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From the crust to the core of Neutron Stars on a microscopic basis

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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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M. Baldo, G. F. Burgio, M. Centelles, B. K. Sharma, X. Viñas

Nuclear Theory · Submitted 10 Aug 2013

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

The authors' main claim The relevance of the crust Equation of state for the Neutron Star radius is particularly emphasised.

how it is stated · asserted 0.92 read the record →

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arXiv ID1308.2304 (version 2)
Pith IDWKW5INKJ, Pith's permanent record of this paper and its review
CitationB. K. Sharma, G. F. Burgio, M. Baldo, M. Centelles, X. Vi\~nas. "From the crust to the core of Neutron Stars on a microscopic basis." arXiv:1308.2304 (2013). https://pith.science/paper/WKW5INKJ
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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, 3,673 input tokens, $0.0002 reported.

What the abstract itself states, as probabilities: claims first 0.95 · states limitation 0.09 · human participants 0.01 · controlled comparison 0.14 · randomized assignment 0.01 · states quantitative result 0.06 · compares with prior results 0.92 · mentions code or data availability 0.02.

The abstract, sentence by sentence

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

Within a microscopic approach the structure of Neutron Stars is usually studied by modelling the homogeneous nuclear matter of the core by a suitable Equation of State, based on a many-body theory, and the crust by a functional based on a more phenomenological approach. We present the first calculation of Neutron Star overall structure by adopting for the core an Equation of State derived from the Brueckner-Hartree-Fock theory and for the crust, including the pasta phase, an Energy Density Functional based on the same Equation of State, and which is able to describe accurately the binding energy of nuclei throughout the mass table. Comparison with other approaches is discussed. The relevance of the crust Equation of state for the Neutron Star radius is particularly emphasised.

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 Within a microscopic approach the structure of Neutron Stars is usually studied by modelling the homogeneous nuclear matter of the core by a suitable Equation of State, based on a many-body theory, and the crust by a functional based on a more phenomenological approach. background 1.00 0.04 0.03 asserted 0.99
s1 We present the first calculation of Neutron Star overall structure by adopting for the core an Equation of State derived from the Brueckner-Hartree-Fock theory and for the crust, including the pasta phase, an Energy Density Functional based on the same Equation of State, and which is able to describe accurately the binding energy of nuclei throughout the mass table. contribution 0.98 0.96 0.32 asserted 1.00
s2 Comparison with other approaches is discussed. contribution 0.48 0.40 0.03 unclear 0.83
s3 The relevance of the crust Equation of state for the Neutron Star radius is particularly emphasised. interpretation 0.92 0.54 0.44 asserted 0.92

What kind of paper the classifier reports this is: theoretical result 0.47 · evidence from simulation or computation 1.00.

What was examined, and what was not

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  • full text
  • figures and tables
  • references and citing sentences
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  • 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

Within a microscopic approach the structure of Neutron Stars is usually studied by modelling the homogeneous nuclear matter of the core by a suitable Equation of State, based on a many-body theory, and the crust by a functional based on a more phenomenological approach. We present the first calculation of Neutron Star overall structure by adopting for the core an Equation of State derived from the Brueckner-Hartree-Fock theory and for the crust, including the pasta phase, an Energy Density Functional based on the same Equation of State, and which is able to describe accurately the binding energy of nuclei throughout the mass table. Comparison with other approaches is discussed. The relevance of the crust Equation of state for the Neutron Star radius is particularly emphasised.

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References
How the literature uses it

2 arXiv papers cite this in 2 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

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