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Volumn 68, Issue 12, 2003, Pages

Radiation from accelerated black holes in an anti-de Sitter universe

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Indexed keywords


EID: 0842325930     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.68.124004     Document Type: Article
Times cited : (80)

References (64)
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    • (1986) Spinors and Space-time , vol.2
    • Penrose, R.1    Rindler, W.2
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    • edited by T. Gold (Cornell University Press, Ithaca, NY)
    • R. Penrose, in The Nature of Time, edited by T. Gold (Cornell University Press, Ithaca, NY, 1967), pp. 42-54.
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    • (1918) Ann. Phys. , vol.59 , pp. 185
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  • 55
    • 33845701627 scopus 로고    scopus 로고
    • note
    • The symmetric product ∨ of two 1-forms is defined as a∨b = ab + ba.
  • 57
    • 33845699133 scopus 로고    scopus 로고
    • note
    • There is no region I in this case. The numbering of regions, starting with II, has been chosen to be consistent with the case of two black holes (cf. Figs. 4-6) and with the C-metric with Λ > 0 [20].
  • 58
    • 85107712939 scopus 로고    scopus 로고
    • note
    • c which separates domains containing different pairs of black holes, cf. Fig. 2(a).
  • 59
    • 85107713840 scopus 로고    scopus 로고
    • note
    • ζ are regular at I in the sense of the tangent space of the conformal manifold with metric (2.14), cf. Ref. [14].
  • 60
    • 33845703066 scopus 로고    scopus 로고
    • note
    • For the particular case of geodesics with c = 0 see Appendix A.
  • 61
    • 85107713624 scopus 로고    scopus 로고
    • note
    • o formally corresponds to R = ∞. Here and in the following the symbol ∝ means a proportionality with a positive factor. Thanks to this convention we do not lose information about the orientation of related vectors.
  • 63
    • 85107712309 scopus 로고    scopus 로고
    • note
    • 2 are real, see Eq. (4.7).


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.