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Thermodynamics of Rotating Lifshitz Dilaton Black Brane in Quartic Quasitopological gravity

High Energy Physics - Phenomenology · Submitted 7 Aug 2024

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

The authors' main claim We also study the thermal stability of the rotating quartic quasitopological Lifshitz dilaton black brane and it is not thermally stable.

how it is stated · asserted 1.00 read the record →

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arXiv ID2408.03710 (version 1)
Pith ID2MMMZP6M, Pith's permanent record of this paper and its review
CitationA. Bazrafshan, F. Esmaeili, Gh. Forozani, M. Ghanaatian. "Thermodynamics of Rotating Lifshitz Dilaton Black Brane in Quartic Quasitopological gravity." arXiv:2408.03710 (2024). https://pith.science/paper/2MMMZP6M
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Compiled by classifier-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-09-23: 1 request, 5,653 input tokens.

What the abstract itself states, as probabilities: claims first 0.04 · states limitation 0.92 · human participants 0.01 · controlled comparison 0.01 · randomized assignment 0.01 · states quantitative result 0.09 · compares with prior results 0.05 · mentions code or data availability 0.01.

The abstract, sentence by sentence

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

In this paper, we obtain the rotating Lifshitz dilaton black brane solutions in the presence of the quartic quasitopological gravity and then probe the related thermodynamics. At first, we obtain the field equations form which a total constant along the radial coordinate $r$ is deduced. Since we cannot solve the solutions exactly, so we investigate their asymptotic behaviors at the horizon and at the infinity. We attain the conserved and thermodynamic quantities such as temperature, angular velocity, entropy, the energy and the angular momentum densities of the rotating quartic quasitopological Lifshitz dilaton black brane. By evaluating the total constant at the horizon and the infinity, we can make a relation between the thermodynamic quantities and so get to a Smarr-type formula. We demonstrate that the thermodynamic quantities of this rotating black brane obey the first law of the thermodynamics. We also study the thermal stability of the rotating quartic quasitopological Lifshitz dilaton black brane and it is not thermally stable.

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 obtain the rotating Lifshitz dilaton black brane solutions in the presence of the quartic quasitopological gravity and then probe the related thermodynamics. contribution 1.00 0.96 0.12 asserted 1.00
s1 At first, we obtain the field equations form which a total constant along the radial coordinate $r$ is deduced. method 0.95 0.96 0.03 asserted 1.00
s2 Since we cannot solve the solutions exactly, so we investigate their asymptotic behaviors at the horizon and at the infinity. method 0.49 0.90 0.02 asserted 1.00
s3 We attain the conserved and thermodynamic quantities such as temperature, angular velocity, entropy, the energy and the angular momentum densities of the rotating quartic quasitopological Lifshitz dilaton black brane. result 0.68 0.96 0.17 asserted 1.00
s4 By evaluating the total constant at the horizon and the infinity, we can make a relation between the thermodynamic quantities and so get to a Smarr-type formula. result 0.59 0.95 0.13 hedged possibility 0.56
s5 We demonstrate that the thermodynamic quantities of this rotating black brane obey the first law of the thermodynamics. result 0.98 0.95 0.23 asserted 1.00
s6 We also study the thermal stability of the rotating quartic quasitopological Lifshitz dilaton black brane and it is not thermally stable. result 0.99 0.96 0.30 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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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 obtain the rotating Lifshitz dilaton black brane solutions in the presence of the quartic quasitopological gravity and then probe the related thermodynamics. At first, we obtain the field equations form which a total constant along the radial coordinate $r$ is deduced. Since we cannot solve the solutions exactly, so we investigate their asymptotic behaviors at the horizon and at the infinity. We attain the conserved and thermodynamic quantities such as temperature, angular velocity, entropy, the energy and the angular momentum densities of the rotating quartic quasitopological Lifshitz dilaton black brane. By evaluating the total constant at the horizon and the infinity, we can make a relation between the thermodynamic quantities and so get to a Smarr-type formula. We demonstrate that the thermodynamic quantities of this rotating black brane obey the first law of the thermodynamics. We also study the thermal stability of the rotating quartic quasitopological Lifshitz dilaton black brane and it is not thermally stable.

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What this paper does with the arXiv papers it cites

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

What it cites · 13 sentences without a confident label

Uses the method or tool of 2 papers
  • The killing vector of a rotating black brane is defined by [equation] where $Ω$ demonstrates the angular velocity of the Killing horizon by [equation] We can also calculate the entropy of the rotating quartic quasitopological Lifshitz dilaton black brane with a flat horizon as the following [ref] [equation] The temperature of the mentioned rotating black brane at the event horizon is also attained by [equation] where we have used of the near horizon expansions [ref] in order to gain the last term.

    Black Hole Entropy is Noether Charge · Thermodynamics · 0.95

  • We can have a finite action by combining a reference term in the spacetime that has been introduced through the substraction method of Brown and York [ref] .

    Temperature, Energy, and Heat Capacity of Asymptotically Anti-De Sitter Black Holes · Thermodynamics · 0.96

Cites as support 1 paper
  • In the quasitopological gravity, the causality is preserved since the constraints coming from the requiring positive energy fluxes condition are in accordance with the causality ones [ref] .

    Holographic studies of quasi-topological gravity · Introduction · 0.96

Cites as background 41 papers

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