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Thomas-Fermi-Dirac model for Low Density Stellar Matter in Presence of a Strong Quantising Magnetic Field

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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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Nandini Nag, Somenath Chakrabarty

Astrophysics · Submitted 9 Dec 1999

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

The authors' main claim It is seen that the decay time scale for magnetic field decreases by at least two orders of magnitude in such model calculaion.

how it is stated · asserted 0.99 read the record →

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arXiv IDastro-ph/9912183 (version 1)
Pith IDCWQRL3BY, Pith's permanent record of this paper and its review
CitationNandini Nag, Somenath Chakrabarty. "Thomas-Fermi-Dirac model for Low Density Stellar Matter in Presence of a Strong Quantising Magnetic Field." arXiv:astro-ph/9912183 (1999). https://pith.science/paper/CWQRL3BY
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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, 3,505 input tokens, $0.0001 reported.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.10 · human participants 0.01 · controlled comparison 0.15 · randomized assignment 0.01 · states quantitative result 0.94 · compares with prior results 0.17 · mentions code or data availability 0.02.

The abstract, sentence by sentence

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

The effect of strong quantising magnetic field on low density stellar matter is investigated using Thomas-Fermi-Dirac (TFD) model. The Wigner-Seitz cell structure is assumed for the low density matter. The significant changes in the properties of such low density matter in presence of strong magnetic fields are discussed. It is seen that the decay time scale for magnetic field decreases by at least two orders of magnitude in such model calculaion.

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 The effect of strong quantising magnetic field on low density stellar matter is investigated using Thomas-Fermi-Dirac (TFD) model. contribution 0.80 0.87 0.06 asserted 0.98
s1 The Wigner-Seitz cell structure is assumed for the low density matter. method 1.00 0.42 0.02 asserted 0.98
s2 The significant changes in the properties of such low density matter in presence of strong magnetic fields are discussed. contribution 0.50 0.61 0.11 asserted 0.73
s3 It is seen that the decay time scale for magnetic field decreases by at least two orders of magnitude in such model calculaion. result 1.00 0.85 0.69 asserted 0.99

What kind of paper the classifier reports this is: theoretical result 0.89 · evidence from simulation or computation 0.67.

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

The effect of strong quantising magnetic field on low density stellar matter is investigated using Thomas-Fermi-Dirac (TFD) model. The Wigner-Seitz cell structure is assumed for the low density matter. The significant changes in the properties of such low density matter in presence of strong magnetic fields are discussed. It is seen that the decay time scale for magnetic field decreases by at least two orders of magnitude in such model calculaion.

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