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Large Distance Modification of Newtonian Potential and Structure Formation in Universe

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Paper breakdownThe authors' claims, conditions and measurements, as JSON Signed receiptProof this review has not been altered
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Mir Hameeda, Sudhaker Upadhyay, Mir Faizal, Ahmed F. Ali, Behnam Pourhassan

General Relativity and Quantum Cosmology · Submitted 21 Dec 2017

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

The authors' main claim We observe that such corrections also modify the virial theorem for such a system of galaxies.

how it is stated · asserted 0.99 read the record →

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arXiv ID1712.08591 (version 1)
Pith ID6NXCIVNJ, Pith's permanent record of this paper and its review
CitationAhmed F. Ali, Behnam Pourhassan, Mir Faizal, Mir Hameeda, Sudhaker Upadhyay. "Large Distance Modification of Newtonian Potential and Structure Formation in Universe." arXiv:1712.08591 (2017). https://pith.science/paper/6NXCIVNJ
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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.

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Compiled by classifier-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-09-23: 1 request, 4,129 input tokens.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.47 · human participants 0.01 · controlled comparison 0.08 · randomized assignment 0.01 · states quantitative result 0.05 · 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 the effects of super-light brane world perturbative modes on structure formation in our universe. As these modes modify the large distance behavior of Newtonian potential, they effect the clustering of a system of galaxies. So, we explicitly calculate the clustering of galaxies interacting through such a modified Newtonian potential. We use a suitable approximation for analyzing this system of galaxies, and discuss the validity of such approximations. We observe that such corrections also modify the virial theorem for such a system of galaxies.

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 the effects of super-light brane world perturbative modes on structure formation in our universe. contribution 0.99 0.87 0.06 asserted 0.74
s1 As these modes modify the large distance behavior of Newtonian potential, they effect the clustering of a system of galaxies. background 0.75 0.17 0.12 asserted 0.99
s2 So, we explicitly calculate the clustering of galaxies interacting through such a modified Newtonian potential. contribution 0.79 0.95 0.09 asserted 0.99
s3 We use a suitable approximation for analyzing this system of galaxies, and discuss the validity of such approximations. method 0.98 0.88 0.03 asserted 0.88
s4 We observe that such corrections also modify the virial theorem for such a system of galaxies. result 0.99 0.92 0.25 asserted 0.99

What kind of paper the classifier reports this is: theoretical result 1.00 · evidence from proof or derivation 0.99.

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
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  • 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

In this paper, we study the effects of super-light brane world perturbative modes on structure formation in our universe. As these modes modify the large distance behavior of Newtonian potential, they effect the clustering of a system of galaxies. So, we explicitly calculate the clustering of galaxies interacting through such a modified Newtonian potential. We use a suitable approximation for analyzing this system of galaxies, and discuss the validity of such approximations. We observe that such corrections also modify the virial theorem for such a system of galaxies.

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References
How the literature uses it

3 arXiv papers cite this in 4 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 · 2 sentences without a confident label

Cites it as background 1 paper

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