208 citations · 1.4k across the 21 of their papers we have counts for
21 papers
Thermal Fluctuations in Nuclear Pasta
M. E. Caplan, C. R. Forsman, A. S. Schneider
Despite their astrophysical relevance, nuclear pasta phases are relatively unstudied at high temperatures. We present molecular dynamics simulations of symmetric nuclear matter wit…
Equation of State and Progenitor Dependence of Stellar-Mass Black-Hole Formation
A. S. Schneider, E. O'Connor, E. Granqvist +2
The core collapse of a massive star results in the formation of a proto-neutron star (PNS). If enough material is accreted onto a PNS it will become gravitationally unstable and fu…
Equation of state effects in the core collapse of a - star
A. S. Schneider, L. F. Roberts, C. D. Ott +1
Uncertainties in our knowledge of the properties of dense matter near and above nuclear saturation density are among the main sources of variations in multi-messenger signatures pr…
The APR equation of state for simulations of supernovae, neutron stars and binary mergers
A. S. Schneider, C. Constantinou, B. Muccioli +1
Differences in the equation of state (EOS) of dense matter translate into differences in astrophysical simulations and their multi-messenger signatures. Thus, extending the number…
The Elasticity of Nuclear Pasta
M. E. Caplan, A. S. Schneider, C. J. Horowitz
The elastic properties of neutron star crusts are relevant for a variety of currently observable or near-future electromagnetic and gravitational wave phenomena. These phenomena ma…
Domains and defects in nuclear "pasta"
Andre da Silva Schneider, Matt E. Caplan, Don K. Berry +1
Nuclear pasta topology is an essential ingredient to determine transport properties in the inner crust of neutron stars. We perform semi-classical molecular dynamics simulations of…