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Bosonic und Fermionic Quasinormal Modes of Rotating Black Holes Through AdS/CFT
High Energy Physics - Theory · Submitted 25 Oct 2022
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim We end with a brief discussion of the implications onto Strong Cosmic Censorship for the near horizon scalar and fermonic modes.
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The abstract, sentence by sentence
We study the holographic duals of bosonic and fermionic fields and compute their Quasinormal Frequencies (QNF) by exploiting that they are massive charged fields in $\mathrm{AdS_2 \times \mathcal{K}}$. In particular, we assess the stability of the scalar and fermionic operators in Myers-Perry's black holes with equal angular momenta. We compute the central charge and the Hawking-entropy and introduce extremality parameters to determine the properties of the dual CFT. Then, we briefly discuss how detection of Spin-2 fields can pave the way for more deep understanding of the holographic principles. We end with a brief discussion of the implications onto Strong Cosmic Censorship for the near horizon scalar and fermonic modes.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We study the holographic duals of bosonic and fermionic fields and compute their Quasinormal Frequencies (QNF) by exploiting that they are massive charged fields in $\mathrm{AdS_2 \times \mathcal{K}}$. | contribution 0.86 | 0.95 | 0.10 | asserted 1.00 |
| s1 | In particular, we assess the stability of the scalar and fermionic operators in Myers-Perry's black holes with equal angular momenta. | contribution 0.99 | 0.86 | 0.12 | asserted 0.93 |
| s2 | We compute the central charge and the Hawking-entropy and introduce extremality parameters to determine the properties of the dual CFT. | contribution 0.66 | 0.93 | 0.09 | asserted 1.00 |
| s3 | Then, we briefly discuss how detection of Spin-2 fields can pave the way for more deep understanding of the holographic principles. | future work 0.90 | 0.22 | 0.05 | hedged possibility 0.88 |
| s4 | We end with a brief discussion of the implications onto Strong Cosmic Censorship for the near horizon scalar and fermonic modes. | interpretation 0.97 | 0.55 | 0.16 | unclear 0.78 |
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The paper
Original abstract
We study the holographic duals of bosonic and fermionic fields and compute their Quasinormal Frequencies (QNF) by exploiting that they are massive charged fields in $\mathrm{AdS_2 \times \mathcal{K}}$. In particular, we assess the stability of the scalar and fermionic operators in Myers-Perry's black holes with equal angular momenta. We compute the central charge and the Hawking-entropy and introduce extremality parameters to determine the properties of the dual CFT. Then, we briefly discuss how detection of Spin-2 fields can pave the way for more deep understanding of the holographic principles. We end with a brief discussion of the implications onto Strong Cosmic Censorship for the near horizon scalar and fermonic modes.
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What this paper does with the arXiv papers it cites
What it cites · 1 sentence without a confident label
Compares with 1 paper
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This is a solution of the differential equation [ref] :
Eigenvalue repulsions and quasinormal mode spectra of Kerr-Newman: an extended study · Kerr-Solution · 0.82
Cites as support 1 paper
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Recent analysis of GW has shown this to be the case [ref] .
Thermal Ringdown of a Kerr Black Hole: Overtone Excitation, Fermi-Dirac Statistics and Greybody Factor · Discussion and Conclusion · 0.98
Cites as background 1 paper
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In a paper by [ref] , the NH region was closely examined in the classical context of GR.
Eigenvalue repulsions and quasinormal mode spectra of Kerr-Newman: an extended study · Kerr-Solution · 0.92
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