A search for neutrinos from fast radio bursts with IceCube
arXiv:1611.03062 · doi:10.3847/1538-4357/aa7e28
Abstract
We present a search for neutrinos in coincidence in time and direction with four fast radio bursts (FRBs) detected by the Parkes and Green Bank radio telescopes during the first year of operation of the complete IceCube Neutrino Observatory (May 2011 through May 2012). The neutrino sample consists of 138,322 muon neutrino candidate events, which are dominated by atmospheric neutrinos and muons but also contain an astrophysical neutrino component. Considering only neutrinos detected on the same day as each FRB, zero IceCube events were found to be compatible with the FRB directions within the estimated 99\% error radius of the neutrino directions. Based on the non-detection, we present the first upper limits on the neutrino fluence from fast radio bursts.
v2: updated to match version published in ApJ (now with discussion of long term outlook and comparison to diffuse astrophysical neutrino flux)
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Cited by in corpus (12)
- Active Galactic Nuclei and the Origin of IceCube's Diffuse Neutrino Flux
- Revisiting AGN as the Source of IceCube's Diffuse Neutrino Flux
- A Search for Neutrino Emission from Fast Radio Bursts with Six Years of IceCube Data
- Multiwavelength observations of Fast Radio Bursts
- A Search for MeV to TeV Neutrinos from Fast Radio Bursts with IceCube
- Fermi-LAT counterparts of IceCube neutrinos above 100 TeV
- Using High-Energy Neutrinos As Cosmic Magnetometers
- Search for high-energy neutrinos in coincidence with Fast Radio Bursts with the ANTARES neutrino telescope
- Time-integrated constraint on neutrino flux of CHIME fast radio burst sources with 10-year IceCube point-source data
- A test of spatial coincidence between CHIME FRBs and IceCube TeV energy neutrinos
- First Search for High-Energy Neutrino Emission from Galaxy Mergers
- Search for Low-Energy Signals from Fast Radio Bursts with the Borexino Detector