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Skyrme-Like Λ Hyperonic Interactions and Neutron Stars Properties

  • PHYSICS OF ELEMENTARY PARTICLES AND ATOMIC NUCLEI. THEORY
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Abstract

At high densities that are achieved in neutron stars, there may be additional sensitivity to certain properties of the baryonic interaction. In the present work, we consider neutron stars consisting of nucleons, leptons, and Λ-hyperons with Skyrme baryonic force. We calculate different characteristics of neutron stars such as mass, radius and tidal deformability and investigate their dependence on the properties of the interactions.

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Funding

This research has been supported by the Interdisciplinary Scientific and Educational School of Moscow University “Fundamental and Applied Space Research”. S.A. Mikheev thanks Theoretical Physics and Mathematics Advancement Foundation “BASIS” for support.

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Correspondence to S. A. Mikheev or T. Yu. Tretyakova.

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The authors declare that they have no conflicts of interest.

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Lanskoy, D.E., Mikheev, S.A., Nasakin, A.I. et al. Skyrme-Like Λ Hyperonic Interactions and Neutron Stars Properties. Phys. Part. Nuclei Lett. 20, 1488–1491 (2023). https://doi.org/10.1134/S1547477123060225

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  • DOI: https://doi.org/10.1134/S1547477123060225

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