Pith. Sign in

RECORD

Quasitopological Lifshitz dilaton black brane

High Energy Physics - Theory · Submitted 25 Aug 2024

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

The authors' main claim Our results show that the quasitopological Lifshitz dilaton black brane solutions are thermally stable for each positive values of the dynamical critiacl exponent, $z$.

how it is stated · asserted 1.00 read the record →

Comment (0) Read on arXiv ↗
Cite ▾
arXiv ID2408.14516 (version 1)
Pith IDH5NLDNUA, Pith's permanent record of this paper and its review
CitationA. Bazrafshan, Gh. Forozani, M. Ghanaatian, S. Rezaei. "Quasitopological Lifshitz dilaton black brane." arXiv:2408.14516 (2024). https://pith.science/paper/H5NLDNUA
Claim paper

The compiled record

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.

Open the compiled record

Compiled by classifier-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-09-23: 1 request, 7,600 input tokens.

What the abstract itself states, as probabilities: claims first 0.17 · states limitation 0.92 · human participants 0.01 · controlled comparison 0.01 · randomized assignment 0.01 · states quantitative result 0.18 · compares with prior results 0.06 · mentions code or data availability 0.02.

The abstract, sentence by sentence

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

We construct a new class of $(n+1)$-dimensional Lifshitz dilaton black brane solutions in the presence of the cubic quasitopological gravity for a flat boundary. The related action supports asymptotically Lifshitz solutions by applying some conditions which are used throughout the paper. We have to add a new boundary term and some new counterterms to the bulk action to have finite solutions. Then we define a finite stress tensor complex by which we can calculate the energy density of the quasitopological Lifshitz dilaton black brane. It is not possible to obtain analytical solutions, and so we use some expantions to probe the functions behaviors near the horizon and at the infinity. Combining the equations, we can attain a total constant along the coordinate $r$. At the horizon, this constant is proportional to the product of the temperature and the entropy and at the infinity, the total constant shows the energ density of the quasitopological Lifshitz dilaton black brane. Therefore, we can reach to a relation between the conserved quantities temperature, entropy and the energy density and get a smarr-type formula. Using the first law of thermodynamics, we can find a relation between the entropy and the temperature and then ontain the heat capacity. Our results show that the quasitopological Lifshitz dilaton black brane solutions are thermally stable for each positive values of the dynamical critiacl exponent, $z$.

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 We construct a new class of $(n+1)$-dimensional Lifshitz dilaton black brane solutions in the presence of the cubic quasitopological gravity for a flat boundary. contribution 1.00 0.96 0.10 asserted 1.00
s1 The related action supports asymptotically Lifshitz solutions by applying some conditions which are used throughout the paper. method 0.53 0.38 0.04 asserted 0.98
s2 We have to add a new boundary term and some new counterterms to the bulk action to have finite solutions. method 0.86 0.89 0.03 asserted 1.00
s3 Then we define a finite stress tensor complex by which we can calculate the energy density of the quasitopological Lifshitz dilaton black brane. method 0.81 0.94 0.04 asserted 0.95
s4 It is not possible to obtain analytical solutions, and so we use some expantions to probe the functions behaviors near the horizon and at the infinity. method 0.64 0.87 0.02 asserted 1.00
s5 Combining the equations, we can attain a total constant along the coordinate $r$. result 0.48 0.92 0.03 asserted 0.77
s6 At the horizon, this constant is proportional to the product of the temperature and the entropy and at the infinity, the total constant shows the energ density of the quasitopological Lifshitz dilaton black brane. result 0.56 0.89 0.08 asserted 1.00
s7 Therefore, we can reach to a relation between the conserved quantities temperature, entropy and the energy density and get a smarr-type formula. result 0.89 0.95 0.21 asserted 0.90
s8 Using the first law of thermodynamics, we can find a relation between the entropy and the temperature and then ontain the heat capacity. method 0.83 0.94 0.06 asserted 0.89
s9 Our results show that the quasitopological Lifshitz dilaton black brane solutions are thermally stable for each positive values of the dynamical critiacl exponent, $z$. result 0.99 0.95 0.74 asserted 1.00

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

What was examined, and what was not

sources read
  • arXiv listing abstract v1
not examined
  • full text
  • figures and tables
  • references and citing sentences
  • relations to other papers
levels run
  • P abstract
not run
  • S sections
  • T body sentences
  • C citations
  • R cross-paper relations

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

We construct a new class of $(n+1)$-dimensional Lifshitz dilaton black brane solutions in the presence of the cubic quasitopological gravity for a flat boundary. The related action supports asymptotically Lifshitz solutions by applying some conditions which are used throughout the paper. We have to add a new boundary term and some new counterterms to the bulk action to have finite solutions. Then we define a finite stress tensor complex by which we can calculate the energy density of the quasitopological Lifshitz dilaton black brane. It is not possible to obtain analytical solutions, and so we use some expantions to probe the functions behaviors near the horizon and at the infinity. Combining the equations, we can attain a total constant along the coordinate $r$. At the horizon, this constant is proportional to the product of the temperature and the entropy and at the infinity, the total constant shows the energ density of the quasitopological Lifshitz dilaton black brane. Therefore, we can reach to a relation between the conserved quantities temperature, entropy and the energy density and get a smarr-type formula. Using the first law of thermodynamics, we can find a relation between the entropy and the temperature and then ontain the heat capacity. Our results show that the quasitopological Lifshitz dilaton black brane solutions are thermally stable for each positive values of the dynamical critiacl exponent, $z$.

Human review
How the literature uses it

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 · 30 sentences without a confident label

Uses the method or tool of 6 papers
  • However, we can specify a stress tensor complex for the asymptotically Lifshitz spacetimes [ref] that consists of energy density $ℰ$, energy flux $ℰ_i$, momentum density $𝒫_i$, and spatial stress tensor $𝒫_ij$ by the bellow formula [equation] and [equation] The above conserved quantities obey the bellow conservation equations [ref] [equation] Using Eqs. [ref]-[ref], we calculate the energy density of the quasitopological Lifshitz dilaton black brane as this [equation] If we replace the large $r$ expansions [ref] in Eq. [ref], so we can attain the mass of this black brane as the following [equation] where $C_tot$ is the total constant at the infinity that has been defined in Eq. [ref].

    Thermodynamics of Lovelock-Lifshitz Black Branes · Thermodynamics and conserved quantities · 0.89

  • However, we can specify a stress tensor complex for the asymptotically Lifshitz spacetimes [ref] that consists of energy density $ℰ$, energy flux $ℰ_i$, momentum density $𝒫_i$, and spatial stress tensor $𝒫_ij$ by the bellow formula [equation] and [equation] The above conserved quantities obey the bellow conservation equations [ref] [equation] Using Eqs. [ref]-[ref], we calculate the energy density of the quasitopological Lifshitz dilaton black brane as this [equation] If we replace the large $r$ expansions [ref] in Eq. [ref], so we can attain the mass of this black brane as the following [equation] where $C_tot$ is the total constant at the infinity that has been defined in Eq. [ref].

    Holographic stress tensor for non-relativistic theories · Thermodynamics and conserved quantities · 0.89

  • However, we can specify a stress tensor complex for the asymptotically Lifshitz spacetimes [ref] that consists of energy density $ℰ$, energy flux $ℰ_i$, momentum density $𝒫_i$, and spatial stress tensor $𝒫_ij$ by the bellow formula [equation] and [equation] The above conserved quantities obey the bellow conservation equations [ref] [equation] Using Eqs. [ref]-[ref], we calculate the energy density of the quasitopological Lifshitz dilaton black brane as this [equation] If we replace the large $r$ expansions [ref] in Eq. [ref], so we can attain the mass of this black brane as the following [equation] where $C_tot$ is the total constant at the infinity that has been defined in Eq. [ref].

    Thermodynamics of Rotating Lovelock-Lifshitz Black Branes · Thermodynamics and conserved quantities · 0.89

Compares with 1 paper
Cites as background 11 papers

Discussion

Know something about this paper? Leave a comment, or highlight any passage above to comment on it.