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Fake supersymmetry and extremal black holes. (English) Zbl 1342.83175

Summary: We derive the BPS type of first order differential equations for the rotating black hole solutions in the three-dimensional Einstein gravity coupled minimally with a self-interacting scalar field, using fake supersymmetry formalism. It turns out that the formalism is not complete and should be augmented by an additional equation to imply the full equations of motion. We identify this additional equation as a constraint by using an effective action method. By computing the renormalized boundary stress tensor, we obtain the mass and angular momentum of the black hole solutions of these first order equations and confirm that they saturate the BPS bound.

MSC:

83C57 Black holes
83E50 Supergravity
Full Text: DOI

References:

[1] K. Skenderis and P.K. Townsend, Gravitational stability and renormalization group flow, Phys. Lett. B 468 (1999) 46 [hep-th/9909070] [INSPIRE]. · Zbl 0993.83033
[2] O. DeWolfe, D. Freedman, S. Gubser and A. Karch, Modeling the fifth-dimension with scalars and gravity, Phys. Rev. D 62 (2000) 046008 [hep-th/9909134] [INSPIRE].
[3] D. Freedman, C. Núñez, M. Schnabl and K. Skenderis, Fake supergravity and domain wall stability, Phys. Rev. D 69 (2004) 104027 [hep-th/0312055] [INSPIRE]. · Zbl 1405.83073
[4] A. Ceresole and G. Dall’Agata, Flow equations for non-BPS extremal black holes, JHEP03 (2007) 110 [hep-th/0702088] [INSPIRE]. · doi:10.1088/1126-6708/2007/03/110
[5] M. Henneaux, C. Martinez, R. Troncoso and J. Zanelli, Black holes and asymptotics of 2 + 1 gravity coupled to a scalar field, Phys. Rev. D 65 (2002) 104007 [hep-th/0201170] [INSPIRE].
[6] C. Martinez, R. Troncoso and J. Zanelli, Exact black hole solution with a minimally coupled scalar field, Phys. Rev. D 70 (2004) 084035 [hep-th/0406111] [INSPIRE].
[7] Y. Kwon, S. Nam, J.-D. Park and S.-H. Yi, Extremal black holes and holographic c-theorem, Nucl. Phys. B 869 (2013) 189 [arXiv:1208.4509] [INSPIRE]. · Zbl 1262.83031 · doi:10.1016/j.nuclphysb.2012.12.016
[8] K. Hotta, Y. Hyakutake, T. Kubota, T. Nishinaka and H. Tanida, The CFT-interpolating black hole in three dimensions, JHEP01 (2009) 010 [arXiv:0811.0910] [INSPIRE]. · Zbl 1243.83045 · doi:10.1088/1126-6708/2009/01/010
[9] M. Bañados, C. Teitelboim and J. Zanelli, The black hole in three-dimensional space-time, Phys. Rev. Lett. 69 (1992) 1849 [hep-th/9204099] [INSPIRE]. · Zbl 0968.83514 · doi:10.1103/PhysRevLett.69.1849
[10] J.D. Brown and M. Henneaux, Central charges in the canonical realization of asymptotic symmetries: an example from three-dimensional gravity, Commun. Math. Phys. 104 (1986) 207 [INSPIRE]. · Zbl 0584.53039 · doi:10.1007/BF01211590
[11] M. Bañados, M. Henneaux, C. Teitelboim and J. Zanelli, Geometry of the (2 + 1) black hole, Phys. Rev. D 48 (1993) 1506 [gr-qc/9302012] [INSPIRE].
[12] J.P. Gauntlett, J.B. Gutowski, C.M. Hull, S. Pakis and H.S. Reall, All supersymmetric solutions of minimal supergravity in five-dimensions, Class. Quant. Grav. 20 (2003) 4587 [hep-th/0209114] [INSPIRE]. · Zbl 1045.83001 · doi:10.1088/0264-9381/20/21/005
[13] J. Bellorín and T. Ortín, A note on simple applications of the Killing spinor identities, Phys. Lett. B 616 (2005) 118 [hep-th/0501246] [INSPIRE]. · Zbl 1247.53061
[14] E. O Colgain and H. Samtleben, 3D gauged supergravity from wrapped M5-branes with AdS/CMT applications, JHEP02 (2011) 031 [arXiv:1012.2145] [INSPIRE]. · Zbl 1294.81182 · doi:10.1007/JHEP02(2011)031
[15] C. Hoyos-Badajoz, C. Núñez and I. Papadimitriou, Comments on the string dual to N = 1 SQCD, Phys. Rev. D 78 (2008) 086005 [arXiv:0807.3039] [INSPIRE].
[16] V. Balasubramanian and P. Kraus, A stress tensor for Anti-de Sitter gravity, Commun. Math. Phys. 208 (1999) 413 [hep-th/9902121] [INSPIRE]. · Zbl 0946.83013 · doi:10.1007/s002200050764
[17] L. Abbott and S. Deser, Stability of gravity with a cosmological constant, Nucl. Phys. B 195 (1982) 76 [INSPIRE]. · Zbl 0900.53033 · doi:10.1016/0550-3213(82)90049-9
[18] S. Deser and B. Tekin, Gravitational energy in quadratic curvature gravities, Phys. Rev. Lett. 89 (2002) 101101 [hep-th/0205318] [INSPIRE]. · Zbl 1267.83086 · doi:10.1103/PhysRevLett.89.101101
[19] S. Deser and B. Tekin, Energy in generic higher curvature gravity theories, Phys. Rev. D 67 (2003) 084009 [hep-th/0212292] [INSPIRE].
[20] J.D. Brown and J.W. York, Quasilocal energy and conserved charges derived from the gravitational action, Phys. Rev. D 47 (1993) 1407 [gr-qc/9209012] [INSPIRE].
[21] J. Gegenberg, C. Martinez and R. Troncoso, A finite action for three-dimensional gravity with a minimally coupled scalar field, Phys. Rev. D 67 (2003) 084007 [hep-th/0301190] [INSPIRE].
[22] Y. Kwon, S. Nam, J.-D. Park and S.-H. Yi, Holographic Renormalization and Stress Tensors in New Massive Gravity, JHEP11 (2011) 029 [arXiv:1106.4609] [INSPIRE]. · Zbl 1306.83066 · doi:10.1007/JHEP11(2011)029
[23] K. Sen, A. Sinha and N.V. Suryanarayana, Counterterms, critical gravity and holography, Phys. Rev. D 85 (2012) 124017 [arXiv:1201.1288] [INSPIRE].
[24] S. Nam, J.-D. Park and S.-H. Yi, Mass and angular momentum of black holes in new massive gravity, Phys. Rev. D 82 (2010) 124049 [arXiv:1009.1962] [INSPIRE].
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