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Volumn 67, Issue 2, 2003, Pages

Classical stability of charged black branes and the Gubser-Mitra conjecture

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; BLACK BRANE; CALCULATION; COSMOLOGICAL PHENOMENA; COSMOS; ELEMENTARY PARTICLE; ENTROPY; HEAT; MAGNETISM; MATHEMATICAL ANALYSIS; PARAMETER; SPACE; THEORY; THERMODYNAMICS;

EID: 0037438307     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.67.024007     Document Type: Article
Times cited : (31)

References (29)
  • 8
    • 85038329225 scopus 로고    scopus 로고
    • Playing with Black Strings, hep-th/0205069
    • G.T. Horowitz, “Playing with Black Strings,” hep-th/0205069.
    • Horowitz, G.T.1
  • 9
    • 85038345184 scopus 로고    scopus 로고
    • Static Axisymmetric Vacuum Solutions and Non-Uniform Black Strings, hep-th/0209051
    • T. Wiseman, “Static Axisymmetric Vacuum Solutions and Non-Uniform Black Strings,” hep-th/0209051.
    • Wiseman, T.1
  • 18
    • 85038336550 scopus 로고    scopus 로고
    • Proceedings of the 11th Workshop on General Relativity and Gravitation, Tokyo, Japan, 2002, hep-th/0202147
    • G. Kang, in Proceedings of the 11th Workshop on General Relativity and Gravitation, Tokyo, Japan, 2002, hep-th/0202147.
    • Kang, G.1
  • 26
    • 85038291098 scopus 로고    scopus 로고
    • L. D. Landau and E. M. Lifshitz, Statistical Physics, 3rd ed. (Pergamon, Oxford, 1980), Part 1
    • L. D. Landau and E. M. Lifshitz, Statistical Physics, 3rd ed. (Pergamon, Oxford, 1980), Part 1.
  • 27
    • 85038327889 scopus 로고    scopus 로고
    • For massless modes, the perturbation equations become equivalent to those for black hole backgrounds, which are expected to be stable
    • For massless modes, the perturbation equations become equivalent to those for black hole backgrounds, which are expected to be stable.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.