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  4. All-sky search in early O3 LIGO data for continuous gravitational-wave signals from unknown neutron stars in binary systems

All-sky search in early O3 LIGO data for continuous gravitational-wave signals from unknown neutron stars in binary systems

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PhysRevD.103.064017.pdf

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sword-2022-01-25T14:27:07.original.xml (130 B)
Original SWORD entry document
Author(s)
LIGO Scientific Collaboration
•
Virgo Collaboration
•
Barnum, Sam
•
Barsotti, Lisa
•
Biscans, Sebastien
•
Biscoveanu, Sylvia
•
Buikema, Aaron
•
Demos, Nicholas
•
Donovan, Frederick J
•
Eisenstein, Robert Alan
more
Date Issued
2021
Journal
Physical Review D
Publisher
American Physical Society (APS)
Citation
2021. "All-sky search in early O3 LIGO data for continuous gravitational-wave signals from unknown neutron stars in binary systems." Physical Review D, 103 (6).
Version
Final published version
Abstract
Rapidly spinning neutron stars are promising sources of persistent, continuous gravitational waves. Detecting such a signal would allow probing of the physical properties of matter under extreme conditions. A significant fraction of the known pulsar population belongs to binary systems. Searching for unknown neutron stars in binary systems requires specialized algorithms to address unknown orbital frequency modulations. We present a search for continuous gravitational waves emitted by neutron stars in binary systems in early data from the third observing run of the Advanced LIGO and Advanced Virgo detectors using the semicoherent, GPU-accelerated, BinarySkyHough pipeline. The search analyzes the most sensitive frequency band of the LIGO detectors, 50 - 300 Hz. Binary orbital parameters are split into four regions, comprising orbital periods of 3 - 45 days and projected semimajor axes of 2 - 40 light-seconds. No detections are reported. We estimate the sensitivity of the search using simulated continuous wave signals, achieving the most sensitive results to date across the analyzed parameter space.
MIT Department
LIGO (Observatory : Massachusetts Institute of Technology)
MIT Kavli Institute for Astrophysics and Space Research
Massachusetts Institute of Technology. Department of Physics
Terms of Use
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.
Persistent DSpace Link
https://hdl.handle.net/1721.1/139688.2
DOI of Published Version
https://doi.org/10.1103/PHYSREVD.103.064017
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