JM Pearson, N Chamel, AY Potekhin, AF Fantina… - ioffe.ru
This is a correction notice for 'Unified equations of state for cold non-accreting neutron stars with Brussels-Montreal functionals. I. Role of symmetry energy'(DOI: https://doi …
JM Pearson, AF Fantina - Monthly Notices of the Royal Astronomical …, 2018 - inis.iaea.org
[en] The theory of the nuclear energy-density functional is used to provide a unified and thermodynamically consistent treatment of all regions of cold non-accreting neutron stars. In …
JM Pearson, N Chamel, AY Potekhin… - Monthly Notices of …, 2019 - academic.oup.com
This is a correction notice for 'Unified equations of state for cold non-accreting neutron stars with Brussels-Montreal functionals. I. Role of symmetry energy'(DOI: https://doi …
JM Pearson, N Chamel, AY Potekhin… - Mon. Not. Roy. Astron …, 2018 - inspirehep.net
The theory of the nuclear energy-density functional is used to provide a unified and thermodynamically consistent treatment of all regions of cold non-accreting neutron stars. In …
JM Pearson, N Chamel, AY Potekhin… - Monthly Notices of the …, 2019 - inria.hal.science
Erratum: Unified equations of state for cold non-accreting neutron stars with Brussels-Montreal functionals. I. Role of symmetry energy - Inria - Institut national de recherche en sciences et …
JM Pearson, N Chamel, AY Potekhin, AF Fantina… - ioffe.ru
The theory of the nuclear energy-density functional is used to provide a unified and thermodynamically consistent treatment of all regions of cold non-accreting neutron stars. In …
JM Pearson, N Chamel, AY Potekhin… - arXiv preprint arXiv …, 2019 - arxiv.org
The theory of the nuclear energy-density functional is used to provide a unified and thermodynamically consistent treatment of all regions of cold non-accreting neutron stars. In …
JM Pearson, N Chamel, AY Potekhin… - Monthly Notices of the …, 2018 - hal.science
The theory of the nuclear energy-density functional is used to provide a unified and thermodynamically consistent treatment of all regions of cold non-accreting neutron stars. In …