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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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