Kerr black hole and black string intersecting M-brane
説明
We find eleven dimensional non-BPS black M-brane solutions from Kerr solution inM-theory by using U-duality. Under the transformation four dimensional Kerrmetric change to non-BPS rotating intersecting M-brane solutions. To easyapplication for AdS/CFT correspondence we must need a supersymmetric black branesolution, which limits special configuration of M-branes, e.g., M2-M2-M2 branesin five dimensional black brane and M5-M5-M5 brane with pp-wave in fourdimensional one. In this case we may easily apply the AdS/CFT correspondence fornon-BPS black hole solutions.
収録刊行物
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- Proceedings of Black Holes in General Relativity and String Theory — PoS(BHs, GR and Strings)
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Proceedings of Black Holes in General Relativity and String Theory — PoS(BHs, GR and Strings) 034-, 2009-10-12
Sissa Medialab
