Search for gravitational wave ringdowns from perturbed intermediate mass black holes in LIGO-Virgo data from 2005–2010

We report results from a search for gravitational waves produced by perturbed intermediate mass black holes (IMBH) in data collected by LIGO and Virgo between 2005 and 2010. The search was sensitive to astrophysical sources that produced damped sinusoid gravitational wave signals, also known as ring...

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Main Authors: Barsotti, Lisa, Biscans, Sebastien, Bodiya, Timothy Paul, Donovan, Frederick J., Essick, Reed Clasey, Evans, Matthew J., Fritschel, Peter K., Gras, Slawek, Isogai, Tomoki, Katsavounidis, Erotokritos, Kwee, Patrick, Lee, J., Libson, Adam, Lynch, Ryan Christopher, MacInnis, Myron E., Mason, Kenneth R., Matichard, Fabrice, Mavalvala, Nergis, Miller, John, Mittleman, Richard K., Oelker, Eric Glenn, Shoemaker, David H., Tse, Maggie, Vaulin, Ruslan, Vitale, Salvatore, Weiss, Rainer, Wipf, C. C., Zhang, Fan, Zucker, Michael E., Aggarwal, Nancy,Ph. D.Massachusetts Institute of Technology.
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:en_US
Published: American Physical Society 2014
Online Access:http://hdl.handle.net/1721.1/90882
https://orcid.org/0000-0002-0026-3877
https://orcid.org/0000-0003-2815-7387
https://orcid.org/0000-0003-0219-9706
https://orcid.org/0000-0001-6550-3045
https://orcid.org/0000-0002-4147-2560
https://orcid.org/0000-0003-1510-4921
https://orcid.org/0000-0001-8459-4499
https://orcid.org/0000-0002-9635-7527
https://orcid.org/0000-0001-8150-7062
https://orcid.org/0000-0002-2544-1596
https://orcid.org/0000-0003-2700-0767
https://orcid.org/0000-0003-1983-3187
https://orcid.org/0000-0002-5163-683X
https://orcid.org/0000-0003-2047-3166
https://orcid.org/0000-0001-8196-9267
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author Barsotti, Lisa
Biscans, Sebastien
Bodiya, Timothy Paul
Donovan, Frederick J.
Essick, Reed Clasey
Evans, Matthew J.
Fritschel, Peter K.
Gras, Slawek
Isogai, Tomoki
Katsavounidis, Erotokritos
Kwee, Patrick
Lee, J.
Libson, Adam
Lynch, Ryan Christopher
MacInnis, Myron E.
Mason, Kenneth R.
Matichard, Fabrice
Mavalvala, Nergis
Miller, John
Mittleman, Richard K.
Oelker, Eric Glenn
Shoemaker, David H.
Tse, Maggie
Vaulin, Ruslan
Vitale, Salvatore
Weiss, Rainer
Wipf, C. C.
Zhang, Fan
Zucker, Michael E.
Aggarwal, Nancy,Ph. D.Massachusetts Institute of Technology.
author2 Massachusetts Institute of Technology. Department of Physics
author_facet Massachusetts Institute of Technology. Department of Physics
Barsotti, Lisa
Biscans, Sebastien
Bodiya, Timothy Paul
Donovan, Frederick J.
Essick, Reed Clasey
Evans, Matthew J.
Fritschel, Peter K.
Gras, Slawek
Isogai, Tomoki
Katsavounidis, Erotokritos
Kwee, Patrick
Lee, J.
Libson, Adam
Lynch, Ryan Christopher
MacInnis, Myron E.
Mason, Kenneth R.
Matichard, Fabrice
Mavalvala, Nergis
Miller, John
Mittleman, Richard K.
Oelker, Eric Glenn
Shoemaker, David H.
Tse, Maggie
Vaulin, Ruslan
Vitale, Salvatore
Weiss, Rainer
Wipf, C. C.
Zhang, Fan
Zucker, Michael E.
Aggarwal, Nancy,Ph. D.Massachusetts Institute of Technology.
author_sort Barsotti, Lisa
collection MIT
description We report results from a search for gravitational waves produced by perturbed intermediate mass black holes (IMBH) in data collected by LIGO and Virgo between 2005 and 2010. The search was sensitive to astrophysical sources that produced damped sinusoid gravitational wave signals, also known as ringdowns, with frequency 50 ≤ f[subscript 0]/Hz ≤ 2000 and decay timescale 0.0001 ≲ τ/s ≲ 0.1 characteristic of those produced in mergers of IMBH pairs. No significant gravitational wave candidate was detected. We report upper limits on the astrophysical coalescence rates of IMBHs with total binary mass 50 ≤ M/M[subscript ⊙] ≤ 450 and component mass ratios of either 1:1 or 4:1. For systems with total mass 100 ≤ M/M[subscript ⊙] ≤ 150, we report a 90% confidence upper limit on the rate of binary IMBH mergers with nonspinning and equal mass components of 6.9 × 10[superscript −8]  Mpc[superscript −3] yr[superscript −1]. We also report a rate upper limit for ringdown waveforms from perturbed IMBHs, radiating 1% of their mass as gravitational waves in the fundamental, ℓ = m = 2, oscillation mode, that is nearly three orders of magnitude more stringent than previous results.
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spelling mit-1721.1/908822022-09-26T11:30:53Z Search for gravitational wave ringdowns from perturbed intermediate mass black holes in LIGO-Virgo data from 2005–2010 Barsotti, Lisa Biscans, Sebastien Bodiya, Timothy Paul Donovan, Frederick J. Essick, Reed Clasey Evans, Matthew J. Fritschel, Peter K. Gras, Slawek Isogai, Tomoki Katsavounidis, Erotokritos Kwee, Patrick Lee, J. Libson, Adam Lynch, Ryan Christopher MacInnis, Myron E. Mason, Kenneth R. Matichard, Fabrice Mavalvala, Nergis Miller, John Mittleman, Richard K. Oelker, Eric Glenn Shoemaker, David H. Tse, Maggie Vaulin, Ruslan Vitale, Salvatore Weiss, Rainer Wipf, C. C. Zhang, Fan Zucker, Michael E. Aggarwal, Nancy,Ph. D.Massachusetts Institute of Technology. Massachusetts Institute of Technology. Department of Physics MIT Kavli Institute for Astrophysics and Space Research Aggarwal, Nancy Barsotti, Lisa Biscans, Sebastien Bodiya, Timothy Paul Donovan, Frederick J. Essick, Reed Clasey Evans, Matthew J. Fritschel, Peter K. Gras, Slawek Isogai, Tomoki Katsavounidis, Erotokritos Kwee, Patrick Lee, J. Libson, Adam Lynch, Ryan Christopher MacInnis, Myron E. Mason, Kenneth R. Matichard, Fabrice Mavalvala, Nergis Miller, John Mittleman, Richard K. Oelker, Eric Glenn Shoemaker, David H. Tse, Maggie Vaulin, Ruslan Vitale, Salvatore Weiss, Rainer Wipf, C. C. Zhang, Fan Zucker, Michael E. We report results from a search for gravitational waves produced by perturbed intermediate mass black holes (IMBH) in data collected by LIGO and Virgo between 2005 and 2010. The search was sensitive to astrophysical sources that produced damped sinusoid gravitational wave signals, also known as ringdowns, with frequency 50 ≤ f[subscript 0]/Hz ≤ 2000 and decay timescale 0.0001 ≲ τ/s ≲ 0.1 characteristic of those produced in mergers of IMBH pairs. No significant gravitational wave candidate was detected. We report upper limits on the astrophysical coalescence rates of IMBHs with total binary mass 50 ≤ M/M[subscript ⊙] ≤ 450 and component mass ratios of either 1:1 or 4:1. For systems with total mass 100 ≤ M/M[subscript ⊙] ≤ 150, we report a 90% confidence upper limit on the rate of binary IMBH mergers with nonspinning and equal mass components of 6.9 × 10[superscript −8]  Mpc[superscript −3] yr[superscript −1]. We also report a rate upper limit for ringdown waveforms from perturbed IMBHs, radiating 1% of their mass as gravitational waves in the fundamental, ℓ = m = 2, oscillation mode, that is nearly three orders of magnitude more stringent than previous results. National Science Foundation (U.S.) United States. National Aeronautics and Space Administration Carnegie Trust David & Lucile Packard Foundation Research Corporation Alfred P. Sloan Foundation 2014-10-10T14:01:23Z 2014-10-10T14:01:23Z 2014-05 2014-03 Article http://purl.org/eprint/type/JournalArticle 1550-7998 1550-2368 http://hdl.handle.net/1721.1/90882 Aasi, J., B. P. Abbott, R. Abbott, T. Abbott, M. R. Abernathy, F. Acernese, K. Ackley, et al. “Search for Gravitational Wave Ringdowns from Perturbed Intermediate Mass Black Holes in LIGO-Virgo Data from 2005–2010.” Phys. Rev. D 89, no. 10 (May 2014). © 2014 American Physical Society https://orcid.org/0000-0002-0026-3877 https://orcid.org/0000-0003-2815-7387 https://orcid.org/0000-0003-0219-9706 https://orcid.org/0000-0001-6550-3045 https://orcid.org/0000-0002-4147-2560 https://orcid.org/0000-0003-1510-4921 https://orcid.org/0000-0001-8459-4499 https://orcid.org/0000-0002-9635-7527 https://orcid.org/0000-0001-8150-7062 https://orcid.org/0000-0002-2544-1596 https://orcid.org/0000-0003-2700-0767 https://orcid.org/0000-0003-1983-3187 https://orcid.org/0000-0002-5163-683X https://orcid.org/0000-0003-2047-3166 https://orcid.org/0000-0001-8196-9267 en_US http://dx.doi.org/10.1103/PhysRevD.89.102006 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. application/pdf American Physical Society American Physical Society
spellingShingle Barsotti, Lisa
Biscans, Sebastien
Bodiya, Timothy Paul
Donovan, Frederick J.
Essick, Reed Clasey
Evans, Matthew J.
Fritschel, Peter K.
Gras, Slawek
Isogai, Tomoki
Katsavounidis, Erotokritos
Kwee, Patrick
Lee, J.
Libson, Adam
Lynch, Ryan Christopher
MacInnis, Myron E.
Mason, Kenneth R.
Matichard, Fabrice
Mavalvala, Nergis
Miller, John
Mittleman, Richard K.
Oelker, Eric Glenn
Shoemaker, David H.
Tse, Maggie
Vaulin, Ruslan
Vitale, Salvatore
Weiss, Rainer
Wipf, C. C.
Zhang, Fan
Zucker, Michael E.
Aggarwal, Nancy,Ph. D.Massachusetts Institute of Technology.
Search for gravitational wave ringdowns from perturbed intermediate mass black holes in LIGO-Virgo data from 2005–2010
title Search for gravitational wave ringdowns from perturbed intermediate mass black holes in LIGO-Virgo data from 2005–2010
title_full Search for gravitational wave ringdowns from perturbed intermediate mass black holes in LIGO-Virgo data from 2005–2010
title_fullStr Search for gravitational wave ringdowns from perturbed intermediate mass black holes in LIGO-Virgo data from 2005–2010
title_full_unstemmed Search for gravitational wave ringdowns from perturbed intermediate mass black holes in LIGO-Virgo data from 2005–2010
title_short Search for gravitational wave ringdowns from perturbed intermediate mass black holes in LIGO-Virgo data from 2005–2010
title_sort search for gravitational wave ringdowns from perturbed intermediate mass black holes in ligo virgo data from 2005 2010
url http://hdl.handle.net/1721.1/90882
https://orcid.org/0000-0002-0026-3877
https://orcid.org/0000-0003-2815-7387
https://orcid.org/0000-0003-0219-9706
https://orcid.org/0000-0001-6550-3045
https://orcid.org/0000-0002-4147-2560
https://orcid.org/0000-0003-1510-4921
https://orcid.org/0000-0001-8459-4499
https://orcid.org/0000-0002-9635-7527
https://orcid.org/0000-0001-8150-7062
https://orcid.org/0000-0002-2544-1596
https://orcid.org/0000-0003-2700-0767
https://orcid.org/0000-0003-1983-3187
https://orcid.org/0000-0002-5163-683X
https://orcid.org/0000-0003-2047-3166
https://orcid.org/0000-0001-8196-9267
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