INTERNATIONAL SPACE SCIENCE INSTITUTE SPATIUM

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Date: 2013-05-23 03:13:04 Stellar black hole Micro black hole Supermassive black hole Dark star Hawking radiation General relativity Primordial black hole No-hair theorem Compact star Physics Black holes Astronomy		INTERNATIONAL SPACE SCIENCE INSTITUTE SPATIUM Add to Reading List Source URL: www.issibern.ch Download Document from Source Website File Size: 753,05 KB Share Document on Facebook

	Kerr black holes with Proca hair Carlos Herdeiro∗, Eugen Radu† and Helgi R´ unarsson‡ Departamento de F´ısica da Universidade de Aveiro and Center for Research and Development in Mathematics and Applications (CI DocID: 1rofY - View Document
	On the topology of black holes in higher dimensions Greg Galloway University of Miami Introduction DocID: 1pVy0 - View Document
	Еlectromagnetic hair of astrophysical black holes Maxim Lyutikov (Purdue U.) • The "no hair" theorem is not applicable to black holes formed from collapse of a rotating neutron star. Rotating neutron stars can selfpro DocID: 1ajAG - View Document
	In physics, whenever we have an equality relation, both sides of the equation should be of the same type i.e. they must have the same dimensions. For example you cannot have a situation where the quantity on the right-ha DocID: 13G84 - View Document
	INTERNATIONAL SPACE SCIENCE INSTITUTE SPATIUM DocID: 12zii - View Document