Density Dependent Hyperonic Interactions in Neutron Stars

Influence of density dependent hyperon–nucleon forces on characteristics of neutron stars is investigated. In particular, the role of the exponent γ, determining the dependence of interaction on the nucleon density, in the description of the matter of neutron stars is studied. It is also shown that the hyperon–nucleon forces proportional to the nucleon density and three-body hyperon–nucleon–nucleon forces can lead to qualitatively different results in neutron stars.

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Publication Details

Journal
Bulletin of the Russian Academy of Sciences Physics
Published
2025-12-01
DOI
https://doi.org/10.1134/s1062873825714801
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
0.00
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article

Density Dependent Hyperonic Interactions in Neutron Stars

T. Yu. Tretyakova, A. I. Nasakin, S. A. Mikheev, D. E. Lanskoy et al.
Bulletin of the Russian Academy of Sciences Physics
Pulsars and Gravitational Waves Research
article

Density Dependent Hyperonic Interactions in Neutron Stars

T. Yu. Tretyakova, A. I. Nasakin, S. A. Mikheev, D. E. Lanskoy, S. V. Sidorov
article en

Abstract

Influence of density dependent hyperon–nucleon forces on characteristics of neutron stars is investigated. In particular, the role of the exponent γ, determining the dependence of interaction on the nucleon density, in the description of the matter of neutron stars is studied. It is also shown that the hyperon–nucleon forces proportional to the nucleon density and three-body hyperon–nucleon–nucleon forces can lead to qualitatively different results in neutron stars.

Bulletin of the Russian Academy of Sciences PhysicsVol. 89(S3)
Lomonosov Moscow State University (RU)
Openalex Percentile: Top 25%
Pulsars and Gravitational Waves Research
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