No-hair theorem

Results: 21



#Item
1Kerr 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

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

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Source URL: arxiv.org

Language: English - Date: 2016-03-09 20:10:11
2On the topology of black holes in higher dimensions Greg Galloway University of Miami  Introduction

On the topology of black holes in higher dimensions Greg Galloway University of Miami Introduction

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Source URL: xtsunxet.usc.es

Language: English - Date: 2007-03-09 06:07:01
3Еlectromagnetic hair of astrophysical black holes Maxim Lyutikov (Purdue U.) • The

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

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Source URL: www.oa.uj.edu.pl

Language: English - Date: 2015-05-26 01:48:10
4In 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

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

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Source URL: www.jyu.fi

Language: English - Date: 2007-08-14 12:15:32
5INTERNATIONAL SPACE SCIENCE INSTITUTE  SPATIUM

INTERNATIONAL SPACE SCIENCE INSTITUTE SPATIUM

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Source URL: www.issibern.ch

Language: English - Date: 2013-05-23 03:13:04
6event horizon  page 1 MOON SOUVENIR EDITION  THURSDAY, 20 MAY, 2010

event horizon page 1 MOON SOUVENIR EDITION THURSDAY, 20 MAY, 2010

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Source URL: www.ccp.org.au

Language: English - Date: 2010-08-23 23:12:45
7A Scenario for Strong Gravity in Particle Physics: An alternative mechanism for black holes to appear at accelerator experiments D. G. Coyne1• and D. C. Cheng2 1 2

A Scenario for Strong Gravity in Particle Physics: An alternative mechanism for black holes to appear at accelerator experiments D. G. Coyne1• and D. C. Cheng2 1 2

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Source URL: arxiv.org

Language: English - Date: 2009-05-11 14:24:46
8return to updates  NEW PHYSICS dies an ignominious death  by Miles Mathis

return to updates NEW PHYSICS dies an ignominious death by Miles Mathis

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Source URL: milesmathis.com

Language: English - Date: 2013-04-05 19:56:57
9Black	
  hole	
  quasinormal	
  modes	
  (QNMs)	
  	
   and	
  massive	
  scalar-­‐tensor	
  theories	
   1)  QNMs:	
  tests	
  within	
  GR	
   No-­‐hair	
  theorem,	
  area	
  theorem	
   Form

Black  hole  quasinormal  modes  (QNMs)     and  massive  scalar-­‐tensor  theories   1)  QNMs:  tests  within  GR   No-­‐hair  theorem,  area  theorem   Form

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Source URL: www.cfa.harvard.edu

Language: English - Date: 2012-09-14 15:02:32
10Testing GR with Merging Black Hole Binaries E. Sterl Phinney Caltech

Testing GR with Merging Black Hole Binaries E. Sterl Phinney Caltech

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Source URL: www.cfa.harvard.edu

Language: English - Date: 2012-05-16 10:29:38