84 citations · 358 across the 20 of their papers we have counts for
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Accurate muonic interactions in neutron star mergers and impact on heavy-element nucleosynthesis
Harry Ho-Yin Ng, Carlo Musolino, Samuel D. Tootle +1
The abundances resulting from -process nucleosynthesis as predicted by simulations of binary neutron star (BNS) mergers remain an open question as the current state of the art i…
Exploring the Phase Diagram of V-QCD with Neutron Star Merger Simulations
Tuna Demircik, Christian Ecker, Matti Järvinen +3
Determining the phase structure of Quantum Chromodynamics (QCD) and its Equation of State (EOS) at densities and temperatures realized inside neutron stars and their mergers is a l…
Crustal magnetic fields do not lead to large magnetic-field amplifications in binary neutron-star mergers
Michail Chabanov, Samuel D. Tootle, Elias R. Most +1
The amplification of magnetic fields plays an important role in explaining numerous astrophysical phenomena associated with binary neutron-star mergers, such as mass ejection and t…
Quark formation and phenomenology in binary neutron-star mergers using V-QCD
Samuel Tootle, Christian Ecker, Konrad Topolski +3
Using full 3+1 dimensional general-relativistic hydrodynamic simulations of equal- and unequal-mass neutron-star binaries with properties that are consistent with those inferred fr…
Impact of extreme spins and mass ratios on the post-merger observables of high-mass binary neutron stars
L. Jens Papenfort, Elias R. Most, Samuel Tootle +1
The gravitational-wave events GW170817 and GW190425 have led to a number of important insights on the equation of state of dense matter and the properties of neutron stars, such as…
On accretion disks formed in MHD simulations of black hole-neutron star mergers with accurate microphysics
Elias R. Most, L. Jens Papenfort, Samuel D. Tootle +1
Remnant accretion disks formed in compact object mergers are an important ingredient in the understanding of electromagnetic afterglows of multi-messenger gravitational-wave events…
Fast ejecta as a potential way to distinguish black holes from neutron stars in high-mass gravitational-wave events
Elias R. Most, L. Jens Papenfort, Samuel Tootle +1
High-mass gravitational-wave events in the neutron-star mass range, such as GW190425, have recently started to be detected by the LIGO/Virgo detectors. If the masses of the two bin…