Warped AdS3 black holes in new massive gravity
By G. Clément. 2009
176 citations recorded by the source corpus.
We investigate stationary, rotationally symmetric solutions of a recently proposed three-dimensional theory of massive gravity. Along with BTZ black holes, we also obtain warped AdS3 black holes, and (for a critical value of the cosmological constant) AdS2 × S1 as solutions. The entropy, mass and angular momentum of these black holes are computed.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics
View Paper: https://www.semanticscholar.org/paper/04536bb578e6c9b51c93b4a57fc2cbb05096bdbe
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In Astronomy and Astrophysics
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Citations in the corpus
- Massive Gravity (2014, unknown): “In the case of NMG as well as the usual BTZ black holes obtained in the presence of a negative cosmological constant there are in a addition a class of warped AdS3 black holes [102] whose metric takes the form ds(2) = −β(2) ρ 2 − ρ(2)0 r2 dt(2) + r(2) ( dφ− ρ+ (1− β (2))ω r2 dt )2 + 1 β2ζ2 dρ(2) ρ2 ”
- On the z=4 Horava-Lifshitz Gravity (2009, background): “1Email: cairg@itp.ac.cn 2Email: liuyan@itp.ac.cn 3Email: sunyw@itp.ac.cn”
- More on Massive 3D Gravity (2009, methodology): “22) The metric is therefore locally isometric to adS2 × S(1) when σ = 1, which is the KK solution found previously in [15], and to dS2 × S(1) when σ = −1.”
- Massive 3D supergravity (2009, unknown): “Other investigations of this model include [11].”