19 citations · 60 across the 12 of their papers we have counts for
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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…
M1 neutrino transport within the numerical-relativistic code BAM with application to low mass binary neutron star mergers
Federico Schianchi, Henrique Gieg, Vsevolod Nedora +4
Neutrino interactions are essential for an accurate understanding of the binary neutron star merger process. In this article, we extend the code infrastructure of the well-establis…
Reverse phase transitions in binary neutron-star systems with exotic-matter cores
Maximiliano Ujevic, Henrique Gieg, Federico Schianchi +3
Multi-messenger observations of binary neutron star mergers provide a unique opportunity to constrain the dense-matter equation of state. Although it is known from quantum chromody…
Incorporating a radiative hydrodynamics scheme in the numerical-relativity code BAM
Henrique Gieg, Federico Schianchi, Tim Dietrich +1
To study binary neutron star systems and to interpret observational data such as gravitational-wave and kilonova signals, one needs an accurate description of the processes that ta…
High-accuracy high-mass ratio simulations for binary neutron stars and their comparison to existing waveform models
Maximiliano Ujevic, Alireza Rashti, Henrique Gieg +2
The subsequent observing runs of the advanced gravitational-wave detector network will likely provide us with various gravitational-wave observations of binary neutron star systems…
Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity
Henrique Gieg, Tim Dietrich, Maximiliano Ujevic
The gravitational wave and electromagnetic signatures connected to the merger of two neutron stars allow us to test the nature of matter at supranuclear densities. Since the Equati…