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https://hdl.handle.net/2440/139211
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Type: | Journal article |
Title: | Limits on Neutrino Emission from GRB 221009A from MeV to PeV Using the IceCube Neutrino Observatory |
Author: | Abbasi, R. Ackermann, M. Adams, J. Agarwalla, S.K. Aggarwal, N. Aguilar, J.A. Ahlers, M. Alameddine, J.M. Amin, N.M. Andeen, K. Anton, G. Argüelles, C. Ashida, Y. Athanasiadou, S. Axani, S.N. Bai, X. Balagopal, A.V. Baricevic, M. Barwick, S.W. Basu, V. et al. |
Citation: | Letters of the Astrophysical Journal, 2023; 946(1):L26-1-L26-10 |
Publisher: | IOP Publishing |
Issue Date: | 2023 |
ISSN: | 2041-8205 2041-8213 |
Statement of Responsibility: | R. Abbasi ... R. T. Burley ... E. G. Carnie-Bronca ... G. H. Collin ... G. C. Hill ... E. J. Roberts ... et al. (IceCube Collaboration) |
Abstract: | Gamma-ray bursts (GRBs) have long been considered a possible source of high-energy neutrinos. While no correlations have yet been detected between high-energy neutrinos and GRBs, the recent observation of GRB 221009A—the brightest GRB observed by Fermi-GBM to date and the first one to be observed above an energy of 10 TeV—provides a unique opportunity to test for hadronic emission. In this paper, we leverage the wide energy range of the IceCube Neutrino Observatory to search for neutrinos from GRB 221009A. We find no significant deviation from background expectation across event samples ranging from MeV to PeV energies, placing stringent upper limits on the neutrino emission from this source. |
Rights: | © 2023. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. |
DOI: | 10.3847/2041-8213/acc077 |
Published version: | http://dx.doi.org/10.3847/2041-8213/acc077 |
Appears in Collections: | Physics publications |
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