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- W3200331393 abstract "A reported 17 MeV boson, which has been proposed as an explanation to the 8 Be and 4 He anomaly, is investigated in the context of its possible influence to neutron stars structure. Implementing a m X =17 MeV to the nuclear equation of state using different incompressibility values K 0 =245 MeV and K 0 =260 MeV and solving Tolman-Oppenheimer-Volkoff equations, we estimate an upper limit of M TOV ≈ 2.4 M ⊙ for a non rotating neutron star with span in radius R between 11.5 km to 14 km. Moving away from pure -NN with admixture of 10% protons and simulating possible softening of equation of state due to hyperons, we see that our estimated limits fit quite well inside the newest reported studies, coming from neutron stars merger event, GW190814" @default.
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- W3200331393 date "2021-01-01" @default.
- W3200331393 modified "2023-10-16" @default.
- W3200331393 title "Neutron star structure with nuclear force mediated by hypothetical X17 boson" @default.
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- W3200331393 doi "https://doi.org/10.1051/epjconf/202125204008" @default.
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