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Volumn 56, Issue 4, 1997, Pages 2226-2235

Cosmological and black hole horizon fluctuations

Author keywords

[No Author keywords available]

Indexed keywords


EID: 0000127129     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.56.2226     Document Type: Article
Times cited : (75)

References (23)
  • 2
    • 85038287335 scopus 로고    scopus 로고
    • How Wrinkled is the Surface of a Black Hole?,” Report No. gr-qc/9701056 (unpublished)
    • R. D. Sorkin, “Two Topics concerning Black Holes: Extremality of the Energy, Fractality of the Horizon,” Report No. (unpublished);“How Wrinkled is the Surface of a Black Hole?,” Report No. gr-qc/9701056 (unpublished).
    • Sorkin, R.D.1
  • 6
    • 85038278043 scopus 로고    scopus 로고
    • Units in which (Formula presented) will be used in this paper. Thus the units of mass, length, and time differ by factors of (Formula presented) from the usual definitions of the Planck mass, Planck length, and Planck time. As most of the discussion in this paper deals with order of magnitude estimates, this should not cause any confusion. The metric signature will be (Formula presented)
    • Units in which (Formula presented) will be used in this paper. Thus the units of mass, length, and time differ by factors of (Formula presented) from the usual definitions of the Planck mass, Planck length, and Planck time. As most of the discussion in this paper deals with order of magnitude estimates, this should not cause any confusion. The metric signature will be (Formula presented).
  • 19
    • 85038309914 scopus 로고    scopus 로고
    • 53, 7028(1996).
    • (1996) , vol.53 , pp. 7028


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.