Expanding the Reach of Gravitational Wave Astronomy to the Edge of the Universe: The Gravitational-Wave International Committee Study Reports on Next Generation Ground-based Gravitational-Wave Observatories
David Reitze, Michele Punturo, Peter Couvares, Stavros Katsanevas,, Takaaki Kajita, Vicky Kalogera, Harald Lueck, David McClelland, Sheila Rowan,, Gary Sanders, B.S. Sathyaprakash, David Shoemaker, Jo van den Brand

TL;DR
This report discusses the development of next-generation ground-based gravitational-wave observatories to significantly extend the observable universe, enabling new scientific discoveries in astrophysics and cosmology over the next 15-20 years.
Contribution
It provides a comprehensive roadmap and scientific rationale for building advanced gravitational-wave detectors beyond current capabilities.
Findings
Proposes a network of third-generation observatories
Extends gravitational-wave detection horizon to the universe's edge
Identifies technological and scientific challenges for future detectors
Abstract
The first direct detection of gravitational waves emitted from a pair of merging black holes in 2015 has been heralded as one of most significant scientific breakthroughs in physics and astronomy of the 21st century. Motivated by the tremendous scientific opportunities now opened by gravitational-wave observatories and recognizing that to fully exploit the new field will require new observatories that may take 15 to 20 years from conception until operations begin, the Gravitational Wave International Committee (GWIC) convened a subcommittee to examine the path to build and operate a network of future ground-based observatories, capable of extending the observational GW horizon well beyond that currently attainable with the current generation of detectors. This report is the first in a six part series of reports by the GWIC 3G Subcommittee: i) Expanding the Reach of Gravitational Wave…
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Taxonomy
TopicsPulsars and Gravitational Waves Research
