Quantum evolution of near-extremal Reissner-Nordstrom black holes

A. Fabbri; D. J. Navarro; J. Navarro-Salas

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Quantum evolution of near-extremal Reissner-Nordstrom black holes

A. Fabbri, D. J. Navarro, J. Navarro-Salas

High Energy Physics - Theory · Submitted 5 Jun 2000

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim We describe analytically the evaporation process which turns out to be compatible with the third law of thermodynamics, i.e., an infinite amount of time is required for the black hole to decay to extremality.

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arXiv IDhep-th/0006035 (version 2)

Pith IDTAGYX74M, Pith's permanent record of this paper and its review

CitationA. Fabbri, D. J. Navarro, J. Navarro-Salas. "Quantum evolution of near-extremal Reissner-Nordstrom black holes." arXiv:hep-th/0006035 (2000). https://pith.science/paper/TAGYX74M

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What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.31 · human participants 0.01 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.15 · compares with prior results 0.12 · mentions code or data availability 0.01.

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arXiv listing abstract v2. Results and the main claim are underlined; show every role.

We study the near-horizon AdS_2\timesS^2 geometry of evaporating near-extremal Reissner-Nordstrom black holes interacting with null matter. The non-local (boundary) terms t_{\pm}, coming from the effective theory corrected with the quantum Polyakov-Liouville action, are treated as dynamical variables. We describe analytically the evaporation process which turns out to be compatible with the third law of thermodynamics, i.e., an infinite amount of time is required for the black hole to decay to extremality. Finally we comment briefly on the implications of our results for the information loss problem.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#	sentence	role	the authors' own work	states the main conclusion	strength
s0	We study the near-horizon AdS_2\timesS^2 geometry of evaporating near-extremal Reissner-Nordstrom black holes interacting with null matter.	contribution 0.98	0.84	0.04	asserted 0.80
s1	The non-local (boundary) terms t_{\pm}, coming from the effective theory corrected with the quantum Polyakov-Liouville action, are treated as dynamical variables.	method 0.94	0.56	0.04	asserted 0.98
s2	We describe analytically the evaporation process which turns out to be compatible with the third law of thermodynamics, i.e., an infinite amount of time is required for the black hole to decay to extremality.	result 0.98	0.92	0.77	asserted 0.80
s3	Finally we comment briefly on the implications of our results for the information loss problem.	interpretation 0.99	0.57	0.03	unclear 0.97

What kind of paper the classifier reports this is: theoretical result 1.00 · evidence from proof or derivation 1.00.

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arXiv listing abstract v2

not examined

full text
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P abstract

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The paper

Original abstract

We study the near-horizon AdS_2\timesS^2 geometry of evaporating near-extremal Reissner-Nordstrom black holes interacting with null matter. The non-local (boundary) terms t_{\pm}, coming from the effective theory corrected with the quantum Polyakov-Liouville action, are treated as dynamical variables. We describe analytically the evaporation process which turns out to be compatible with the third law of thermodynamics, i.e., an infinite amount of time is required for the black hole to decay to extremality. Finally we comment briefly on the implications of our results for the information loss problem.

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References

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Cited by 5 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

Explorations of Non-Perturbative JT Gravity and Supergravity
hep-th 2020-06 conditional novelty 6.0 of 10

Truncating an infinite-order string equation to six or seven minimal models gives explicit non-perturbative spectra and spectral form factors for JT gravity and two JT supergravities, showing how wormhole contribution...
JT Supergravity, Minimal Strings, and Matrix Models
hep-th 2020-05 conditional novelty 6.0 of 10

JT supergravity in the (2Γ+1,2) Altland-Zirnbauer family is defined non-perturbatively as a specific weighted sum of type 0A minimal string models, with a single nonlinear string equation supplying both perturbative a...
Semi-classical spacetime thermodynamics
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Derives semi-classical gravity from thermodynamics of stretched light cones in 2D dilaton gravity with explicit conformal anomaly backreaction and shows equations of motion follow from dynamical Wald entropy in Brans-...
Quasi-local energy and microcanonical entropy in two-dimensional nearly de Sitter gravity
hep-th 2022-03 accept novelty 5.0 of 10

The on-shell Euclidean microcanonical action of a causal diamond in semi-classical JT gravity equals minus the generalized entropy, so minimizing the action extremizes the entropy and yields the island rule in dS2 wit...
Dilaton Gravity in Two Dimensions
hep-th 2002-04 accept novelty 2.0 of 10

Two-dimensional dilaton gravity can be quantized exactly in its geometric sector, with matter handled perturbatively, and this review assembles the supporting results into a coherent framework.

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11 arXiv papers cite this in 11 sentences

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Papers whose main result relates to this one's

Found among the papers closest to this one by title and main claim. Pith's classifier compared each pair's main results and a second model family confirmed the relation; checked against two further families, shown conflicts agreed 118 times in 120 and shown same results 218 times in 239. The quoted sentence is the other paper's main claim.

States the same result 2 papers

We find that an infinite amount of time is required for the black hole to decay to extremality.

Evaporation of charged black holes near extremality · 1.00
The corresponding one-loop quantum theory remains solvable and allows to follow analytically the evaporation process which is shown to require an infinite amount of time.

Evaporation of near-extremal Reissner-Nordstrom black holes · 0.96

Papers citing it · 6 sentences without a confident label

Cites it as background 5 papers

Recently, there has been renewed interest in Jackiw–Teitelboim (JT) gravity [ref] , a two dimensional theory of gravity that emerges in various physical contexts, such as the study of the near–horizon dynamics of nearly extreme black holes [ref] , or as a partial gravitational dual of certain one–dimensional quantum mechanical systems pertinent to studies of condensed matter and quantum chaos.

JT Supergravity, Minimal Strings, and Matrix Models · Introduction · 1.00
Describing the low-energy dynamics of a wide class of near-extremal black holes and branes [ref] , JT gravity also features in a precise realization of holographic AdS$_2$/CFT$_1$, arising as the low-energy gravitational dual to the Sachdev-Ye-Kitaev (SYK) 1D quantum mechanical system [ref] .

A JT supergravity as a double-cut matrix model · Introduction · 0.97
A popular such model is classical JT gravity in $AdS_2$ [ref] , following from a spherical reduction of the Einstein–Hilbert action describing near-extremal black holes with near-horizon geometry $AdS_2×X$ [ref] , where $X$ is the transverse space whose size is controlled by the dilaton.

Quasi-local energy and microcanonical entropy in two-dimensional nearly de Sitter gravity · Two roads to de Sitter JT gravity · 0.99

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