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Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube
Name
Albert_2019_ApJ_870_134.pdf
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1.31 MB
Format
Adobe PDF
Checksum (MD5)
9a1e4e1cf428e22697e5b51cfe11b40e
Date Issued
2019
Journal
Astrophysical Journal
Publisher
American Astronomical Society
Citation
Albert, A., M. André, M. Anghinolfi, M. Ardid, J.-J. Aubert, J. Aublin, T. Avgitas, et al. “Search for Multimessenger Sources of Gravitational Waves and High-Energy Neutrinos with Advanced LIGO During Its First Observing Run, ANTARES, and IceCube.” The Astrophysical Journal 870, no. 2 (January 16, 2019): 134. doi:10.3847/1538-4357/aaf21d.
Version
Final published version
Abstract
© 2019. The American Astronomical Society.. Astrophysical sources of gravitational waves, such as binary neutron star and black hole mergers or core-collapse supernovae, can drive relativistic outflows, giving rise to non-thermal high-energy emission. High-energy neutrinos are signatures of such outflows. The detection of gravitational waves and high-energy neutrinos from common sources could help establish the connection between the dynamics of the progenitor and the properties of the outflow. We searched for associated emission of gravitational waves and high-energy neutrinos from astrophysical transients with minimal assumptions using data from Advanced LIGO from its first observing run O1, and data from the Antares and IceCube neutrino observatories from the same time period. We focused on candidate events whose astrophysical origins could not be determined from a single messenger. We found no significant coincident candidate, which we used to constrain the rate density of astrophysical sources dependent on their gravitational-wave and neutrino emission processes.
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Creative Commons Attribution 3.0 unported license
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DOI of Published Version
http://dx.doi.org/10.3847/1538-4357/aaf21d