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Bayesian Inferences of Neutron Stars' Properties: When Astro and Nuclear physics go hand in hand
Gabriele Montefusco
17/09/2025 11:30
Understanding the equation of state (EoS) of dense matter is crucial in simulations of neutron star structure and dynamics, as well as for the interpretation of astrophysical data. In particular, the EoS of cold neutron stars defines their stationary structure, from their masses and radii to their tidal deformabilities and the oscillation spectra of their normal modes. However, a...