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On 4D-Hawing Radiation from Effective Action
High Energy Physics - Theory · Submitted 3 Mar 1994
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim The result is applied to $4d$-black holes and it is shown that the energy momentum tensor derived from the (nonlocal) effective action contains the Hawking radiation.
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The paper's own sentences, arranged. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.
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The abstract, sentence by sentence
We determine the $s$-waves contribution of a scalar field to the four dimensional effective action for arbitrary spherically symmetric external gravitational fields. The result is applied to $4d$-black holes and it is shown that the energy momentum tensor derived from the (nonlocal) effective action contains the Hawking radiation. The luminosity is close to the expected one in the $s$-channel. The energy momentum tensor may be used as starting point to study the backreaction problem.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We determine the $s$-waves contribution of a scalar field to the four dimensional effective action for arbitrary spherically symmetric external gravitational fields. | contribution 0.98 | 0.95 | 0.08 | asserted 1.00 |
| s1 | The result is applied to $4d$-black holes and it is shown that the energy momentum tensor derived from the (nonlocal) effective action contains the Hawking radiation. | result 0.94 | 0.93 | 0.74 | asserted 1.00 |
| s2 | The luminosity is close to the expected one in the $s$-channel. | result 0.97 | 0.87 | 0.13 | asserted 0.90 |
| s3 | The energy momentum tensor may be used as starting point to study the backreaction problem. | future work 0.95 | 0.37 | 0.07 | hedged possibility 1.00 |
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The paper
Original abstract
We determine the $s$-waves contribution of a scalar field to the four dimensional effective action for arbitrary spherically symmetric external gravitational fields. The result is applied to $4d$-black holes and it is shown that the energy momentum tensor derived from the (nonlocal) effective action contains the Hawking radiation. The luminosity is close to the expected one in the $s$-channel. The energy momentum tensor may be used as starting point to study the backreaction problem.
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References
How the literature uses it
13 arXiv papers cite this in 14 sentences
Papers citing it · 10 sentences without a confident label
Uses its method or tool 1 paper
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For $N≫1$ the one-loop effective action describing the semiclassical back-reaction due to this matter sector is given by adding the following conformal anomaly term to the action [ref] , S_q = - N/12 ∫d^2x √(-g) ( 1/2 R ^-1 R - 6 (∇r)^2/r^2 ^-1 R - 6 R lnr ) .
Thermodynamics of Large AdS Black Holes · One-loop action · 0.83
Cites it as background 3 papers
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In the nineties, other approaches based on effective action have been proposed [ref] - [ref] .
Thermodynamics of nonspherical black holes from Liouville theory · Introduction · 0.97
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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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The derivation of $T_H$ via effective actions and their associated energy-momentum-tensors of semiclassical scalars has been explored in various settings [ref] .
A Near Horizon CFT Dual for Kerr-Newman-$AdS$ · Introduction · 0.96
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