Prospects for doubling the range of Advanced LIGO

In the coming years, the gravitational-wave community will be optimizing detector performance to target a variety of astrophysical sources which make competing demands on detector sensitivity in different frequency bands. In this paper we describe a number of technologies that are being developed as...

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Main Authors: Miller, John, Barsotti, Lisa, Vitale, Salvatore, Sigg, Daniel, Fritschel, Peter K, Evans, Matthew J
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:English
Published: American Physical Society 2015
Online Access:http://hdl.handle.net/1721.1/96149
https://orcid.org/0000-0001-8459-4499
https://orcid.org/0000-0003-2700-0767
https://orcid.org/0000-0003-1983-3187
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author Miller, John
Barsotti, Lisa
Vitale, Salvatore
Sigg, Daniel
Fritschel, Peter K
Evans, Matthew J
author2 Massachusetts Institute of Technology. Department of Physics
author_facet Massachusetts Institute of Technology. Department of Physics
Miller, John
Barsotti, Lisa
Vitale, Salvatore
Sigg, Daniel
Fritschel, Peter K
Evans, Matthew J
author_sort Miller, John
collection MIT
description In the coming years, the gravitational-wave community will be optimizing detector performance to target a variety of astrophysical sources which make competing demands on detector sensitivity in different frequency bands. In this paper we describe a number of technologies that are being developed as anticipated upgrades to the Advanced LIGO detectors and quantify the potential sensitivity improvement they offer. Specifically, we consider squeezed light injection for the reduction of quantum noise, detector design and materials changes which mitigate thermal noise and mirrors with significantly increased mass. We explore how each of these technologies impacts the detection of the most promising gravitational-wave sources and suggest an effective progression of upgrades which culminates in a twofold improvement in broadband sensitivity.
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spelling mit-1721.1/961492022-10-03T11:10:52Z Prospects for doubling the range of Advanced LIGO Miller, John Barsotti, Lisa Vitale, Salvatore Sigg, Daniel Fritschel, Peter K Evans, Matthew J Massachusetts Institute of Technology. Department of Physics LIGO (Observatory : Massachusetts Institute of Technology) MIT Kavli Institute for Astrophysics and Space Research Miller, John Barsotti, Lisa Vitale, Salvatore Fritschel, Peter K. Evans, Matthew J. In the coming years, the gravitational-wave community will be optimizing detector performance to target a variety of astrophysical sources which make competing demands on detector sensitivity in different frequency bands. In this paper we describe a number of technologies that are being developed as anticipated upgrades to the Advanced LIGO detectors and quantify the potential sensitivity improvement they offer. Specifically, we consider squeezed light injection for the reduction of quantum noise, detector design and materials changes which mitigate thermal noise and mirrors with significantly increased mass. We explore how each of these technologies impacts the detection of the most promising gravitational-wave sources and suggest an effective progression of upgrades which culminates in a twofold improvement in broadband sensitivity. National Science Foundation (U.S.) (Laser Interferometer Gravitational Wave Observatory. Grant PHY-0757058) National Science Foundation (U.S.) (Advanced Laser Interferometer Gravitational Wave Observatory. Award PHY-0823459) 2015-03-24T16:26:25Z 2015-03-24T16:26:25Z 2015-03 2014-10 2015-03-16T22:00:04Z Article http://purl.org/eprint/type/JournalArticle 1550-7998 1550-2368 http://hdl.handle.net/1721.1/96149 Miller, John, Lisa Barsotti, Salvatore Vitale, Peter Fritschel, Matthew Evans, and Daniel Sigg. “Prospects for Doubling the Range of Advanced LIGO.” Phys. Rev. D 91, no. 6 (March 2015). © 2015 American Physical Society https://orcid.org/0000-0001-8459-4499 https://orcid.org/0000-0003-2700-0767 https://orcid.org/0000-0003-1983-3187 en http://dx.doi.org/10.1103/PhysRevD.91.062005 Physical Review D Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. American Physical Society application/pdf American Physical Society American Physical Society
spellingShingle Miller, John
Barsotti, Lisa
Vitale, Salvatore
Sigg, Daniel
Fritschel, Peter K
Evans, Matthew J
Prospects for doubling the range of Advanced LIGO
title Prospects for doubling the range of Advanced LIGO
title_full Prospects for doubling the range of Advanced LIGO
title_fullStr Prospects for doubling the range of Advanced LIGO
title_full_unstemmed Prospects for doubling the range of Advanced LIGO
title_short Prospects for doubling the range of Advanced LIGO
title_sort prospects for doubling the range of advanced ligo
url http://hdl.handle.net/1721.1/96149
https://orcid.org/0000-0001-8459-4499
https://orcid.org/0000-0003-2700-0767
https://orcid.org/0000-0003-1983-3187
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