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Thermodynamics and logarithmic corrections of symmergent black holes

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Riasat Ali, Rimsha Babar, Zunaira Akhtar, Ali Övgün

General Relativity and Quantum Cosmology · Submitted 24 Feb 2023

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

The authors' main claim It is determined that a stable model is generated by logarithmic corrections arising from thermal fluctuations.

how it is stated · asserted 1.00 read the record →

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arXiv ID2302.12875 (version 1)
Pith IDLQRMXC2H, Pith's permanent record of this paper and its review
CitationAli \"Ovg\"un, Riasat Ali, Rimsha Babar, Zunaira Akhtar. "Thermodynamics and logarithmic corrections of symmergent black holes." arXiv:2302.12875 (2023). https://pith.science/paper/LQRMXC2H
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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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Compiled by classifier-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-09-23: 1 request, 8,009 input tokens.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.07 · human participants 0.01 · controlled comparison 0.05 · randomized assignment 0.01 · states quantitative result 0.06 · compares with prior results 0.07 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v1. Results and the main claim are underlined; .

In this paper, we study quantum gravity effect on the symmergent black hole which is derived from quadratic-curvature gravity. To do so, we use the Klein-Gordon equation which is modified by generalized uncertainty principle (GUP). After solving the field equations, we examine the symmergent black hole's tunneling and Hawking temperature. We explore the graphs of the temperature through the outer horizon to check the GUP influenced conditions of symmergent black hole stability. We also explain how symmergent black holes behave physically when influenced by quantum gravity. The impacts of thermal fluctuations on the thermodynamics of a symmergent black holes spacetime are examined. We first evaluate the model under consideration's thermodynamic properties, such as its Hawking temperature, angular velocity, entropy, and electric potential. We evaluate the logarithmic correction terms for entropy around the equilibrium state in order to examine the impacts of thermal fluctuations. In the presence of these correction terms, we also examine the viability of the first law of thermodynamics. Finally, we evaluate the system's stability using the Hessian matrix and heat capacity. It is determined that a stable model is generated by logarithmic corrections arising from thermal fluctuations.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 In this paper, we study quantum gravity effect on the symmergent black hole which is derived from quadratic-curvature gravity. contribution 0.98 0.83 0.03 asserted 0.81
s1 To do so, we use the Klein-Gordon equation which is modified by generalized uncertainty principle (GUP). method 1.00 0.90 0.02 asserted 0.98
s2 After solving the field equations, we examine the symmergent black hole's tunneling and Hawking temperature. method 0.60 0.95 0.03 asserted 0.93
s3 We explore the graphs of the temperature through the outer horizon to check the GUP influenced conditions of symmergent black hole stability. method 0.62 0.94 0.04 asserted 0.70
s4 We also explain how symmergent black holes behave physically when influenced by quantum gravity. contribution 0.74 0.84 0.06 asserted 0.78
s5 The impacts of thermal fluctuations on the thermodynamics of a symmergent black holes spacetime are examined. contribution 0.99 0.88 0.04 asserted 0.85
s6 We first evaluate the model under consideration's thermodynamic properties, such as its Hawking temperature, angular velocity, entropy, and electric potential. method 0.60 0.94 0.03 asserted 0.98
s7 We evaluate the logarithmic correction terms for entropy around the equilibrium state in order to examine the impacts of thermal fluctuations. method 0.89 0.94 0.04 asserted 0.93
s8 In the presence of these correction terms, we also examine the viability of the first law of thermodynamics. method 0.55 0.92 0.04 unclear 0.51
s9 Finally, we evaluate the system's stability using the Hessian matrix and heat capacity. method 0.98 0.94 0.07 asserted 0.87
s10 It is determined that a stable model is generated by logarithmic corrections arising from thermal fluctuations. result 0.99 0.91 0.81 asserted 1.00

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

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  • references and citing sentences
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  • T body sentences
  • C citations
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Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

The paper
Original abstract

In this paper, we study quantum gravity effect on the symmergent black hole which is derived from quadratic-curvature gravity. To do so, we use the Klein-Gordon equation which is modified by generalized uncertainty principle (GUP). After solving the field equations, we examine the symmergent black hole's tunneling and Hawking temperature. We explore the graphs of the temperature through the outer horizon to check the GUP influenced conditions of symmergent black hole stability. We also explain how symmergent black holes behave physically when influenced by quantum gravity. The impacts of thermal fluctuations on the thermodynamics of a symmergent black holes spacetime are examined. We first evaluate the model under consideration's thermodynamic properties, such as its Hawking temperature, angular velocity, entropy, and electric potential. We evaluate the logarithmic correction terms for entropy around the equilibrium state in order to examine the impacts of thermal fluctuations. In the presence of these correction terms, we also examine the viability of the first law of thermodynamics. Finally, we evaluate the system's stability using the Hessian matrix and heat capacity. It is determined that a stable model is generated by logarithmic corrections arising from thermal fluctuations.

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5 arXiv papers cite this in 6 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

Papers citing it · 4 sentences without a confident label

Cites it as background 2 papers

What it cites · 52 sentences without a confident label

Uses the method or tool of 5 papers
  • Under the steepest decent method, the equation of corrected entropy takes the the following form [ref] [equation] By using the conditions $∂S̃/∂ξ=0$ and $∂^2 S̃/∂ξ^2>0$, the corrected entropy relation under the first-order corrections has been modified [ref] and by neglecting the higher order terms, the exact expression of entropy is expressed as [ref] [equation] where $ψ$ represents the logarithmic correction parameter.

    Logarithmic corrections of charged hairy black hole in (2+1) dimension · Thermal fluctuations · 0.80

  • Under the steepest decent method, the equation of corrected entropy takes the the following form [ref] [equation] By using the conditions $∂S̃/∂ξ=0$ and $∂^2 S̃/∂ξ^2>0$, the corrected entropy relation under the first-order corrections has been modified [ref] and by neglecting the higher order terms, the exact expression of entropy is expressed as [ref] [equation] where $ψ$ represents the logarithmic correction parameter.

    Thermal Fluctuations in a Charged AdS Black Hole · Thermal fluctuations · 0.80

  • Under the steepest decent method, the equation of corrected entropy takes the the following form [ref] [equation] By using the conditions $∂S̃/∂ξ=0$ and $∂^2 S̃/∂ξ^2>0$, the corrected entropy relation under the first-order corrections has been modified [ref] and by neglecting the higher order terms, the exact expression of entropy is expressed as [ref] [equation] where $ψ$ represents the logarithmic correction parameter.

    General Logarithmic Corrections to Black Hole Entropy · Thermal fluctuations · 0.80

Uses data or values from 1 paper
Cites as background 14 papers

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