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Cited by 378

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Constraints on Neutron Star Radii Based on Chiral Effective Field Theory Interactions

Open access
Hebeler, K., Lattimer, J. M., Pethick, C. J., Schwenk, A.·2010·Physical Review Letters

Abstract

We show that microscopic calculations based on chiral effective field theory interactions constrain the properties of neutron-rich matter below nuclear densities to a much higher degree than is reflected in commonly used equations of state. Combined with observed neutron star masses, our results lead to a radius R=9.7-13.9 km for a 1.4M⊙ star, where the theoretical range is due, in about equal amounts, to uncertainties in many-body forces and to the extrapolation to high densities.

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Metadata

Authors
Hebeler, K., Lattimer, J. M., Pethick, C. J., & Schwenk, A.
Venue
Physical Review Letters
Published
2010-10-13
Volume
105
Issue
16
Pages
161102-161102
ISSN
  • 0031-9007 (ISSN-L)
  • 1079-7114
OpenAlex
W2084001590
Cited by
378
References
1
FWCI
15.32
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Constraints on Neutron Star Radii Based on Chiral Effective Field Theory Interactions. https://app.cochat.ai/papers/10.1103/physrevlett.105.161102
The paper
Hebeler, K., Lattimer, J. M., Pethick, C. J., & Schwenk, A. (2010). Constraints on Neutron Star Radii Based on Chiral Effective Field Theory Interactions. Physical Review Letters. https://doi.org/10.1103/physrevlett.105.161102

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Bibliographic data: Semantic Scholar, OpenAlex, Crossref.

Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.