Equations of state for supernovae and compact stars
M Oertel, M Hempel, T Klähn, S Typel - Reviews of Modern Physics, 2017 - APS
A review is given of various theoretical approaches for the equation of state (EoS) of dense
matter, relevant for the description of core-collapse supernovae, compact stars, and compact …
matter, relevant for the description of core-collapse supernovae, compact stars, and compact …
Nuclear equation of state from ground and collective excited state properties of nuclei
This contribution reviews the present status on the available constraints to the nuclear
equation of state (EoS) around saturation density from nuclear structure calculations on …
equation of state (EoS) around saturation density from nuclear structure calculations on …
Unified equations of state for cold non-accreting neutron stars with Brussels–Montreal functionals–I. Role of symmetry energy
JM Pearson, N Chamel, AY Potekhin… - Monthly Notices of …, 2018 - academic.oup.com
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 …
thermodynamically consistent treatment of all regions of cold non-accreting neutron stars. In …
r-process nucleosynthesis: connecting rare-isotope beam facilities with the cosmos
This is an exciting time for the study of r-process nucleosynthesis. Recently, a neutron star
merger GW170817 was observed in extraordinary detail with gravitational waves and …
merger GW170817 was observed in extraordinary detail with gravitational waves and …
Nuclear mass predictions for the crustal composition of neutron stars: A Bayesian neural network approach
Background: Besides their intrinsic nuclear-structure value, nuclear mass models are
essential for astrophysical applications, such as r-process nucleosynthesis and neutron-star …
essential for astrophysical applications, such as r-process nucleosynthesis and neutron-star …
[HTML][HTML] The neutron-rich edge of the nuclear landscape: Experiment and theory.
In this review, we describe the experimental facilities and methods which make it possible to
produce and measure the properties of the extreme neutron-rich nuclei. We then develop …
produce and measure the properties of the extreme neutron-rich nuclei. We then develop …
Masses of exotic nuclei
T Yamaguchi, H Koura, YA Litvinov, M Wang - Progress in Particle and …, 2021 - Elsevier
Recent developments in precision mass spectrometry of radioactive isotopes (RI) and some
selected related physics subjects are reviewed. In the last decades, besides conventional …
selected related physics subjects are reviewed. In the last decades, besides conventional …
Warming nuclear pasta with dark matter: kinetic and annihilation heating of neutron star crusts
Neutron stars serve as excellent next-generation thermal detectors of dark matter, heated by
the scattering and annihilation of dark matter accelerated to relativistic speeds in their deep …
the scattering and annihilation of dark matter accelerated to relativistic speeds in their deep …
Shape Coexistence in as the Portal to the Fifth Island of Inversion
Large-scale shell-model calculations predict that the region of deformation which comprises
the heaviest chromium and iron isotopes at and beyond N= 40 will merge with a new one at …
the heaviest chromium and iron isotopes at and beyond N= 40 will merge with a new one at …
Unified equation of state for neutron stars on a microscopic basis
BK Sharma, M Centelles, X Viñas, M Baldo… - Astronomy & …, 2015 - aanda.org
We derive a new equation of state (EoS) for neutron stars (NS) from the outer crust to the
core based on modern microscopic calculations using the Argonne v 18 potential plus three …
core based on modern microscopic calculations using the Argonne v 18 potential plus three …