Hidden conformal symmetry for dyonic Kerr-Sen black hole and its gauged family
arXiv:2208.02722 · doi:10.1140/epjc/s10052-023-11412-2
Abstract
Motivated by advanced progress in the holographic theory between rotating black holes and CFT, we explore the conformal invariance on dyonic Kerr-Sen black hole and its gauged family. We consider a neutral massless scalar probe on the black holes' background within the low-frequency limit and exhibit that the solution space possesses isometry. The periodic identification of the azimuthal angle corresponds to the spontaneous conformal symmetry breaking by temperatures . Using the computation of the central charges on Ref. [25] that we recalculate by considering the contributions of all associated fields, we successfully derive the Bekenstein-Hawking entropy from Cardy entropy formula. Furthermore, we also calculate the absorption cross-section from gravity side for generic non-extremal dyonic Kerr-Sen black hole and near-extremal gauged dyonic Kerr-Sen black hole. Our calculations show that those quantities are in a perfect match with the calculation from CFT. Therefore, our findings further support the duality between rotating black holes and CFTs.
arXiv comment13 pages, published in Eur. Phys. J. C
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- Thermodynamic topology of Kerr-Sen black holes via Rényi statistics
- Chaos and fast scrambling delays of dyonic Kerr-Sen-AdS black hole and its ultra-spinning version
- Dual CFT on Dyonic Kerr-Sen black hole and its gauged and ultraspinning counterparts
- Cooling and heating regions of Joule-Thomson expansion for AdS black holes: Einstein-Maxwell-Power-Yang-Mills and Kerr Sen black holes
- Dual CFT on Nariai limit for Kerr-Sen-dS black holes
- Stationary Solution to Charged Hairy Black Hole in AdS4: Kasner Interior, Rotating Shock Waves, and Fast Scrambling
- Near-extremal Kerr-like ECO in the Kerr/CFT Correspondence in Higher Spin Perturbations