45 citations · 116 across the 6 of their papers we have counts for
6 papers
Generalized density functional equation of state for astrophysical simulations with 3-body forces and quark gluon plasma
J. Pocahontas Olson, MacKenzie Warren, Matthew Meixner +3
We present an updated general purpose nuclear equation of state (EoS) for use in simulations of core-collapse supernovae, neutron star mergers and black hole collapse. This EoS is…
Impact of sterile neutrino dark matter on core-collapse supernovae
MacKenzie L. Warren, Grant J. Mathews, Matthew Meixner +2
We summarize the impact of sterile neutrino dark matter on core-collapse supernova explosions. We explore various oscillations between electron neutrinos or mixed neutrinos a…
Sterile neutrino oscillations in core-collapse supernovae
MacKenzie L. Warren, Matthew Meixner, Grant Mathews +2
We have made core-collapse supernova simulations that allow oscillations between electron neutrinos (or their anti particles) with right-handed sterile neutrinos. We have considere…
The NDL Equation of State for Supernova Simulations
Matthew Meixner, J. Pocahontas Olson, Grant Mathews +2
We present an updated and improved equation of state (which we call the NDL EoS) for use in neutron-star structure and supernova simulations. This EoS is based upon a framework ori…
Updates of the nuclear equation of state for core-collapse supernovae and neutron Stars: effects of 3-body forces, QCD, and magnetic fields
G J Mathews, M Meixner, J P Olson +7
We summarize several new developments in the nuclear equation of state for supernova simulations and neutron stars. We discuss an updated and improved Notre-Dame-Livermore Equation…
Ultra-Dense Neutron Star Matter, Strange Quark Stars, and the Nuclear Equation of State
Fridolin Weber, Matthew Meixner, Rodrigo P. Negreiros +1
With central densities way above the density of atomic nuclei, neutron stars contain matter in one of the densest forms found in the universe. Depending of the density reached in t…