335 citations · 1.7k across the 32 of their papers we have counts for
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Polytropic fits of modern and unified equations of state
Lami Suleiman, Morgane Fortin, Julian-Leszek Zdunik +1
Equations of state for a cold neutron star's interior are presented in three-column tables that relate the baryonic density, the energy density, and the pressure. A few analytical…
Thermal evolution of relativistic hyperonic compact stars with calibrated equations of state
Morgane Fortin, Adriana R. Raduta, Sidney Avancini +1
A set of unified relativistic mean-field equations of state for hyperonic compact stars recently built in [M. Fortin, Ad. R. Raduta, S. Avancini, and C. Providencia, Phys. Rev. D {…
Empirical constraints on the high-density equation of state from multi-messenger observables
Márcio Ferreira, M. Fortin, Tuhin Malik +2
We search for possible correlations between neutron star observables and thermodynamic quantities that characterize high density nuclear matter. We generate a set of model-independ…
GW170817: constraining the nuclear matter equation of state from the neutron star tidal deformability
Tuhin Malik, N. Alam, M. Fortin +5
Constraints set on key parameters of the nuclear matter equation of state (EoS) by the values of the tidal deformability, inferred from GW170817, are examined by using a diverse se…
(No) neutron star maximum mass constraint from hypernuclei
M. Fortin, S. S. Avancini, C. Providência +1
(Abridged) The recent measurement of the mass of two pulsars has raised the question whether such large masses allow for the existence of exotic degrees of freedom, s…
Strong correlations of neutron star radii with the slopes of nuclear matter incompressibility and symmetry energy at saturation
N. Alam, B. K. Agrawal, M. Fortin +4
We examine the correlations of neutron star radii with the nuclear matter incompressibility, symmetry energy, and their slopes, which are the key parameters of the equation of stat…
Thermalisation time and specific heat of neutron stars crust
M. Fortin, F. Grill, J. Margueron +1
We discuss the thermalisation process of the neutron stars crust described by solving the heat transport equation with a microscopic input for the specific heat of baryonic matter.…