B. S. Sathyaprakash, Matthew Bailes, Mansi M. Kasliwal, Samaya Nissanke, Shreya Anand, Igor Andreoni, Monica Colpi, Michael Coughlin, Evan Hall, Vicky Kalogera, Dan Kasen, Alberto Sesana
Published 2019-03-22Version 1
Future GW detector networks and EM observatories will provide a unique opportunity to observe the most luminous events in the Universe involving matter in extreme environs. They will address some of the key questions in physics and astronomy: formation and evolution of compact binaries, sites of formation of heavy elements and the physics of jets.
Comments: 11 pages, two tables, White Paper submitted to the Astro-2020 (2020 Astronomy and Astrophysics Decadal Survey) by GWIC-3G Science Case Team (GWIC: Gravitational-Wave International Committee)
Gravitational waves from neutron star mergers and their relation to the nuclear equation of state
Constraining the neutron-matter equation of state with gravitational waves
Stacked Search for Gravitational Waves from the 2006 SGR 1900+14 Storm
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