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arXiv · 1908.05114

Density-dependent van der Waals model under the GW170817 constraint

O. Lourenço·M. Dutra·C. H. Lenzi·M. Bhuyan·S. K. Biswal·B. M. Santos
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Abstract

We propose a density-dependent function for the attractive interaction in the original van der Waals model to correctly describe the flow constraint at the high-density regime of the symmetric nuclear matter. After a generalization to asymmetric nuclear matter, it was also possible to study the stellar matter regime from this new model. The mass-radius relation for neutron stars under $\beta$-equilibrium is found to agree with recent X-ray observations. The neutron star masses supported against gravity, obtained from some parametrizations of the model, are in the range of $(1.97-2.07)M_{\odot}$, compatible with observational data from the PSR J0348+0432 pulsar. Furthermore, we verify the reliability of the model in predicting tidal deformabilities of the binary system related to the GW170817 neutron star merger event and find a full agreement with the new bounds obtained by the LIGO/Virgo collaboration.

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O. Lourenço, M. Dutra, C. H. Lenzi, M. Bhuyan, S. K. Biswal, B. M. Santos. 2019-08-14. Density-dependent van der Waals model under the GW170817 constraint. https://doi.org/10.3847/1538-4357/ab3122

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