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First and second laws of modified gravity theories on dynamical holographic screens

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Shao-Feng Wu, Xian-Hui Ge, Peng-Ming Zhang, Guo-Hong Yang

High Energy Physics - Theory · Submitted 12 Aug 2010

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The authors' main claim We show that field equations of some typical modified gravity theories can be recast as thermodynamic first law on dynamical holographic screens.

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arXiv ID1008.2072 (version 2)
Pith IDQWTY5MZR, Pith's permanent record of this paper and its review
CitationGuo-Hong Yang, Peng-Ming Zhang, Shao-Feng Wu, Xian-Hui Ge. "First and second laws of modified gravity theories on dynamical holographic screens." arXiv:1008.2072 (2010). https://pith.science/paper/QWTY5MZR
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What the abstract itself states, as probabilities: claims first 0.13 · states limitation 0.14 · human participants 0.01 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.03 · compares with prior results 0.06 · mentions code or data availability 0.02.

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

We show that field equations of some typical modified gravity theories can be recast as thermodynamic first law on dynamical holographic screens. The thermodynamic second law are also presented.

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#sentencerolethe authors' own workstates the main conclusionstrength
s0 We show that field equations of some typical modified gravity theories can be recast as thermodynamic first law on dynamical holographic screens. result 0.69 0.93 0.84 asserted 1.00
s1 The thermodynamic second law are also presented. result 0.60 0.80 0.16 asserted 0.97

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Original abstract

We show that field equations of some typical modified gravity theories can be recast as thermodynamic first law on dynamical holographic screens. The thermodynamic second law are also presented.

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2 arXiv papers cite this in 5 sentences

Each citing sentence is taken from the citing paper's LaTeX source and typed by Pith's classifier. A label appears at probability 0.8 or more (0.95 for support), a contest at 0.7 or more; the quoted words are the citing authors'. How each label was checked · JSON

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What it cites · 49 sentences without a confident label

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  • Similar to the monotonicity of Misner-Sharp energy on untrapped spheres [ref] , this second law has the physical interpretation that the entropy contained in an outer (inner) untrapped screen is non-decreasing as the screen is perturbed outwards (inwards) along the spatial or null tangent vector of the screen.

    Gravitational Energy in Spherical Symmetry · Second law of modified gravity theories on dynamical holographic screens · 0.91

Cites as background 5 papers
  • Moreover, Hayward also proved the monotonicity of Misner-Sharp energy on untrapped spheres [ref] , which states that if the dominant energy condition holds on an untrapped sphere, the Misner-Sharp energy is non-decreasing in any outgoing spatial or null direction.

    Gravitational Energy in Spherical Symmetry · Second law of modified gravity theories on dynamical holographic screens · 0.80

  • It is known that the entropy of stationary horizon is well defined by Wald entropy [ref] , which is a Noether charge associated with the Killing vector, but it is less understood for the horizon entropy in a dynamical spacetime, where the Killing vector can not be found in general.

    Black Hole Entropy is Noether Charge · Thermodynamical parameters on dynamical holographic screens · 0.98

  • Moreover, certain timelike screen is also proposed to repeat the local Rindler horizon thermodynamics [ref] .

    Gauss-Codazzi thermodynamics on the timelike screen · Introduction · 0.87

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