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.
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)
References in corpus (10)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- An Ordinary Short Gamma-Ray Burst with Extraordinary Implications: Fermi-GBM Detection of GRB 170817A
- A gravitational-wave standard siren measurement of the Hubble constant
- Origin of the heavy elements in binary neutron-star mergers from a gravitational wave event
- The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. I. Dark Energy Camera Discovery of the Optical Counterpart
- Determination of Dark Energy by the Einstein Telescope: Comparing with CMB, BAO and SNIa Observations
- Estimating cosmological parameters by the simulated data of gravitational waves from the Einstein Telescope
- Constraining stellar binary black hole formation scenarios with eLISA eccentricity measurements
- Spitzer Mid-Infrared Detections of Neutron Star Merger GW170817 Suggests Synthesis of the Heaviest Elements
- On the Progenitor of Binary Neutron Star Merger GW170817