6 papers
Consistent Treatment of Muons in Binary Neutron Star Mergers
Henrique Gieg, Ramon Jaeger, Maximiliano Ujevic +1
We present a set of numerical-relativity binary neutron star merger simulations incorporating muons and muonic reactions for two baseline baryonic equations-of-state. In order to i…
Estimation of the MTOV precision for ET, CE, and NEMO from the post-merger of BNS coalescences
Gabriela Conde-Saavedra, Odylio Denys Aguiar, Henrique P. de Oliveira +1
The detection of the gravitational waves produced after the coalescence of two neutron stars is greatly anticipated because it will be able to provide information about matter in e…
Simulating Binary Neutron Star Mergers with Finite-temperature Equations of State: The influences of the slope of the symmetry energy and artificial heating
Henrique Gieg, Maximiliano Ujevic, Armen Sedrakian +1
We present a new set of numerical-relativity simulations of merging binary neutron stars, aiming to identify possible observable signatures of the slope of the symmetry energy $L_{…
On the Role of Muons in Binary Neutron Star Mergers: First Simulations
Henrique Gieg, Federico Schianchi, Maximiliano Ujevic +1
In this work we present a set of binary neutron star (BNS) merger simulations including the net muon fraction as an additional degree-of-freedom in the equation of state (EoS) and…
General-Relativistic Hydrodynamics Simulation of a Neutron Star - Sub-Solar-Mass Black Hole Merger
Ivan Markin, Anna Neuweiler, Adrian Abac +4
Over the last few years, there has been an increasing interest in sub-solar mass black holes due to their potential to provide valuable information about cosmology or the black hol…
The error budget of binary neutron star merger simulations for configurations with high spin
Hao-Jui Kuan, Ivan Markin, Maximiliano Ujevic +4
Numerical-relativity simulations offer a unique approach to investigating the dynamics of binary neutron star mergers and provide the most accurate predictions of waveforms in the…