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Tolman-Bondi Space-Time in Brane World Scenario

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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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Subenoy Chakraborty, Asit Banerjee, Ujjal Debnath

General Relativity and Quantum Cosmology · Submitted 17 Feb 2006

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

The authors' main claim The first solution shows that the end state of collapse may be black hole or a naked singularity depending signs of various parameters involved.

how it is stated · hedged possibility 0.93 read the record →

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arXiv IDgr-qc/0602068 (version 1)
Pith ID44KJWQHL, Pith's permanent record of this paper and its review
CitationAsit Banerjee, Subenoy Chakraborty, Ujjal Debnath. "Tolman-Bondi Space-Time in Brane World Scenario." arXiv:gr-qc/0602068 (2006). https://pith.science/paper/44KJWQHL
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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-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 4,187 input tokens, $0.0002 reported.

What the abstract itself states, as probabilities: claims first 0.04 · states limitation 0.14 · human participants 0.01 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.05 · 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 the present work, inhomogeneous Tolman-Bondi type dust space-time is studied on the brane. There are two sets of solutions of the above model. The first solution represents either a collapsing model starting from an infinite volume at infinite past to the singularity or a model starting from a singularity and expanding for ever having a transition from decelerating phase to accelerating phase. The first solution shows that the end state of collapse may be black hole or a naked singularity depending signs of various parameters involved. The second solution represents a bouncing model where the bounce occurs at different comoving radii at different epochs.

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 the present work, inhomogeneous Tolman-Bondi type dust space-time is studied on the brane. contribution 0.99 0.89 0.04 asserted 0.96
s1 There are two sets of solutions of the above model. result 0.96 0.80 0.05 asserted 1.00
s2 The first solution represents either a collapsing model starting from an infinite volume at infinite past to the singularity or a model starting from a singularity and expanding for ever having a transition from decelerating phase to accelerating phase. result 1.00 0.83 0.25 asserted 0.90
s3 The first solution shows that the end state of collapse may be black hole or a naked singularity depending signs of various parameters involved. result 0.80 0.84 0.26 hedged possibility 0.93
s4 The second solution represents a bouncing model where the bounce occurs at different comoving radii at different epochs. result 1.00 0.86 0.14 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

In the present work, inhomogeneous Tolman-Bondi type dust space-time is studied on the brane. There are two sets of solutions of the above model. The first solution represents either a collapsing model starting from an infinite volume at infinite past to the singularity or a model starting from a singularity and expanding for ever having a transition from decelerating phase to accelerating phase. The first solution shows that the end state of collapse may be black hole or a naked singularity depending signs of various parameters involved. The second solution represents a bouncing model where the bounce occurs at different comoving radii at different epochs.

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