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Trace anomaly and Hawking effect in generic 2D dilaton gravity theories
General Relativity and Quantum Cosmology · Submitted 9 Oct 1995
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim A general and simple formula relating the magnitude of the Hawking effect to the dilaton potential evaluated on the horizon is derived.
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The abstract, sentence by sentence
Black hole solutions in the context of a generic matter-coupled two-dimensional dilaton gravity theory are discussed both at the classical and semiclassical level. Starting from general assumptions, a criterion for the existence of black holes is given. The relationship between conformal anomaly and Hawking radiation is extended to a broad class of two-dimensional dilaton gravity models. A general and simple formula relating the magnitude of the Hawking effect to the dilaton potential evaluated on the horizon is derived.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | Black hole solutions in the context of a generic matter-coupled two-dimensional dilaton gravity theory are discussed both at the classical and semiclassical level. | contribution 0.65 | 0.70 | 0.07 | asserted 0.92 |
| s1 | Starting from general assumptions, a criterion for the existence of black holes is given. | contribution 0.58 | 0.87 | 0.07 | asserted 1.00 |
| s2 | The relationship between conformal anomaly and Hawking radiation is extended to a broad class of two-dimensional dilaton gravity models. | contribution 0.73 | 0.86 | 0.28 | asserted 1.00 |
| s3 | A general and simple formula relating the magnitude of the Hawking effect to the dilaton potential evaluated on the horizon is derived. | result 0.94 | 0.95 | 0.61 | asserted 1.00 |
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The paper
Original abstract
Black hole solutions in the context of a generic matter-coupled two-dimensional dilaton gravity theory are discussed both at the classical and semiclassical level. Starting from general assumptions, a criterion for the existence of black holes is given. The relationship between conformal anomaly and Hawking radiation is extended to a broad class of two-dimensional dilaton gravity models. A general and simple formula relating the magnitude of the Hawking effect to the dilaton potential evaluated on the horizon is derived.
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References
How the literature uses it
7 arXiv papers cite this in 9 sentences
Papers citing it · 4 sentences without a confident label
Cites it as background 5 papers
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Other closely related approaches for scalar fields and 2-dimensional theories include [ref]
Entropy and Temperature From Black-Hole/Near-Horizon-CFT Duality · Effective Action and Hawking Temperature · 0.90
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For CGHS gravity, the relation between dilaton profiles and the ADM black hole mass is discussed in e.g. [ref] .
Entanglement between two evaporating black holes · ADM mass formula in Flat CGHS gravity · 0.91
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Since Hawking's original analysis of the density of quantum states in terms of Bogolyubov coefficients, analysis via effective actions and their associated energy momentum tensors of the semiclassical matter fields has been explored in various settings for arriving at $T_H$ [ref] .
Near-Extremal Kerr AdS2xS2 Solution and Black-Hole/Near-Horizion-CFT Duality · Black Hole Temperature and Effective Action · 0.98
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