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For a general three dimensional theory of (super-)gravity coupled to arbitrary matter fields with arbitrary set of higher derivative terms in the effective action, we give an algorithm for consistently truncating the theory to a theory of pure (super-)gravity with the gravitational sector containing only Einstein-Hilbert, cosmological constant and Chern-Simons terms.
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1985
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K. Sfetsos and K. Skenderis, “Microscopic derivation of the Bekenstein-Hawking entropy formula for non-extremal black holes,” Nucl. Phys. B 517
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A. Strominger, “Black hole entropy from near-horizon microstates,” JHEP 9802
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J. de Boer, “Six-dimensional supergravity on S**3 x AdS(3) and 2d conformal field theory,” Nucl. Phys. B 548
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K. Skenderis, “Black holes and branes in string theory,” Lect. Notes Phys. 541
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P. Kraus and F. Larsen, “Microscopic black hole entropy in theories with higher derivatives,” JHEP 0509
P. Kraus and F. Larsen, “Holographic gravitational anomalies,” JHEP 0601
2006
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2007
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K. Hanaki, K. Ohashi and Y. Tachikawa, “Supersymmetric Completion of an R 2 R^{2} Term in Five-Dimensional Supergravity,” Prog. Theor. Phys. 117
2007
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A. Castro, J. L. Davis, P. Kraus and F. Larsen, “5D attractors with higher derivatives,” JHEP 0704
2007
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A. Castro, J. L. Davis, P. Kraus and F. Larsen, “5D Black Holes and Strings with Higher Derivatives,” JHEP 0706
2007
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2005
Cited alongside, same era.
E. Witten, “Three-Dimensional Gravity Revisited,” arXiv:0706.3359 [hep-th]
Cited in the paper.
Cited in the paper.
M. Alishahiha, “On R 2 R^{2} corrections for 5D black holes,” arXiv:hep-th/0703099
Cited in the paper.