Nuclear equation of state for compact stars and supernovae
G Fiorella Burgio, AF Fantina - The Physics and Astrophysics of Neutron …, 2018 - Springer
The equation of state (EoS) of hot and dense matter is a fundamental input to describe static
and dynamical properties of neutron stars, core-collapse supernovae and binary compact …
and dynamical properties of neutron stars, core-collapse supernovae and binary compact …
Nuclear Equation of state for Compact Stars and Supernovae
GF Burgio, AF Fantina - arXiv preprint arXiv:1804.03020, 2018 - arxiv.org
The equation of state (EoS) of hot and dense matter is a fundamental input to describe static
and dynamical properties of neutron stars, core-collapse supernovae and binary compact …
and dynamical properties of neutron stars, core-collapse supernovae and binary compact …
Nuclear Equation of State for Compact Stars and Supernovae
GF Burgio, AF Fantina - The Physics and Astrophysics of Neutron Stars, 2018 - Springer
The equation of state (EoS) of hot and dense matter is a fundamental input to describe static
and dynamical properties of neutron stars, core-collapse supernovae and binary compact …
and dynamical properties of neutron stars, core-collapse supernovae and binary compact …
[引用][C] Nuclear Equation of State for Compact Stars and Supernovae
GF Burgio, AF Fantina - The Physics and Astrophysics of Neutron Stars, 2018 - cir.nii.ac.jp
Nuclear Equation of State for Compact Stars and Supernovae | CiNii Research CiNii 国立情報学
研究所 学術情報ナビゲータ[サイニィ] 詳細へ移動 検索フォームへ移動 論文・データをさがす 大学 …
研究所 学術情報ナビゲータ[サイニィ] 詳細へ移動 検索フォームへ移動 論文・データをさがす 大学 …
Nuclear Equation of state for Compact Stars and Supernovae
GF Burgio, AF Fantina - The Physics and Astrophysics of Neutron Stars, 2018 - hal.science
The equation of state (EoS) of hot and dense matter is a fundamental input to describe static
and dynamical properties of neutron stars, core-collapse supernovae and binary compact …
and dynamical properties of neutron stars, core-collapse supernovae and binary compact …
Nuclear Equation of State for Compact Stars and Supernovae
G Fiorella Burgio, AF Fantina - Astrophysics and Space …, 2018 - ui.adsabs.harvard.edu
The equation of state (EoS) of hot and dense matter is a fundamental input to describe static
and dynamical properties of neutron stars, core-collapse supernovae and binary compact …
and dynamical properties of neutron stars, core-collapse supernovae and binary compact …
Nuclear Equation of State for Compact Stars and Supernovae
GF Burgio, AF Fantina - The Physics and Astrophysics of Neutron …, 2019 - books.google.com
The equation of state (EoS) of hot and dense matter is a fundamental input to describe static
and dynamical properties of neutron stars, core-collapse supernovae and binary compact …
and dynamical properties of neutron stars, core-collapse supernovae and binary compact …
[PDF][PDF] Nuclear Equation of State for Compact Stars and Supernovae
GF Burgio, AF Fantina - The Physics and Astrophysics of …, 2018 - ndl.ethernet.edu.et
The equation of state (EoS) of hot and dense matter is a fundamental input to describe static
and dynamical properties of neutron stars, core-collapse supernovae and binary compact …
and dynamical properties of neutron stars, core-collapse supernovae and binary compact …
Nuclear Equation of state for Compact Stars and Supernovae
G Fiorella Burgio, AF Fantina - Astrophys. Space Sci. Libr., 2018 - inspirehep.net
The equation of state (EoS) of hot and dense matter is a fundamental input to describe static
and dynamical properties of neutron stars, core-collapse supernovae and binary compact …
and dynamical properties of neutron stars, core-collapse supernovae and binary compact …