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most citedGravitational waves and mass ejecta from binary neutron star mergers: Effect of the mass-ratio

191 citations · 1.2k across the 41 of their papers we have counts for

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gr-qc2025

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…

gr-qc2025★ 3 cited

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_{…

gr-qc2025

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…

gr-qc2024★ 11 cited

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…

gr-qc2023★ 58 cited

New and Robust Gravitational-Waveform Model for High-Mass-Ratio Binary Neutron Star Systems with Dynamical Tidal Effects

Adrian Abac, Tim Dietrich, Alessandra Buonanno +2

For the analysis of gravitational-wave signals, fast and accurate gravitational-waveform models are required. These enable us to obtain information on the system properties from co…

gr-qc2023

The Radiant Massive Magnetic Dipole

José Diaz Polanco, José Ayala, Maximiliano Ujevic

We present an exact, time-dependent solution for the Einstein field equations that models the coupling between an anisotropic fluid and a magnetic field in an axially symmetric spa…