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Equation of state for dense nucleon matter

Wiringa, R. B., Fiks, V., Fabrocini, A.·1988·Physical Review C
DOI 10.1103/physrevc.38.1010
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Abstract

We report microscopic calculations of the equation of state for dense nuclear and neutron matter. The calculations are performed for five Hamiltonians: the Argonne ${v}_{14}$ and Urbana ${v}_{14}$ two-nucleon potentials, both alone and with the Urbana VII three-nucleon potential, and the density-dependent Urbana ${v}_{14}$ plus three-nucleon interaction model of Lagaris, Friedman, and Pandharipande. The beta-stable equation of state and neutron star structure are also calculated for three of the models. The models with the three-nucleon potential bracket the density-dependent model and are significantly stiffer than those with an unmodified two-nucleon potential only. The Argonne ${v}_{14}$ plus Urbana VII Hamiltonian produces a softening in the neutron matter equation of state localized around twice nuclear matter density which may indicate a neutral pion condensate.

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Metadata

Authors
Wiringa, R. B., Fiks, V., & Fabrocini, A.
Venue
Physical Review C
Publisher
American Physical Society (APS)
Published
1988-08-01
Volume
38
Issue
2
Pages
1010-1037
ISSN
0556-2813 (ISSN-L)
DOI
10.1103/physrevc.38.1010
OpenAlex
W2057910081
Cited by
1,001
References
0
FWCI
4.98
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Equation of state for dense nucleon matter. https://app.cochat.ai/papers/10.1103/physrevc.38.1010
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Wiringa, R. B., Fiks, V., & Fabrocini, A. (1988). Equation of state for dense nucleon matter. Physical Review C. https://doi.org/10.1103/physrevc.38.1010

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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.