Darwin-Riemann problems in general relativity
S. Bonazzola, E. Gourgoulhon, P. Grandclement, J.-A. Marck (DARC,, CNRS, Observatoire de Paris)
TL;DR
This paper reviews recent progress in calculating irrotational Darwin-Riemann configurations in general relativity, which model the late inspiral phase of binary neutron star systems.
Contribution
It provides an overview of new computational results for relativistic binary neutron star models nearing merger.
Findings
Improved methods for computing relativistic binary configurations.
Enhanced understanding of late inspiral dynamics.
Potential implications for gravitational wave predictions.
Abstract
A review is given of recent results about the computation of irrotational Darwin-Riemann configurations in general relativity. Such configurations are expected to represent fairly well the late stages of inspiralling binary neutron stars.
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