Exploring Populations of Low Mass Merging Compact Binary Systems with Single Einstein Telescope
Abstract
Einstein Telescope (ET), a the future third generation gravitational wave detector will be sensitive to gravitational wave signal down to 1 Hz. We present an algorithm to estimate the parameters of the low mass merging compact binary systems such as localisation, chirp mass, redshift, mass ratios and total mass of the source which are crucial in order to estimate the capability of ET to study various compact binary populations. We analysed the compact binary populations of (i) Pop I and Pop II, (ii) Pop III, and (iii) globular clusters, with single ET.
- Publication:
-
Neutron Star Astrophysics at the Crossroads: Magnetars and the Multimessenger Revolution
- Pub Date:
- 2023
- DOI:
- 10.1017/S1743921322000849
- Bibcode:
- 2023IAUS..363..363S
- Keywords:
-
- gravitational waves;
- stars: neutron;
- black hole;
- methods: data analysis