Pith. Sign in

RECORD

The Thermal Response of a Pulsar Glitch : The Non-spherical Symmetric Case

PaperPDF from arXiv

data files

Paper breakdownThe authors' claims, conditions and measurements, as JSON Signed receiptProof this review has not been altered
X Bluesky LinkedIn Reddit Hacker News
K.S. Cheng, Y.Li, W.-M. Suen

General Relativity and Quantum Cosmology · Submitted 8 Mar 1999

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

The authors' main claim Even for young pulsars with a hot core like the Vela pulsar, we find that a detectable hot spot can be observed after a glitch.

how it is stated · asserted 0.99 read the record →

Comment (0) Read on arXiv ↗
Cite ▾
arXiv IDgr-qc/9903033 (version 1)
Pith IDDHBDOYLJ, Pith's permanent record of this paper and its review
CitationK.S. Cheng, W.-M. Suen, Y.Li. "The Thermal Response of a Pulsar Glitch : The Non-spherical Symmetric Case." arXiv:gr-qc/9903033 (1999). https://pith.science/paper/DHBDOYLJ
Claim paper

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.

Open the compiled record

Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 4,812 input tokens, $0.0002 reported.

What the abstract itself states, as probabilities: claims first 0.04 · states limitation 0.13 · human participants 0.01 · controlled comparison 0.42 · randomized assignment 0.01 · states quantitative result 0.06 · compares with prior results 0.93 · mentions code or data availability 0.02.

The abstract, sentence by sentence

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

We study the thermal evolution of a pulsar after a glitch in which the energy is released from a relative compact region. A set of relativistic thermal transport and energy balance equations is used to study the thermal evolution, without making the assumption of spherical symmetry. We use an exact cooling model to solve this set of differential equtions. Our results differ significantly from those obtained under the assumption of spherical symmetry. Even for young pulsars with a hot core like the Vela pulsar, we find that a detectable hot spot can be observed after a glitch. The results suggest that the intensity variation and the relative phases of hard X-ray emissions in different epoches can provide important information on the equation of state.

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 study the thermal evolution of a pulsar after a glitch in which the energy is released from a relative compact region. contribution 0.81 0.73 0.04 asserted 0.90
s1 A set of relativistic thermal transport and energy balance equations is used to study the thermal evolution, without making the assumption of spherical symmetry. method 0.98 0.88 0.05 asserted 0.98
s2 We use an exact cooling model to solve this set of differential equtions. method 1.00 0.91 0.04 asserted 1.00
s3 Our results differ significantly from those obtained under the assumption of spherical symmetry. result 0.98 0.83 0.34 asserted 1.00
s4 Even for young pulsars with a hot core like the Vela pulsar, we find that a detectable hot spot can be observed after a glitch. result 1.00 0.95 0.32 asserted 0.99
s5 The results suggest that the intensity variation and the relative phases of hard X-ray emissions in different epoches can provide important information on the equation of state. interpretation 1.00 0.57 0.30 hedged possibility 1.00

What kind of paper the classifier reports this is: simulation study 0.65 · evidence from simulation or computation 0.79.

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

We study the thermal evolution of a pulsar after a glitch in which the energy is released from a relative compact region. A set of relativistic thermal transport and energy balance equations is used to study the thermal evolution, without making the assumption of spherical symmetry. We use an exact cooling model to solve this set of differential equtions. Our results differ significantly from those obtained under the assumption of spherical symmetry. Even for young pulsars with a hot core like the Vela pulsar, we find that a detectable hot spot can be observed after a glitch. The results suggest that the intensity variation and the relative phases of hard X-ray emissions in different epoches can provide important information on the equation of state.

Human review

How Pith checks papers → · Full audit of this paper →

Discussion

Know something about this paper? Leave a comment, or highlight any passage above to comment on it.