Note on small black holes in AdSp × Sq | Zendy

Gary T. Horowitz | Zendy; Veronika E. Hubeny | Zendy

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Note on small black holes in AdS_p × S^q

Author(s) -

Gary T. Horowitz,

Veronika E. Hubeny

Publication year - 2000

Publication title -

journal of high energy physics

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 0.998

H-Index - 261

eISSN - 1126-6708

pISSN - 1029-8479

DOI - 10.1088/1126-6708/2000/06/031

Subject(s) - physics , schwarzschild radius , supergravity , horizon , mathematical physics , black hole (networking) , schwarzschild metric , spacetime , photon sphere , theoretical physics , charged black hole , quantum mechanics , supersymmetry , general relativity , astronomy , computer network , routing protocol , routing (electronic design automation) , computer science , link state routing protocol

It is commonly believed that small black holes in AdS_5 x S^5 can bedescribed by the ten dimensional Schwarzschild solution. This requires that theself-dual five-form (which is nonzero in the background) does not fall throughthe horizon and cause the black hole to grow. We verify that this is indeed thecase: There are static solutions to the five-form field equations in a tendimensional Schwarzschild spacetime. Similar results hold for other backgroundsAdS_p x S^q of interest in supergravity.Comment: 11 pages, 1 figur

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