dc.contributor.author | LIGO Scientific Collaboration | en |
dc.contributor.author | Virgo Collaboration | en |
dc.contributor.author | Aasi, J. | |
dc.contributor.author | Maglione, C. | |
dc.contributor.author | Quiroga, C. | |
dc.date.accessioned | 2021-09-14T22:49:43Z | |
dc.date.available | 2021-09-14T22:49:43Z | |
dc.date.issued | 2014 | |
dc.identifier.issn | 1550-2368 | |
dc.identifier.uri | http://hdl.handle.net/11086/20313 | |
dc.identifier.uri | https://arxiv.org/abs/1403.5306v2 | |
dc.identifier.uri | De la versión publicada: https://doi.org/10.1103/PhysRevD.89.102006 | |
dc.description | Paper producido por "The LIGO Scientific Collaboration and the Virgo Collaboration". (En el registro se mencionan solo algunos autores de las decenas de personas que participan). | es |
dc.description | Journal reference: Phys. Rev. D 89, 102006 (2014) | |
dc.description.abstract | 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≤f0/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⊙≤450 and component mass ratios of either 1:1 or 4:1. For systems with total mass 100≤M/M⊙≤150, we report a 90%-confidence upper limit on the rate of binary IMBH mergers with non-spinning and equal mass components of 6.9×10−8Mpc−3yr−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. | en |
dc.format.medium | Impreso; Electrónico y/o Digital | |
dc.language.iso | eng | es |
dc.rights | Attribution-NonCommercial-NoDerivatives 4.0 International | * |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/4.0/ | * |
dc.subject | Gravitational wave | en |
dc.subject | General Relativity | en |
dc.subject | Quantum Cosmology | en |
dc.title | Search for gravitational wave ringdowns from perturbed intermediate mass black holes in LIGO-Virgo data from 2005-2010 | en |
dc.type | article | es |
dc.description.version | submittedVersion | es |
dc.description.fil | Fil: Aasi, J. LIGO. California Institute of Technology; Estados Unidos de América. | es |
dc.description.fil | Fil: Maglione, C. Argentinian Gravitational Wave Group; Argentina. | es |
dc.description.fil | Fil: Quiroga, C. Argentinian Gravitational Wave Group; Argentina. | es |
dc.journal.country | Estados Unidos | es |
dc.journal.editorial | American Physical Society | es |
dc.journal.title | Phys. Rev. D | es |
dc.journal.volume | 89 | es |
dc.description.field | Física de Partículas y Campos | |