Black holes with metric and fields of the same form

Details Black holes with metric and fields of the same form Black holes with metric and fields of the same form

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012gregr..44..157k&link_type=abstract

General Relativity and Gravitation, Volume 44, Issue 1, pp.157-199

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Black Hole Solutions, Metric And Fields Of The Same Form

Scientific paper

We present two rotating black hole solutions with axion ξ, dilaton {φ} and two U(1) vector fields. Starting from a non-rotating metric with three arbitrary parameters, which we have found previously, and applying the "Newman-Janis complex coordinate trick" we get a rotating metric g μν with four arbitrary parameters namely the mass M, the rotation parameter a and the charges electric Q E and magnetic Q M . Then we find a solution of the equations of motion having this g μν as metric. Our solution is asymptotically flat and has angular momentum J = M a, gyromagnetic ratio g = 2, two horizons, the singularities of the solution of Kerr, axion and dilaton singular only when r = a cos θ = 0 etc. By applying to our solution the S-duality transformation we get a new solution, whose axion, dilaton and vector fields have one more parameter. The metrics, the vector fields and the quantity {λ=ξ+ie^{-2φ}} of our solutions and the solution of: Sen for Q E , Sen for Q E and Q M , Kerr-Newman for Q E and Q M , Kerr, Reference Kyriakopoulos [Class. Quantum Grav. 23:7591, 2006, Eqs. (54-57)], Shapere, Trivedi and Wilczek, Gibbons-Maeda-Garfinkle-Horowitz-Strominger, Reissner-Nordström, Schwarzschild are the same function of a, and two functions ρ 2 = r( r + b) + a 2 cos2 θ and Δ = r( r + b) - 2 Mr + a 2 + c, of a, b and two functions for each vector field, and of a, b and d respectively, where a, b, c and d are constants. From our solutions several known solutions can be obtained for certain values of their parameters. It is shown that our two solutions satisfy the weak the dominant and the strong energy conditions outside and on the outer horizon and that all solutions with a metric of our form, whose parameters satisfy some relations satisfy also these energy conditions outside and on the outer horizon. This happens to all solutions given in the "Appendix". Mass formulae for our solutions and for all solutions which are mentioned in the paper are given. One mass formula for each solution is of Smarr's type and another a differential mass formula. Many solutions with metric, vector fields and λ of the same functional form, which include most physically interesting and well known solutions, are listed in an "Appendix".

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