期刊
ASTROPHYSICAL JOURNAL
卷 857, 期 2, 页码 -出版社
IOP Publishing Ltd
DOI: 10.3847/1538-4357/aab4f8
关键词
astroparticle physics; cosmic rays; elementary particles; neutrinos; radiation mechanisms: non-thermal
资金
- USA-U.S. National Science Foundation-Office of Polar Programs
- U.S. National Science Foundation-Physics Division
- Wisconsin Alumni Research Foundation
- Center for High Throughput Computing (CHTC) at the University of WisconsinMadison
- Open Science Grid (OSG)
- Extreme Science and Engineering Discovery Environment (XSEDE)
- U.S. Department of EnergyNational Energy Research Scientific Computing Center
- Particle astrophysics research computing center at the University of Maryland
- Institute for Cyber-Enabled Research at Michigan State University
- Astroparticle physics computational facility at Marquette University
- Belgium-Funds for Scientific Research (FRS-FNRS)
- Belgium-Funds for Scientific Research (FWO)
- FWO Odysseus programme
- FWO Big Science programme
- Belgian Federal Science Policy Office (Belspo)
- Germany-Bundesministerium fur Bildung und Forschung (BMBF)
- Deutsche Forschungsgemeinschaft (DFG)
- German Excellence Initiative
- Helmholtz Alliance for Astroparticle Physics (HAP)
- Initiative and Networking Fund of the Helmholtz Association
- Deutsches Elektronen Synchrotron (DESY)
- High Performance Computing cluster of the RWTH Aachen
- Sweden-Swedish Research Council
- Swedish Polar Research Secretariat
- Swedish National Infrastructure for Computing (SNIC)
- Knut and Alice Wallenberg Foundation
- Australia-Australian Research Council
- Canada-Natural Sciences and Engineering Research Council of Canada
- Calcul Qubec
- Compute Ontario
- Canada Foundation for Innovation
- WestGrid
- Compute Canada
- Denmark-Villum Fonden
- Danish National Research Foundation (DNRF)
- New Zealand-Marsden Fund
- Japan-Japan Society for Promotion of Science (JSPS)
- Institute for Global Prominent Research (IGPR) of Chiba University
- Korea-National Research Foundation of Korea (NRF)
- Switzerland-Swiss National Science Foundation (SNSF)
- STFC [ST/P000770/1] Funding Source: UKRI
- Direct For Mathematical & Physical Scien
- Division Of Physics [1505230, 1505296, 1607199] Funding Source: National Science Foundation
- Office of Advanced Cyberinfrastructure (OAC)
- Direct For Computer & Info Scie & Enginr [1626251] Funding Source: National Science Foundation
We present a search for coincidence between IceCube TeV neutrinos and fast radio bursts (FRBs). During the search period from 2010 May 31 to 2016 May 12, a total of 29 FRBs with 13 unique locations have been detected in the whole sky. An unbinned maximum likelihood method was used to search for spatial and temporal coincidence between neutrinos and FRBs in expanding time windows, in both the northern and southern hemispheres. No significant correlation was found in six years of IceCube data. Therefore, we set upper limits on neutrino fluence emitted by FRBs as a function of time window duration. We set the most stringent limit obtained to date on neutrino fluence from FRBs with an E-2 energy spectrum assumed, which is 0.0021 GeV cm(-2) per burst for emission timescales up to similar to 10(2) s from the northern hemisphere stacking search.
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