Distance measures in gravitational-wave astrophysics and cosmology
We present quantities which characterize the sensitivity of gravitational-wave observatories to sources at cosmological distances. In particular, we introduce and generalize the horizon, range, response, and reach distances. These quantities incorporate a number of important effects, including cosmo...
Main Authors: | , , , , , |
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Format: | Article |
Language: | English |
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IOP Publishing
2022
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Online Access: | https://hdl.handle.net/1721.1/142503 |
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author | Chen, Hsin-Yu Holz, Daniel E Miller, John Evans, Matthew Vitale, Salvatore Creighton, Jolien |
author2 | LIGO (Observatory : Massachusetts Institute of Technology) |
author_facet | LIGO (Observatory : Massachusetts Institute of Technology) Chen, Hsin-Yu Holz, Daniel E Miller, John Evans, Matthew Vitale, Salvatore Creighton, Jolien |
author_sort | Chen, Hsin-Yu |
collection | MIT |
description | We present quantities which characterize the sensitivity of gravitational-wave observatories to sources at cosmological distances. In particular, we introduce and generalize the horizon, range, response, and reach distances. These quantities incorporate a number of important effects, including cosmologically well-defined distances and volumes, cosmological redshift, cosmological time dilation, and rate density evolution. In addition, these quantities incorporate unique aspects of gravitational wave detectors, such as the variable sky sensitivity of the detectors and the scaling of the sensitivity with inverse distance. An online calculator (https://users.rcc.uchicago.edu/~dholz/gwc/) and python notebook (https://github.com/hsinyuc/distancetool) to determine GW distances are available. We provide answers to the question: ‘How far can gravitational-wave detectors hear. |
first_indexed | 2024-09-23T16:41:25Z |
format | Article |
id | mit-1721.1/142503 |
institution | Massachusetts Institute of Technology |
language | English |
last_indexed | 2024-09-23T16:41:25Z |
publishDate | 2022 |
publisher | IOP Publishing |
record_format | dspace |
spelling | mit-1721.1/1425032023-02-15T20:10:24Z Distance measures in gravitational-wave astrophysics and cosmology Chen, Hsin-Yu Holz, Daniel E Miller, John Evans, Matthew Vitale, Salvatore Creighton, Jolien LIGO (Observatory : Massachusetts Institute of Technology) We present quantities which characterize the sensitivity of gravitational-wave observatories to sources at cosmological distances. In particular, we introduce and generalize the horizon, range, response, and reach distances. These quantities incorporate a number of important effects, including cosmologically well-defined distances and volumes, cosmological redshift, cosmological time dilation, and rate density evolution. In addition, these quantities incorporate unique aspects of gravitational wave detectors, such as the variable sky sensitivity of the detectors and the scaling of the sensitivity with inverse distance. An online calculator (https://users.rcc.uchicago.edu/~dholz/gwc/) and python notebook (https://github.com/hsinyuc/distancetool) to determine GW distances are available. We provide answers to the question: ‘How far can gravitational-wave detectors hear. 2022-05-12T18:01:51Z 2022-05-12T18:01:51Z 2020 2022-05-12T17:51:53Z Article http://purl.org/eprint/type/JournalArticle https://hdl.handle.net/1721.1/142503 Chen, Hsin-Yu, Holz, Daniel E, Miller, John, Evans, Matthew, Vitale, Salvatore et al. 2020. "Distance measures in gravitational-wave astrophysics and cosmology." Classical and Quantum Gravity, 38 (5). en 10.1088/1361-6382/ABD594 Classical and Quantum Gravity Attribution-NonCommercial-ShareAlike 4.0 International https://creativecommons.org/licenses/by-nc-sa/4.0/ application/pdf IOP Publishing arXiv |
spellingShingle | Chen, Hsin-Yu Holz, Daniel E Miller, John Evans, Matthew Vitale, Salvatore Creighton, Jolien Distance measures in gravitational-wave astrophysics and cosmology |
title | Distance measures in gravitational-wave astrophysics and cosmology |
title_full | Distance measures in gravitational-wave astrophysics and cosmology |
title_fullStr | Distance measures in gravitational-wave astrophysics and cosmology |
title_full_unstemmed | Distance measures in gravitational-wave astrophysics and cosmology |
title_short | Distance measures in gravitational-wave astrophysics and cosmology |
title_sort | distance measures in gravitational wave astrophysics and cosmology |
url | https://hdl.handle.net/1721.1/142503 |
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