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Geometry and Thermodynamics of Black Holes in Magnetic Fields ...

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Magnetised <strong>Black</strong> <strong>Holes</strong> <strong>in</strong> STU Supergravity• We can magnetise black holes <strong>in</strong> supergravities too. Currentlywe (Cvetič, Gibbons, Saleem, CNP) are look<strong>in</strong>g <strong>in</strong> the fourdimensionalSTU model (N = 2 supergravity coupled to 3vector multiplets). Now have four <strong>in</strong>dependent U(1) gaugefields, so four charges <strong>and</strong> four magnetic fields. We no use theO(4, 4) symmetry <strong>of</strong> the associated KK reduced 3-dimensionalsigma model to generate the magnetised solutions.• As well as magnetis<strong>in</strong>g electric black holes, it is also now<strong>of</strong> <strong>in</strong>terest to magnetise magnetically-charged black holes.Consider static black holes for simplicity. The metric isds 2 = H ds 2 3 + H−1 s<strong>in</strong> 2 θ (dφ − ωdt) 2 ,(ds 2 3 = −r(2 − 2m)dt2 + R 1 r 2 r 3 r 4 dθ 2 + R )1r 2 r 3 r 4r(r − 2m) dr2ω =4∑i=1[− p iB i+ p iB 1 B 2 B 3 B 4 [r i + (r − 2m) cos 2 ]θ]r,2r i 8B i r iH 2 1 ∏ 4 (=(1 + 1r 1 r 2 r 3 r2 B ip i cos θ) 2 + B2 i r 1r 2 r 3 r 44 i=1ri2r i = r + 2m s<strong>in</strong>h 2 δ i , p i = 2m s<strong>in</strong>h δ i cosh δ i .,]s<strong>in</strong> 2 θ ,

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