5–7 Nov 2020
Universität Hamburg
Europe/Berlin timezone

Using gravitational waves to distinguish between neutron stars and black holes in binaries

5 Nov 2020, 15:00
20m
Online (Universität Hamburg)

Online

Universität Hamburg

Speaker

Stephanie Brown (Max Planck Institut für Gravitationsphysik)

Description

In August 2017, the first detection of a neutron star merger, GW170817, created an opportunity to explore the equation of state of supranuclear matter using gravitational waves. But it is unknown under what circumstances this kind of gravitational wave data could distinguish between different types of mergers. For example, can the data distinguish a merger of black holes from a merger of neutron stars or the merger of a neutron star and a black hole? Here we build on earlier results using chiral effective field theory to explore whether the data from LIGO and Virgo, A+, Voyager, or Cosmic Explorer can lead to such a distinction. The results suggest that LIGO and Virgo will be able to distinguish between a binary neutron star and a binary black hole but not between neutron-star--black-hole binary and a black hole binary.

Authors

Stephanie Brown (Max Planck Institut für Gravitationsphysik) Dr Ingo Tews (Los Alamos National Laboratory) Dr Badri Krishnan (Max Planck Institut für Gravitationsphysik) Dr Sumit Kumar (Max Planck Institut für Gravitationsphysik) Dr Collin Capano (Max Planck Institut für Gravitationsphysik) Dr Duncan Brown (Syracuse University) Dr Sanjay Reddy (University of Washington)

Presentation materials