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Volumn 58, Issue 8, 1998, Pages

Spherical black holes cannot support scalar hair

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EID: 0542442140     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.58.087502     Document Type: Article
Times cited : (62)

References (25)
  • 1
    • 0012234537 scopus 로고
    • J. D. Bekenstein, Ann. Phys. (N.Y.) 82, 535 (1974). Actually Bekenstein’s original solution included also an electromagnetic field. However, for simplicity in the present paper, its contribution will be ignored. Its inclusion does not change the issue at hand.
    • (1974) Ann. Phys. (N.Y.) , vol.82 , pp. 535
    • Bekenstein, J.D.1
  • 8
    • 85038991946 scopus 로고    scopus 로고
    • P. Bizon, Jagellonian University, Institute of Physics, Cracow, Poland, report, 1994
    • P. Bizon, Jagellonian University, Institute of Physics, Cracow, Poland, report, 1994.
  • 14
    • 85038997507 scopus 로고    scopus 로고
    • See, for example, Sec. 4.6 of R. M. Wald, Quantum Field Theory in Curved Space time and Black Hole Thermodynamics (The University of Chicago Press, Chicago, 1994)
    • See, for example, Sec. 4.6 of R. M. Wald, Quantum Field Theory in Curved Space time and Black Hole Thermodynamics (The University of Chicago Press, Chicago, 1994).
  • 16
    • 0004179874 scopus 로고
    • Wiley, New York, or for a more complicated, case see J. Louko and R. Sorkin, Class. Quantum Grav. (to be published)
    • The regularization scheme employed is rather a standard one. See, for example, J. D. Jackson, Classical Electrodynamics (Wiley, New York, 1975) for an elementary example, or for a more complicated, case see J. Louko and R. Sorkin, Class. Quantum Grav. (to be published).
    • (1975) Classical Electrodynamics
    • Jackson, J.D.1
  • 25


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.