Hairy Holes

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A second Hairy mans hole, just waiting to be entered, or possibly a Dorcas cave (its just not as funny) This looked a lot more promising. Listeners: Ken Ford, Duration: 1 minute, 19 seconds, Date story recorded: December 1996, Date story went live: 24 January 2008. Vote up content that is on-topic, within the rules/guidelines, and will likely stay relevant long-term. If the "yes hair theorem" stands up to scrutiny, he said it could be the first step in connecting the theories of relativity - which concern gravity and quantum mechanics which largely focus on the three other forces of nature, which are electromagnetism and two nuclear forces.

On the other hand, for shift symmetric theories of Horndeski and beyond Horndeski, black holes involve two classes of solutions: those that include, at the level of the action, a linear coupling to the Gauss–Bonnet term and those that involve time dependence in the galileon field. Scott is a bold and confident actor, who isn’t afraid of being vulnerable on stage, acting out orgasms and sex scenes on her own.The first version of the no-hair theorem for the simplified case of the uniqueness of the Schwarzschild metric was shown by Werner Israel in 1967. Now Vitor Cardoso of the Technical University of Lisbon in Portugal and his colleagues have a new way to give black holes hair. Numerical relativity simulations, originally developed to understand strong-field astrophysical processes, could prove extremely useful to understand HEP processes such as trans-Planckian scattering and gauge–gravity dualities. Magnetic charge, if detected as predicted by some theories, would form the fourth parameter possessed by a classical black hole.

It was conjectured in [1, 2], that the existence of such clouds at the linear level implies the existence of a new family of BH solutions at the nonlinear level.

The time-dependent solutions describe homogeneous (isotropic or anisotropic) cosmologies which show a late-time self-acceleration or other types of behavior.