Difference between revisions of "The No-Hair Theorem Parameters can be Reduced to solely the Black Hole's Specific Angular Momentum"
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| − | [[Category:Expansion Tectonics]] | + | [[Category:Expansion Tectonics|no-hair theorem parameters reduced solely black hole 's specific angular momentum]] |
| − | [[Category:Gravity]] | + | [[Category:Gravity|no-hair theorem parameters reduced solely black hole 's specific angular momentum]] |
| − | [[Category:Cosmology]] | + | [[Category:Cosmology|no-hair theorem parameters reduced solely black hole 's specific angular momentum]] |
Latest revision as of 20:04, 1 January 2017
| Scientific Paper | |
|---|---|
| Title | The No-Hair Theorem Parameters can be Reduced to solely the Black Hole\'s Specific Angular Momentum |
| Read in full | Link to paper |
| Author(s) | Thierry De Mees |
| Keywords | Coriolis Gravity, Gravitomagnetism, No-Hair Theorem, black hole, star, specific angular velocity, specific gravity |
| Published | 2011 |
| Journal | General Science Journal |
| No. of pages | 3 |
Read the full paper here
Abstract
The physicist John Wheeler is told having made a famous remark, "Black holes have no hair." This referred to the postulate that all black hole solutions of the general relativity, better, of the Einstein-Maxwell equations of gravitation, and of electromagnetism, can be completely characterized by only three externally observable classical parameters: mass, electric charge, and angular momentum, when observed from outside its event horizon. I show here that consequently, Gravitomagnetism is fully compatible with the No-Hair Theorem. Also, I deduce here that for a globally electrically neutral black hole, the No-Hair Theorem can be reduced to the knowledge of its specific angular momentum only, without the need of its gravitational attributes. Finally, I deduce the black hole's angular momentum out of the black holes' observed gravitational properties upon an orbiting object.
