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Record W2981844146 · doi:10.1103/physrevd.101.063007

Nonparametric inference of neutron star composition, equation of state, and maximum mass with GW170817

2020· article· en· W2981844146 on OpenAlexfundno aff
R. C. Essick, Philippe Landry, D. E. Holz

Bibliographic record

VenuePhysical review. D/Physical review. D. · 2020
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPulsars and Gravitational Waves Research
Canadian institutionsnot available
FundersNatural Sciences and Engineering Research Council of CanadaKavli FoundationKavli Institute for Theoretical Physics, University of California, Santa BarbaraUniversity of ChicagoNational Science Foundation
KeywordsNeutron starStar (game theory)InferenceEquation of stateNonparametric statisticsComposition (language)PhysicsAstrophysicsApplied mathematicsMathematicsStatistical physicsEconometricsComputer scienceThermodynamicsArtificial intelligence

Abstract

fetched live from OpenAlex

The detection of GW170817 in gravitational waves provides unprecedented constraints on the equation of state (EOS) of the ultradense matter within the cores of neutron stars (NSs). We extend the nonparametric analysis first introduced by Landry and Essick (2019), and confirm that GW170817 favors soft EOSs. We infer macroscopic observables for a canonical $1.4\text{ }\text{ }{M}_{\ensuremath{\bigodot}}$ NS, including the tidal deformability ${\mathrm{\ensuremath{\Lambda}}}_{1.4}={211}_{\ensuremath{-}137}^{+312}$ $({491}_{\ensuremath{-}181}^{+216})$ and radius ${R}_{1.4}=10.8{6}_{\ensuremath{-}1.42}^{+2.04}$ $({12.51}_{\ensuremath{-}0.88}^{+1.00})\text{ }\mathrm{km}$, as well as the maximum mass for nonrotating NSs ${M}_{\mathrm{max}}=2.06{4}_{\ensuremath{-}0.134}^{+0.260}$ $({2.017}_{\ensuremath{-}0.087}^{+0.238})\text{ }{M}_{\ensuremath{\bigodot}}$, with nonparametric priors loosely (tightly) constrained to resemble candidate EOSs from the literature. Furthermore, we find weak evidence that GW170817 involved at least one NS based on gravitational-wave data alone (${B}_{\mathrm{BBH}}^{\mathrm{NS}}=3.3\ifmmode\pm\else\textpm\fi{}1.4$), consistent with the observation of electromagnetic counterparts. We also investigate GW170817's implications for the maximum spin frequency of millisecond pulsars, and find that the fastest known pulsar is spinning at more than 50% of its breakup frequency at 90% confidence. We additionally find modest evidence in favor of quark matter within NSs, and GW170817 favors the presence of at least one disconnected hybrid star branch in the mass-radius relation over a single stable branch by a factor of 2. Assuming there are multiple stable branches, we find a suggestive posterior preference for a sharp softening around nuclear density followed by stiffening around twice nuclear density, consistent with a strong first-order phase transition. While the statistical evidence in favor of new physics within NS cores remains tenuous with GW170817 alone, these tantalizing hints reemphasize the promise of gravitational waves for constraining the supranuclear EOS.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Theoretical or conceptual · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.556
Threshold uncertainty score0.961

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0010.000
Bibliometrics0.0000.001
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.024
GPT teacher head0.434
Teacher spread0.410 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one teacher head, not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designTheoretical or conceptual
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations198
Published2020
Admission routes1
Has abstractyes

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