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astro-ph.HE2020
Shedding light on the angular momentum evolution of binary neutron star merger remnants: a semi-analytic model
Matteo Lucca, Laura Sagunski, Federico Guercilena +1
The main features of the gravitational dynamics of binary neutron star systems are now well established. While the inspiral can be precisely described in the post-Newtonian approxi…
astro-ph.HE2019
The lifetime of binary neutron star merger remnants
Matteo Lucca, Laura Sagunski
Although the main features of the evolution of binary neutron star systems are now well established, many details are still subject to debate, especially regarding the post-merger…