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Weak Gravity Conjecture, Central Charges and $\eta/s$

High Energy Physics - Theory · Submitted 3 Mar 2010

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

The authors' main claim The result that follows from this example suggests that WGC makes the KSS conjecture to hold in the extremal limit but only when one of the coefficient vanishes ($c_1=0, c_2\neq 0$ or $c_2=0, c_1\neq 0$) and when both the coefficients are non zero it can respect and/or violate the KSS conjecture depending on the choice to $c_1$ at extremality, even though $\eta/s$ do not depend on $c_1$ at extremality.

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arXiv ID1003.0745 (version 2)
Pith ID2ALMU5QS, Pith's permanent record of this paper and its review
CitationShesansu Sekhar Pal. "Weak Gravity Conjecture, Central Charges and $\eta/s$." arXiv:1003.0745 (2010). https://pith.science/paper/2ALMU5QS
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Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 3,914 input tokens, $0.0002 reported.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.87 · human participants 0.01 · controlled comparison 0.05 · randomized assignment 0.01 · states quantitative result 0.32 · compares with prior results 0.34 · mentions code or data availability 0.01.

The abstract, sentence by sentence

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

We correlate the weak gravity conjecture (WGC), the KSS conjecture with chemical potential at extremality and the central charges by going through a particular example in five dimensional AdS spacetime with two unknown coefficients $c_1, c_2$, assuming WGC exists in AdS spacetime. The result that follows from this example suggests that WGC makes the KSS conjecture to hold in the extremal limit but only when one of the coefficient vanishes ($c_1=0, c_2\neq 0$ or $c_2=0, c_1\neq 0$) and when both the coefficients are non zero it can respect and/or violate the KSS conjecture depending on the choice to $c_1$ at extremality, even though $\eta/s$ do not depend on $c_1$ at extremality. Moreover, WGC is not fully compatible with the calculation of central charges even though the bounds on coefficient $c_1$ that follows from demanding WGC stays within the bounds that central charges predict. As usual, the KSS conjecture is violated, of course, in the non-extremal limit.

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 correlate the weak gravity conjecture (WGC), the KSS conjecture with chemical potential at extremality and the central charges by going through a particular example in five dimensional AdS spacetime with two unknown coefficients $c_1, c_2$, assuming WGC exists in AdS spacetime. contribution 0.68 0.87 0.08 asserted 0.91
s1 The result that follows from this example suggests that WGC makes the KSS conjecture to hold in the extremal limit but only when one of the coefficient vanishes ($c_1=0, c_2\neq 0$ or $c_2=0, c_1\neq 0$) and when both the coefficients are non zero it can respect and/or violate the KSS conjecture depending on the choice to $c_1$ at extremality, even though $\eta/s$ do not depend on $c_1$ at extremality. result 0.97 0.89 0.76 hedged possibility 0.99
s2 Moreover, WGC is not fully compatible with the calculation of central charges even though the bounds on coefficient $c_1$ that follows from demanding WGC stays within the bounds that central charges predict. result 0.96 0.81 0.15 asserted 0.99
s3 As usual, the KSS conjecture is violated, of course, in the non-extremal limit. result 0.46 0.25 0.06 asserted 1.00

What kind of paper the classifier reports this is: theoretical result 1.00 · evidence from proof or derivation 0.89.

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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

We correlate the weak gravity conjecture (WGC), the KSS conjecture with chemical potential at extremality and the central charges by going through a particular example in five dimensional AdS spacetime with two unknown coefficients $c_1, c_2$, assuming WGC exists in AdS spacetime. The result that follows from this example suggests that WGC makes the KSS conjecture to hold in the extremal limit but only when one of the coefficient vanishes ($c_1=0, c_2\neq 0$ or $c_2=0, c_1\neq 0$) and when both the coefficients are non zero it can respect and/or violate the KSS conjecture depending on the choice to $c_1$ at extremality, even though $\eta/s$ do not depend on $c_1$ at extremality. Moreover, WGC is not fully compatible with the calculation of central charges even though the bounds on coefficient $c_1$ that follows from demanding WGC stays within the bounds that central charges predict. As usual, the KSS conjecture is violated, of course, in the non-extremal limit.

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4 arXiv papers cite this in 8 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

Compares with it 2 papers
Cites it as background 2 papers

What it cites · 20 sentences without a confident label

Builds on 1 paper
  • Let us consider an effective action of the following type S=12κ^2∫√(-g)[R+12-14F^MNF_MN+c_1R_MNKLR^MNKL+c_2 R^MNKL F_MNF_KL], this action is a special case to the action considered in [ref] , but for our purpose this is good enough.

    Holographic Hydrodynamics with a Chemical Potential · A gravitational system · 0.86

Uses the method or tool of 5 papers
  • The coefficient of shear viscosity can be very easily computed using the prescription given in [ref] and the result is same as in [ref] η=r^3_02κ^2(1-24 c_1 q^2r^6_0) and the entropy density in terms of $q/r^3_0$, can be calculated using the Wald's entropy formula [ref] s=4πr^3_02κ^2[1+8 c_1-q^2r^6_0(28 c_1+24 c_2)]

    Universality of the hydrodynamic limit in AdS/CFT and the membrane paradigm · shear viscosity and $η/s$ · 0.91

  • The coefficient of shear viscosity can be very easily computed using the prescription given in [ref] and the result is same as in [ref] η=r^3_02κ^2(1-24 c_1 q^2r^6_0) and the entropy density in terms of $q/r^3_0$, can be calculated using the Wald's entropy formula [ref] s=4πr^3_02κ^2[1+8 c_1-q^2r^6_0(28 c_1+24 c_2)]

    Holographic Hydrodynamics with a Chemical Potential · shear viscosity and $η/s$ · 0.91

  • The coefficient of shear viscosity can be very easily computed using the prescription given in [ref] and the result is same as in [ref] η=r^3_02κ^2(1-24 c_1 q^2r^6_0) and the entropy density in terms of $q/r^3_0$, can be calculated using the Wald's entropy formula [ref] s=4πr^3_02κ^2[1+8 c_1-q^2r^6_0(28 c_1+24 c_2)]

    Black Hole Entropy is Noether Charge · shear viscosity and $η/s$ · 0.91

Compares with 1 paper
Cites as background 4 papers

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