메뉴 건너뛰기




Volumn 55, Issue 10, 1997, Pages 6014-6018

Instability of an “approximate black hole

Author keywords

[No Author keywords available]

Indexed keywords


EID: 0000116637     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.55.6014     Document Type: Article
Times cited : (14)

References (13)
  • 4
    • 85038268250 scopus 로고    scopus 로고
    • general, we have tried to follow van Putten’s notation fairly closely. However, we found the field (Formula presented) to be a useful quantity in the perturbation and use it instead of van Putten’s (Formula presented). Note too that at one point in his derivation van Putten uses (Formula presented), but for a quantity different from what we have defined above
    • In general, we have tried to follow van Putten’s notation fairly closely. However, we found the field (Formula presented) to be a useful quantity in the perturbation and use it instead of van Putten’s (Formula presented). Note too that at one point in his derivation van Putten uses (Formula presented), but for a quantity different from what we have defined above.
  • 6
    • 85038320994 scopus 로고    scopus 로고
    • What it means for a solution with a naked singularity at the origin to disperse is perhaps not well defined at the moment. However, the evolution clearly indicates that the energy content is moving toward large radius
    • What it means for a solution with a naked singularity at the origin to disperse is perhaps not well defined at the moment. However, the evolution clearly indicates that the energy content is moving toward large radius.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.