Criteria for identifying and evaluating locations that could potentially host the Cosmic Explorer observatories

Fuente: arXiv
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Main Authors: Daniel, Kathryne J., Smith, Joshua R., Ballmer, Stefan, Bristol, Warren, Driggers, Jennifer C., Effler, Anamaria, Evans, Matthew, Hoover, Joseph, Kuns, Kevin, Landry, Michael, Lovelace, Geoffrey, Lukinbeal, Chris, Mandic, Vuk, Pham, Kiet, Read, Jocelyn, Russell, Joshua B., Schiettekatte, Francois, Schofield, Robert M. S., Scholz, Christopher A., Shoemaker, David H., Sledge, Piper, Strunk, Amber
Format: Preprint
Published: 2024
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author Daniel, Kathryne J.
Smith, Joshua R.
Ballmer, Stefan
Bristol, Warren
Driggers, Jennifer C.
Effler, Anamaria
Evans, Matthew
Hoover, Joseph
Kuns, Kevin
Landry, Michael
Lovelace, Geoffrey
Lukinbeal, Chris
Mandic, Vuk
Pham, Kiet
Read, Jocelyn
Russell, Joshua B.
Schiettekatte, Francois
Schofield, Robert M. S.
Scholz, Christopher A.
Shoemaker, David H.
Sledge, Piper
Strunk, Amber
author_facet Daniel, Kathryne J.
Smith, Joshua R.
Ballmer, Stefan
Bristol, Warren
Driggers, Jennifer C.
Effler, Anamaria
Evans, Matthew
Hoover, Joseph
Kuns, Kevin
Landry, Michael
Lovelace, Geoffrey
Lukinbeal, Chris
Mandic, Vuk
Pham, Kiet
Read, Jocelyn
Russell, Joshua B.
Schiettekatte, Francois
Schofield, Robert M. S.
Scholz, Christopher A.
Shoemaker, David H.
Sledge, Piper
Strunk, Amber
contents Cosmic Explorer (CE) is a next-generation ground-based gravitational-wave observatory that is being designed in the 2020s and is envisioned to begin operations in the 2030s together with the Einstein Telescope in Europe. The CE concept currently consists of two widely separated L-shaped observatories in the United States, one with 40 km-long arms and the other with 20 km-long arms. This order of magnitude increase in scale with respect to the LIGO-Virgo-KAGRA observatories will, together with technological improvements, deliver an order of magnitude greater astronomical reach, allowing access to gravitational waves from remnants of the first stars and opening a wide discovery aperture to the novel and unknown. In addition to pushing the reach of gravitational-wave astronomy, CE endeavors to approach the lifecycle of large scientific facilities in a way that prioritizes mutually beneficial relationships with local and Indigenous communities. This article describes the (scientific, cost and access, and social) criteria that will be used to identify and evaluate locations that could potentially host the CE observatories.
format Preprint
id arxiv_https___arxiv_org_abs_2410_00293
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Criteria for identifying and evaluating locations that could potentially host the Cosmic Explorer observatories
Daniel, Kathryne J.
Smith, Joshua R.
Ballmer, Stefan
Bristol, Warren
Driggers, Jennifer C.
Effler, Anamaria
Evans, Matthew
Hoover, Joseph
Kuns, Kevin
Landry, Michael
Lovelace, Geoffrey
Lukinbeal, Chris
Mandic, Vuk
Pham, Kiet
Read, Jocelyn
Russell, Joshua B.
Schiettekatte, Francois
Schofield, Robert M. S.
Scholz, Christopher A.
Shoemaker, David H.
Sledge, Piper
Strunk, Amber
Instrumentation and Detectors
Instrumentation and Methods for Astrophysics
Cosmic Explorer (CE) is a next-generation ground-based gravitational-wave observatory that is being designed in the 2020s and is envisioned to begin operations in the 2030s together with the Einstein Telescope in Europe. The CE concept currently consists of two widely separated L-shaped observatories in the United States, one with 40 km-long arms and the other with 20 km-long arms. This order of magnitude increase in scale with respect to the LIGO-Virgo-KAGRA observatories will, together with technological improvements, deliver an order of magnitude greater astronomical reach, allowing access to gravitational waves from remnants of the first stars and opening a wide discovery aperture to the novel and unknown. In addition to pushing the reach of gravitational-wave astronomy, CE endeavors to approach the lifecycle of large scientific facilities in a way that prioritizes mutually beneficial relationships with local and Indigenous communities. This article describes the (scientific, cost and access, and social) criteria that will be used to identify and evaluate locations that could potentially host the CE observatories.
title Criteria for identifying and evaluating locations that could potentially host the Cosmic Explorer observatories
topic Instrumentation and Detectors
Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2410.00293