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[Paper Review] Cosmic Explorer: The U.S. Contribution to Gravitational-Wave Astronomy beyond LIGO
D. H. Reitze, R. X. Adhikari|arXiv (Cornell University)|Jul 10, 2019
History and Developments in Astronomy510 citations
TL;DR
The paper outlines the U.S. plan and the ten-year R&D needed to realize Cosmic Explorer, a future third-generation gravitational-wave detector beyond LIGO.
ABSTRACT
This white paper describes the research and development needed over the next decade to realize "Cosmic Explorer," the U.S. node of a future third-generation detector network that will be capable of observing and characterizing compact gravitational-wave sources to cosmological redshifts.
Motivation & Objective
- Motivate the development of a third-generation gravitational-wave detector network beyond LIGO.
- Identify the key R&D areas and technology requirements for Cosmic Explorer over the coming decade.
- Characterize the scientific capabilities needed to observe and characterize compact sources to cosmological redshifts.
- Define the role of Cosmic Explorer in a global network for gravitational-wave astronomy.
Proposed method
- Describe the research and development needed over the next decade to realize Cosmic Explorer.
- Outline the technical challenges and technology development areas for a next-generation detector.
- Discuss how Cosmic Explorer would integrate into a broader detector network and science goals.
Experimental results
Research questions
- RQ1What are the essential R&D areas required to achieve a third-generation gravitational-wave detector beyond LIGO?
- RQ2What technical capabilities and innovations are needed to observe and characterize compact binary sources to cosmological redshifts?
- RQ3How would Cosmic Explorer contribute to a global gravitational-wave astronomy network in the next decade?
Key findings
- Cosmic Explorer is envisioned as the U.S. node of a future third-generation detector network.
- The paper identifies the research and development needed over the next decade to realize Cosmic Explorer.
- The goals include observing and characterizing compact gravitational-wave sources at cosmological redshifts.
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This review was created by AI and reviewed by human editors.