Stephan Rosswog | Multi-messenger signals from merging neutron stars: a new tool and a new scenario

Europe/Berlin
SR 05 (Villa)

SR 05

Villa

Description
Neutron star mergers are related to a large number of (astro-)physical
questions. For example, they had long been suspected to produce gravitational
waves, gamma ray bursts and -by some- to produce heavy "rapid neutron
capture" elements. While overall convincing, all these conjectures were
only based on indirect arguments and none was proven by direct observations.
This situation changed dramatically on August 17, 2017 when the first ever
neutron star merger was detected in both gravitational and electromagnetic
waves. In this talk I will discuss our current understanding of the merger process
and its multi-messenger signatures. I will also present a novel simulation tool:
the Lagrangian Numerical Relativity code SPHINCS_BSSN. As an application of this
new tool, I will discuss a merger scenario that has not been explored before.
The agenda of this meeting is empty