4.7 Article

A Search for Neutrino Emission from Fast Radio Bursts with Six Years of IceCube Data

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

  1. USA-U.S. National Science Foundation-Office of Polar Programs
  2. U.S. National Science Foundation-Physics Division
  3. Wisconsin Alumni Research Foundation
  4. Center for High Throughput Computing (CHTC) at the University of WisconsinMadison
  5. Open Science Grid (OSG)
  6. Extreme Science and Engineering Discovery Environment (XSEDE)
  7. U.S. Department of EnergyNational Energy Research Scientific Computing Center
  8. Particle astrophysics research computing center at the University of Maryland
  9. Institute for Cyber-Enabled Research at Michigan State University
  10. Astroparticle physics computational facility at Marquette University
  11. Belgium-Funds for Scientific Research (FRS-FNRS)
  12. Belgium-Funds for Scientific Research (FWO)
  13. FWO Odysseus programme
  14. FWO Big Science programme
  15. Belgian Federal Science Policy Office (Belspo)
  16. Germany-Bundesministerium fur Bildung und Forschung (BMBF)
  17. Deutsche Forschungsgemeinschaft (DFG)
  18. German Excellence Initiative
  19. Helmholtz Alliance for Astroparticle Physics (HAP)
  20. Initiative and Networking Fund of the Helmholtz Association
  21. Deutsches Elektronen Synchrotron (DESY)
  22. High Performance Computing cluster of the RWTH Aachen
  23. Sweden-Swedish Research Council
  24. Swedish Polar Research Secretariat
  25. Swedish National Infrastructure for Computing (SNIC)
  26. Knut and Alice Wallenberg Foundation
  27. Australia-Australian Research Council
  28. Canada-Natural Sciences and Engineering Research Council of Canada
  29. Calcul Qubec
  30. Compute Ontario
  31. Canada Foundation for Innovation
  32. WestGrid
  33. Compute Canada
  34. Denmark-Villum Fonden
  35. Danish National Research Foundation (DNRF)
  36. New Zealand-Marsden Fund
  37. Japan-Japan Society for Promotion of Science (JSPS)
  38. Institute for Global Prominent Research (IGPR) of Chiba University
  39. Korea-National Research Foundation of Korea (NRF)
  40. Switzerland-Swiss National Science Foundation (SNSF)
  41. STFC [ST/P000770/1] Funding Source: UKRI
  42. Direct For Mathematical & Physical Scien
  43. Division Of Physics [1505230, 1505296, 1607199] Funding Source: National Science Foundation
  44. Office of Advanced Cyberinfrastructure (OAC)
  45. Direct For Computer & Info Scie & Enginr [1626251] Funding Source: National Science Foundation

向作者/读者索取更多资源

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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