Contents 1 Introduction 1.1 Why gravity is richer in d > 4 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1.2 Why gravity is more difficult in d > 4 . . . . . . . . . . . . . . . . . . . . . . . .

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Date: 2013-02-21 02:38:07 String theory General relativity Asymptotically flat spacetime Schwarzschild metric AdS black hole Hawking radiation Black brane Rotating black hole Higher-dimensional Einstein gravity Physics Black holes Kerr metric		Contents 1 Introduction 1.1 Why gravity is richer in d > 4 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1.2 Why gravity is more difficult in d > 4 . . . . . . . . . . . . . . . . . . . . . . . . Add to Reading List Source URL: www.advanced-astronomy-guru-rupnathji.net63.net Download Document from Source Website File Size: 841,47 KB Share Document on Facebook

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