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

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Summary

The heat kernel method

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]

The scalar heat kernel
The fermion heat kernel
Integer spin fields
Half-integer spin fields
The Logarithmic Correction
Bosonic contribution
Fermionic contribution
The logarithmic correction
Conclusions and outlook
A The discrete modes for the graviton
B Discrete modes of the gravitino
C Zero modes of the gravitino in the graviphoton background
D Useful summation formulae

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