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 …
Explosion mechanisms of core-collapse supernovae
HT Janka - Annual Review of Nuclear and Particle Science, 2012 - annualreviews.org
Supernova theory, numerical and analytic, has made remarkable progress in the past
decade. This progress was made possible by more sophisticated simulation tools, especially …
decade. This progress was made possible by more sophisticated simulation tools, especially …
New neutron star equation of state with quark–hadron crossover
We present a much improved equation of state for neutron star matter, QHC19, with a
smooth crossover from the hadronic regime at lower densities to the quark regime at higher …
smooth crossover from the hadronic regime at lower densities to the quark regime at higher …
Detecting and reconstructing gravitational waves from the next galactic core-collapse supernova in the advanced detector era
We performed a detailed analysis of the detectability of a wide range of gravitational waves
derived from core-collapse supernova simulations using gravitational-wave detector noise …
derived from core-collapse supernova simulations using gravitational-wave detector noise …
[HTML][HTML] Nuclear equation of state for core-collapse supernova simulations with realistic nuclear forces
H Togashi, K Nakazato, Y Takehara, S Yamamuro… - Nuclear Physics A, 2017 - Elsevier
A new table of the nuclear equation of state (EOS) based on realistic nuclear potentials is
constructed for core-collapse supernova numerical simulations. Adopting the EOS of uniform …
constructed for core-collapse supernova numerical simulations. Adopting the EOS of uniform …
Maximal neutron star mass and the resolution of the hyperon puzzle in modified gravity
The so-called “hyperon puzzle” in the theory of neutron stars is considered in the framework
of modified f (R) gravity. We show that for simple hyperon equations of state, it is possible to …
of modified f (R) gravity. We show that for simple hyperon equations of state, it is possible to …
Neutron matter from chiral effective field theory interactions
The neutron-matter equation of state constrains the properties of many physical systems
over a wide density range and can be studied systematically using chiral effective field …
over a wide density range and can be studied systematically using chiral effective field …
New hyperon equations of state for supernovae and neutron stars in density-dependent hadron field theory
S Banik, M Hempel… - The Astrophysical Journal …, 2014 - iopscience.iop.org
We develop new hyperon equation of state (EoS) tables for core-collapse supernova
simulations and neutron stars. These EoS tables are based on a density-dependent …
simulations and neutron stars. These EoS tables are based on a density-dependent …
Unified treatment of subsaturation stellar matter at zero and finite temperature
F Gulminelli, AR Raduta - Physical Review C, 2015 - APS
The standard variational derivation of stellar-matter structure in the Wigner-Seitz
approximation is generalized to the finite-temperature situation where a wide distribution of …
approximation is generalized to the finite-temperature situation where a wide distribution of …
Hypernuclei and massive neutron stars
Background: The recent accurate measurement of the mass of two pulsars close to or above
2 M⊙ has raised the question of whether such large pulsar masses allow for the existence …
2 M⊙ has raised the question of whether such large pulsar masses allow for the existence …