Abstract
We compute the logarithmic correction to black hole entropy about exponentially suppressed saddle points of the Quantum Entropy Function corresponding to ℤ N orbifolds of the near horizon geometry of the extremal black hole under study. By carefully accounting for zero mode contributions we show that the logarithmic contributions for quarter-BPS black holes in $$ \mathcal{N}=4 $$ supergravity and one-eighth BPS black holes in $$ \mathcal{N}=8 $$ supergravity perfectly match with the prediction from the microstate counting. We also find that the logarithmic contribution for half-BPS black holes in $$ \mathcal{N}=2 $$ supergravity depends non-trivially on the ℤ N orbifold. Our analysis draws heavily on the results we had previously obtained for heat kernel coefficients on ℤ N orbifolds of spheres and hyperboloids in arXiv:1311.6286 and we also propose a generalization of the Plancherel formula to ℤ N orbifolds of hyperboloids to an expression involving the Harish-Chandra character of sl (2, R), a result which is of possible mathematical interest.
Highlights
Where we have set all fundamental constants except the Newton’s constant to one
We compute the logarithmic correction to black hole entropy about exponentially suppressed saddle points of the Quantum Entropy Function corresponding to ZN orbifolds of the near horizon geometry of the extremal black hole under study
By carefully accounting for zero mode contributions we show that the logarithmic contributions for quarter-BPS black holes in N = 4 supergravity and one-eighth BPS black holes in N = 8 supergravity perfectly match with the prediction from the microstate counting
Summary
We note here that the number of zero modes (3.5) can be read off from the coefficient of the e0 term in the full heat kernel expansion (3.3). Gravitini and gravitons in a basis of states obtained by acting derivatives and gamma matrices on scalars and Dirac fermions, as applicable This is outlined partially in appendices A and B, and we further refer the reader to [33, 34] for complete details. For this reason, we shall concentrate on the heat kernels over over scalars and Dirac fermions on AdS2 ⊗ S2 /ZN , reviewing the expressions obtained in [35]
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.