Multimessenger Universe with Gravitational Waves from Binaries
arXiv:1903.09277
Abstract
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.
arXiv comment11 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)
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- Gravitational Collider Physics
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- Gravitational Wave observatories may be able to detect hyperbolic encounters of Black Holes
- Distinguishing high-mass binary neutron stars from binary black holes with second- and third-generation gravitational wave observatories
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