Lectures on Black Holes and the AdS3/CFT2 Correspondence
By Per Kraus. 2006
384 citations recorded by the source corpus.
We present a detailed discussion of AdS_3 black holes and their connection to two-dimensional conformal field theories via the AdS/CFT correspondence. Our emphasis is on deriving refined versions of black hole partition functions that include the effect of higher derivative terms in the spacetime action as well as non-perturbative effects. We include background material on gravity in AdS_3, in the context of holographic renormalization.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics
View Paper: https://www.semanticscholar.org/paper/0c98adf7ffaa1196ebc5020d199103671494a0ad
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Citations in the corpus
- Black holes, black rings and their microstates (2007, background): “Reviews of this can be found in [ 60 , 61], and a limited sample of work that is related to the exploration presented here can be found in [62, 63, 64, 65, 66, 145, 146, 147, 148, 149].”
- Two-dimensional SCFTs from wrapped branes and c-extremization (2013, background): “Most of the material presented in the first part is nicely reviewed in [57, 58], while some details were discussed in [59].”
- On renormalization group flows and the a-theorem in 6d (2012, neutral): “The ten dimensional string frame geometry is [39] ds(2) = (Z1Z5) −1/2(−dt2 + dx(2)) + (Z1Z5)(dr(2) + r(2)dΩ(2)3) + (Z1/Z5)1/2ds2M4 , (C.”
- Black hole entropy function, attractors and precision counting of microstates (2007, methodology): “As long as the near horizon geometry of the black hole is given by a locally AdS3 space, the results (4.2.6), (4.2.8) are exact.”
- Asymptotically flat spacetimes in three-dimensional higher spin gravity (2013, background): “[27] P.”
- The Weak Gravity Conjecture in three dimensions (2016, background): “, [52, 64]) that its contribution precisely agrees with (4.”
- Thermodynamics of higher spin black holes in AdS3 (2013, background): “To this end, it is useful to consider the following change of coordinates [30]: z = 1− iτ 2 w + 1 + iτ 2 w̄ (4.”
- Symmetries in Quantum Field Theory and Quantum Gravity (2018, background): “In AdS the natural boundary conditions for Maxwell-Chern Simons theory are to set either the left-moving or right-moving part of the pullback of A to the AdS boundary to zero, and also to require the vanishing of the pullback of ?F there [109, 110].”
- A theory of reparameterizations for AdS3 gravity (2018, background): “[53]), which exhibits the requisite Cardy-like growth at high temperature.”
- Higher spin black holes (2011, result): “q 3 4 compared to the entropy at W = 0. This behavior is to be contrasted with that of the BTZ black hole, or its charged generalizations with respect to bulk U(1) gauge fields [ 41 ].”
- Higher spin black holes from CFT (2012, background): “There have been some ideas that the relevant transformation property will be of the same structure (3)In particular, this argument relies on the spectral flow automorphism of the U(1) current algebra, see for example [29].”