All-sky search for short gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run
After the detection of gravitational waves from compact binary coalescences, the search for transient gravitational-wave signals with less well-defined waveforms for which matched filtering is not well-suited is one of the frontiers for gravitational-wave astronomy. Broadly classified into "...
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| Other Authors: | |
| Format: | Article |
| Language: | English |
| Published: |
American Physical Society (APS)
2022
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| Online Access: | https://hdl.handle.net/1721.1/142164 |
| _version_ | 1826193064652177408 |
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| author | Mavalvala, Nergis |
| author2 | LIGO (Observatory : Massachusetts Institute of Technology) |
| author_facet | LIGO (Observatory : Massachusetts Institute of Technology) Mavalvala, Nergis |
| author_sort | Mavalvala, Nergis |
| collection | MIT |
| description | After the detection of gravitational waves from compact binary coalescences,
the search for transient gravitational-wave signals with less well-defined
waveforms for which matched filtering is not well-suited is one of the
frontiers for gravitational-wave astronomy. Broadly classified into "short" $
\lesssim 1~$\,s and "long" $ \gtrsim 1~$\,s duration signals, these signals are
expected from a variety of astrophysical processes, including non-axisymmetric
deformations in magnetars or eccentric binary black hole coalescences. In this
work, we present a search for long-duration gravitational-wave transients from
Advanced LIGO and Advanced Virgo's third observing run from April 2019 to March
2020. For this search, we use minimal assumptions for the sky location, event
time, waveform morphology, and duration of the source. The search covers the
range of $2~\text{--}~ 500$~s in duration and a frequency band of $24 - 2048$
Hz. We find no significant triggers within this parameter space; we report
sensitivity limits on the signal strength of gravitational waves characterized
by the root-sum-square amplitude $h_{\mathrm{rss}}$ as a function of waveform
morphology. These $h_{\mathrm{rss}}$ limits improve upon the results from the
second observing run by an average factor of 1.8. |
| first_indexed | 2024-09-23T09:33:32Z |
| format | Article |
| id | mit-1721.1/142164 |
| institution | Massachusetts Institute of Technology |
| language | English |
| last_indexed | 2024-09-23T09:33:32Z |
| publishDate | 2022 |
| publisher | American Physical Society (APS) |
| record_format | dspace |
| spelling | mit-1721.1/1421642023-12-20T17:46:56Z All-sky search for short gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run Mavalvala, Nergis LIGO (Observatory : Massachusetts Institute of Technology) After the detection of gravitational waves from compact binary coalescences, the search for transient gravitational-wave signals with less well-defined waveforms for which matched filtering is not well-suited is one of the frontiers for gravitational-wave astronomy. Broadly classified into "short" $ \lesssim 1~$\,s and "long" $ \gtrsim 1~$\,s duration signals, these signals are expected from a variety of astrophysical processes, including non-axisymmetric deformations in magnetars or eccentric binary black hole coalescences. In this work, we present a search for long-duration gravitational-wave transients from Advanced LIGO and Advanced Virgo's third observing run from April 2019 to March 2020. For this search, we use minimal assumptions for the sky location, event time, waveform morphology, and duration of the source. The search covers the range of $2~\text{--}~ 500$~s in duration and a frequency band of $24 - 2048$ Hz. We find no significant triggers within this parameter space; we report sensitivity limits on the signal strength of gravitational waves characterized by the root-sum-square amplitude $h_{\mathrm{rss}}$ as a function of waveform morphology. These $h_{\mathrm{rss}}$ limits improve upon the results from the second observing run by an average factor of 1.8. 2022-04-28T12:42:42Z 2022-04-28T12:42:42Z 2021 2022-04-28T12:28:30Z Article http://purl.org/eprint/type/JournalArticle https://hdl.handle.net/1721.1/142164 Mavalvala, Nergis. 2021. "All-sky search for short gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run." Physical Review D, 104 (12). en 10.1103/PHYSREVD.104.122004 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 (APS) APS |
| spellingShingle | Mavalvala, Nergis All-sky search for short gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run |
| title | All-sky search for short gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run |
| title_full | All-sky search for short gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run |
| title_fullStr | All-sky search for short gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run |
| title_full_unstemmed | All-sky search for short gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run |
| title_short | All-sky search for short gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run |
| title_sort | all sky search for short gravitational wave bursts in the third advanced ligo and advanced virgo run |
| url | https://hdl.handle.net/1721.1/142164 |
| work_keys_str_mv | AT mavalvalanergis allskysearchforshortgravitationalwaveburstsinthethirdadvancedligoandadvancedvirgorun |