Unified equations of state for cold non-accreting neutron stars with BrusselsMontreal functionals–I. Role of symmetry energy

JM Pearson, N Chamel, AY Potekhin… - Monthly Notices of …, 2018 - academic.oup.com
… to be valid in any neutron star that is not accreting from a … CCM picture is valid throughout
the star except in a thin layer … The unified treatment of all three regions of neutron stars that …

Neutron star properties with unified equations of state of dense matter

AF Fantina, N Chamel, JM Pearson… - Astronomy & astrophysics, 2013 - aanda.org
… of neutron stars (NSs), as predicted by the Brussels-Montreal … The interior of a NS is assumed
to be made of cold catalysed … here are mostly suitable for non-accreting NSs. For simplicity, …

Unified equation of state for neutron stars on a microscopic basis

BK Sharma, M Centelles, X Viñas, M Baldo… - Astronomy & …, 2015 - aanda.org
… More recently, unified EoSs for NS have been derived by the Brussels-Montreal group (Chamel
et al… This is a meaningful assumption for non-accreting neutron stars that have lived long …

Unified equation of state for neutron stars based on the gogny interaction

X Viñas, C Gonzalez-Boquera, M Centelles, C Mondal… - Symmetry, 2021 - mdpi.com
… to the BSk22 Skyrme force obtained by the BrusselsMontreal group and reported in Ref. […
of the outer crust of a cold, non-accreting star. These calculations are performed within the so-…

A modern view of the equation of state in nuclear and neutron star matter

GF Burgio, HJ Schulze, I Vidaña, JB Wei - Symmetry, 2021 - mdpi.com
… We also include three EOSs derived within the modern Brussels-Montreal family of unified
… matter are defined, one can calculate the composition and the EOS of cold, neutrino-free, …

Constraints on the equation of state of cold dense matter from nuclear physics and astrophysics

AF Fantina, N Chamel, JM Pearson… - EPJ Web of …, 2014 - epj-conferences.org
… ρ, is a crucial ingredient for the description of neutron stars (NSs). These stellar remnants of
… are well-suited for a unified description of all regions of a NS. For non-accreting NSs, it is a …

Unified equation of state for neutron stars and supernova cores using the nuclear energy-density functional theory

AF Fantina, N Chamel, JM Pearson… - Journal of Physics …, 2012 - iopscience.iop.org
… Conclusion We have presented three different unified EoSs of NS based on the EDF theory.
… the limiting case of cold catalyzed matter as relevant for cold non-accreting NS, our method …

Nuclear Pasta in Cold Non-Accreting Neutron Stars: Symmetry Energy Effects

NN Shchechilin, JM Pearson, N Chamel - Physical Sciences Forum, 2023 - mdpi.com
… in cold non-accreting neutron stars. For this purpose, we apply three BrusselsMontreal
data on nuclei and realistic neutron-matter equations of state. These functionals differ in their …

Crustal heating in accreting neutron stars from the nuclear energy-density functional theory-I. Proton shell effects and neutron-matter constraint

AF Fantina, JL Zdunik, N Chamel, JM Pearson… - Astronomy & …, 2018 - aanda.org
… of accurately calibrated BrusselsMontreal functionals BSk19… of a non-accreting (isolated)
NS is that it is made of “cold-… nuclear matter thus providing a unified description of all regions …

Unified description of dense matter in neutron stars and magnetars

N Chamel, RL Pavlov, LM Mihailov… - Proceedings of the …, 2012 - cambridge.org
… We have determined the internal structure a cold non-accreting NS endowed with a
strong magnetic field using a unified treatment of dense matter based on the nuclear energy-density …