Multimessenger Universe with Gravitational Waves from Binaries

Alberto Sesana (U. Birmingham); B.S. Sathyaprakash (Penn State; Cardiff University); Dan Kasen (UC Berkeley); Evan Hall (MIT); Igor Andreoni (Caltech); Mansi M. Kasliwal (Caltech); Matthew Bailes (Swinburne U.); Michael Coughlin (Caltech); Monica Colpi (U. of Milano - Bicocca)

arxiv: 1903.09277 · v1 · pith:OZ4XKK5Anew · submitted 2019-03-22 · 🌌 astro-ph.HE · nucl-th

Multimessenger Universe with Gravitational Waves from Binaries

B.S. Sathyaprakash (Penn State , Cardiff University) , Matthew Bailes (Swinburne U.) , Mansi M. Kasliwal (Caltech) , Samaya Nissanke (U. of Amsterdam) , Shreya Anand (Caltech) , Igor Andreoni (Caltech) , Monica Colpi (U. of Milano - Bicocca)

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Michael Coughlin (Caltech) Evan Hall (MIT) Vicky Kalogera (Northwestern U.) Dan Kasen (UC Berkeley) Alberto Sesana (U. Birmingham)

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classification 🌌 astro-ph.HE nucl-th

keywords binariesformationphysicsuniversewilladdressastronomycompact

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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.

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