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Multi-messenger Astronomy of Gravitational-wave Sources with Flexible Wide-area Radio Transient Surveys

Yancey, Cregg C. and Bear, Brandon E. and Akukwe, Bernadine and Chen, Kevin and Dowell, Jayce and Gough, Jonathan D. and Kanner, Jonah and Kavic, Michael and Obenberger, Kenneth and Shawhan, Peter and Simonetti, John H. and Taylor, Gregory B. and Tsai, Jr-Wei (2015) Multi-messenger Astronomy of Gravitational-wave Sources with Flexible Wide-area Radio Transient Surveys. Astrophysical Journal, 812 (2). Art. No. 168. ISSN 0004-637X. http://resolver.caltech.edu/CaltechAUTHORS:20151218-102211138

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Abstract

We explore opportunities for multi-messenger astronomy using gravitational waves (GWs) and prompt, transient low-frequency radio emission to study highly energetic astrophysical events. We review the literature on possible sources of correlated emission of GWs and radio transients, highlighting proposed mechanisms that lead to a short-duration, high-flux radio pulse originating from the merger of two neutron stars or from a superconducting cosmic string cusp. We discuss the detection prospects for each of these mechanisms by low-frequency dipole array instruments such as LWA1, the Low Frequency Array and the Murchison Widefield Array. We find that a broad range of models may be tested by searching for radio pulses that, when de-dispersed, are temporally and spatially coincident with a LIGO/Virgo GW trigger within a ~30 s time window and ~200–500 deg^2 sky region. We consider various possible observing strategies and discuss their advantages and disadvantages. Uniquely, for low-frequency radio arrays, dispersion can delay the radio pulse until after low-latency GW data analysis has identified and reported an event candidate, enabling a prompt radio signal to be captured by a deliberately targeted beam. If neutron star mergers do have detectable prompt radio emissions, a coincident search with the GW detector network and low-frequency radio arrays could increase the LIGO/Virgo effective search volume by up to a factor of ~2. For some models, we also map the parameter space that may be constrained by non-detections.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0004-637X/812/2/168DOIArticle
http://iopscience.iop.org/article/10.1088/0004-637X/812/2/168/metaPublisherArticle
ORCID:
AuthorORCID
Kanner, Jonah0000-0001-8115-0577
Additional Information:© 2015. The American Astronomical Society. Received 2015 August 6; accepted 2015 September 16; published 2015 October 20. We would like to thank Sean Cutchin for insightful comments and shared knowledge. We would like to acknowledge the funding support provided by the U.S. National Science Foundation through grants PHY-1068549 and PHY-1404121, as well as Cooperative Agreement PHY-0757058.
Group:LIGO
Funders:
Funding AgencyGrant Number
NSFPHY-1068549
NSFPHY-1404121
NSFPHY-0757058
Subject Keywords:gravitational waves – methods: observational – telescopes
Record Number:CaltechAUTHORS:20151218-102211138
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20151218-102211138
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:63065
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:18 Dec 2015 23:40
Last Modified:06 Oct 2017 18:28

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