • 4
    • 42749102782 scopus 로고    scopus 로고
    • gr-qc/0402037 (to be published)
    • V. Cardoso, O. J. C. Dias, J. P. S. Lemos, and S. Yoshida, Phys. Rev. D 70, 044039 (2004); V. Cardoso and O. J. C. Dias, Phys. Rev. D 70, 084011 (2004); H. Furuhashi and Y. Nambu, gr-qc/0402037 [Prog. Theor. Phys. (to be published)]. H. R. Beyer, Commun. Math. Phys. 221, 659 (2001); R. A. Konoplya and A. V. Zhidenko, gr-qc/0411059.
    • Prog. Theor. Phys.
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    • V. Cardoso, O. J. C. Dias, J. P. S. Lemos, and S. Yoshida, Phys. Rev. D 70, 044039 (2004); V. Cardoso and O. J. C. Dias, Phys. Rev. D 70, 084011 (2004); H. Furuhashi and Y. Nambu, gr-qc/0402037 [Prog. Theor. Phys. (to be published)]. H. R. Beyer, Commun. Math. Phys. 221, 659 (2001); R. A. Konoplya and A. V. Zhidenko, gr-qc/0411059.
    • (2001) Commun. Math. Phys. , vol.221 , pp. 659
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    • R. A. Konoplya and A. V. Zhidenko, gr-qc/0411059
    • V. Cardoso, O. J. C. Dias, J. P. S. Lemos, and S. Yoshida, Phys. Rev. D 70, 044039 (2004); V. Cardoso and O. J. C. Dias, Phys. Rev. D 70, 084011 (2004); H. Furuhashi and Y. Nambu, gr-qc/0402037 [Prog. Theor. Phys. (to be published)]. H. R. Beyer, Commun. Math. Phys. 221, 659 (2001); R. A. Konoplya and A. V. Zhidenko, gr-qc/0411059.
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    • note
    • Note that a time-domain study of late-time tails of massive scalar fields in black hole spacetimes has been performed before using a Teukolsky code very similar to this one (just in different coordinates) [5]. That work demonstrated that the late-time tail of massive scalars with axisymmetry, in both Schwarzchild and Kerr spacetimes is the same, i.e., t-5/6.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.