Advanced LIGO

Fil: Domínguez, Alfredo Eduardo. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina.

Bibliographic Details
Main Authors: Aasi, J., Abbott, B. P., Abbott, R., Abbott, T., Abernathy, M. R., Ackley, K., Domínguez, Alfredo Eduardo, Maglione, César Germán, Ortega Larcher, Walter Emanuel, Quiroga, Gonzalo Damián, Reula, Oscar Alejandro
Format:
Language:eng
Published: 2022
Subjects:
Online Access:http://hdl.handle.net/11086/29142
https://doi.org/10.48550/arXiv.1411.4547
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author Aasi, J.
Abbott, B. P.
Abbott, R.
Abbott, T.
Abernathy, M. R.
Ackley, K.
Domínguez, Alfredo Eduardo
Maglione, César Germán
Ortega Larcher, Walter Emanuel
Quiroga, Gonzalo Damián
Reula, Oscar Alejandro
author_facet Aasi, J.
Abbott, B. P.
Abbott, R.
Abbott, T.
Abernathy, M. R.
Ackley, K.
Domínguez, Alfredo Eduardo
Maglione, César Germán
Ortega Larcher, Walter Emanuel
Quiroga, Gonzalo Damián
Reula, Oscar Alejandro
author_sort Aasi, J.
collection Repositorio Digital Universitario
description Fil: Domínguez, Alfredo Eduardo. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina.
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institution Universidad Nacional de Cordoba
language eng
publishDate 2022
record_format dspace
spelling rdu-unc.291422023-08-31T13:16:44Z Advanced LIGO Aasi, J. Abbott, B. P. Abbott, R. Abbott, T. Abernathy, M. R. Ackley, K. Domínguez, Alfredo Eduardo Maglione, César Germán Ortega Larcher, Walter Emanuel Quiroga, Gonzalo Damián Reula, Oscar Alejandro Gravitational waves Interferometers Seismic isolation Optics submittedVersion Fil: Domínguez, Alfredo Eduardo. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina. Fil: Domínguez, Alfredo Eduardo. Argentinian Gravitational Wave Group; Argentina. Fil: Maglione, César Germán. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina. Fil: Maglione, César Germán. Argentinian Gravitational Wave Group; Argentina. Fil: Ortega Larcher, Walter Emanuel. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina. Fil: Ortega Larcher, Walter Emanuel. Argentinian Gravitational Wave Group; Argentina. Fil: Quiroga, Gonzalo Damián. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina. Fil: Quiroga, Gonzalo Damián. Argentinian Gravitational Wave Group; Argentina. Fil: Reula, Oscar Alejandro. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina. Fil: Reula, Oscar Alejandro. Argentinian Gravitational Wave Group; Argentina. The Advanced LIGO gravitational wave detectors are second-generation instruments designed and built for the two LIGO observatories in Hanford, WA and Livingston, LA, USA. The two instruments are identical in design, and are specialized versions of a Michelson interferometer with 4 km long arms. As in Initial LIGO, Fabry–Perot cavities are used in the arms to increase the interaction time with a gravitational wave, and power recycling is used to increase the effective laser power. Signal recycling has been added in Advanced LIGO to improve the frequency response. In the most sensitive frequency region around 100 Hz, the design strain sensitivity is a factor of 10 better than Initial LIGO. In addition, the low frequency end of the sensitivity band is moved from 40 Hz down to 10 Hz. All interferometer components have been replaced with improved technologies to achieve this sensitivity gain. Much better seismic isolation and test mass suspensions are responsible for the gains at lower frequencies. Higher laser power, larger test masses and improved mirror coatings lead to the improved sensitivity at mid and high frequencies. Data collecting runs with these new instruments are planned to begin in mid-2015. submittedVersion Fil: Domínguez, Alfredo Eduardo. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina. Fil: Domínguez, Alfredo Eduardo. Argentinian Gravitational Wave Group; Argentina. Fil: Maglione, César Germán. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina. Fil: Maglione, César Germán. Argentinian Gravitational Wave Group; Argentina. Fil: Ortega Larcher, Walter Emanuel. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina. Fil: Ortega Larcher, Walter Emanuel. Argentinian Gravitational Wave Group; Argentina. Fil: Quiroga, Gonzalo Damián. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina. Fil: Quiroga, Gonzalo Damián. Argentinian Gravitational Wave Group; Argentina. Fil: Reula, Oscar Alejandro. Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física; Argentina. Fil: Reula, Oscar Alejandro. Argentinian Gravitational Wave Group; Argentina. Física de Partículas y Campos 2022-10-25T14:36:05Z 2022-10-25T14:36:05Z 2015 article http://hdl.handle.net/11086/29142 https://doi.org/10.48550/arXiv.1411.4547 eng De la versión publicada: https://doi.org/10.1088/0264-9381/32/7/074001 Attribution-NonCommercial-NoDerivatives 4.0 International http://creativecommons.org/licenses/by-nc-nd/4.0/ Impreso; Electrónico y/o Digital ISSN: 0264-9381 e-ISSN: 1361-6382
spellingShingle Gravitational waves
Interferometers
Seismic isolation
Optics
Aasi, J.
Abbott, B. P.
Abbott, R.
Abbott, T.
Abernathy, M. R.
Ackley, K.
Domínguez, Alfredo Eduardo
Maglione, César Germán
Ortega Larcher, Walter Emanuel
Quiroga, Gonzalo Damián
Reula, Oscar Alejandro
Advanced LIGO
title Advanced LIGO
title_full Advanced LIGO
title_fullStr Advanced LIGO
title_full_unstemmed Advanced LIGO
title_short Advanced LIGO
title_sort advanced ligo
topic Gravitational waves
Interferometers
Seismic isolation
Optics
url http://hdl.handle.net/11086/29142
https://doi.org/10.48550/arXiv.1411.4547
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