Effects of nuclear matter properties in neutron star mergers
Maximilian Jacobi, Federico Maria Guercilena, Sabrina Huth, Giacomo, Ricigliano, Almudena Arcones, Achim Schwenk

TL;DR
This study investigates how different nuclear matter properties, modeled through various equations of state, influence the dynamics, gravitational wave signals, and matter ejection in binary neutron star mergers.
Contribution
It systematically analyzes the effects of specific nuclear matter parameters on merger outcomes using multiple Skyrme-based EOS models.
Findings
Some merger aspects are sensitive to EOS near saturation density.
Other aspects depend on high-density EOS behavior.
Density dependence of the EOS significantly affects merger dynamics.
Abstract
The dynamics in mergers of binary neutron star (BNS) systems depend sensitively on the equation of state (EOS) of dense matter. This has profound implications on the emission of gravitational waves (GWs) and the ejection of matter in the merger and post-merger phases and is thus of high interest for multi-messenger astronomy. Today, a variety of nuclear EOSs are available with various underlying microphysical models. This calls for a study to focus on EOS effects from different physical nuclear matter properties and their influence on BNS mergers. We perform simulations of equal-mass BNS mergers with a set of 9 different EOSs based on Skyrme density functionals. In the models, we systematically vary the effective nucleon mass, incompressibility, and symmetry energy at saturation density. This allows us to investigate the influence of specific nuclear matter properties on the dynamics of…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Gamma-ray bursts and supernovae · High-pressure geophysics and materials
