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On flat space limits of AdS4 black holes

Abstract

With a view towards understanding flat space holography, we study the flat space limit of asymptotically AdS4 black holes in gauged 𝒩=2 supergravity. Using holographic renormalisation, we carefully analyse the flat space limit of the on-shell action of various black holes in this setting and make explicit the states that contribute to the partition function in this limit. We find several features: large black holes lead to a divergence in the partition function which can be understood as a thermodynamic volume divergence. Meanwhile, semiclassically, small black holes reproduce the partition function of their flat space counterparts, and we clarify the mapping between BPS, (near-)extremal or non-extremal black holes on both sides for charged and rotating solutions. Finally, by studying a suitable flat limit of the BPS Kerr-Newman-AdS4 black hole in M-theory, we obtain a charged BPS solution in flat space. On the dual side, we determine a Carrollian-like limit on the known ABJM partition function on S1Γ— S2 at large N, and show that it reproduces the correct entropy of the BPS charged black hole in asymptotically flat space.

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BibTeX
@misc{marto2026flat,
  title = {{On flat space limits of $AdS_4$ black holes}},
  author = {Pedro Vicente Marto and Shradha Ramakrishnan and Stefan Vandoren},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2608.21518},
  eprint = {2608.21518},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2608.21518},
}
RIS
TY  - UNPB
TI  - On flat space limits of AdS_4 black holes
AU  - Pedro Vicente Marto
AU  - Shradha Ramakrishnan
AU  - Stefan Vandoren
PY  - 2026
DA  - 2026/09/14
PB  - arXiv
DO  - 10.48550/arxiv.2608.21518
UR  - https://arxiv.org/abs/2608.21518
AB  - With a view towards understanding flat space holography, we study the flat space limit of asymptotically AdS_4 black holes in gauged 𝒩=2 supergravity. Using holographic renormalisation, we carefully analyse the flat space limit of the on-shell action of various black holes in this setting and make explicit the states that contribute to the partition function in this limit. We find several features: large black holes lead to a divergence in the partition function which can be understood as a thermodynamic volume divergence. Meanwhile, semiclassically, small black holes reproduce the partition function of their flat space counterparts, and we clarify the mapping between BPS, (near-)extremal or non-extremal black holes on both sides for charged and rotating solutions. Finally, by studying a suitable flat limit of the BPS Kerr-Newman-AdS_4 black hole in M-theory, we obtain a charged BPS solution in flat space. On the dual side, we determine a Carrollian-like limit on the known ABJM partition function on S^1Γ— S^2 at large N, and show that it reproduces the correct entropy of the BPS charged black hole in asymptotically flat space.
ER  -