A Search for Coincident Neutrino Emission from Fast Radio Bursts with Seven Years of IceCube Cascade Events
Journal article, 2023
This paper presents the results of a search for neutrinos that are spatially and temporally coincident with 22 unique, nonrepeating fast radio bursts (FRBs) and one repeating FRB (FRB 121102). FRBs are a rapidly growing class of Galactic and extragalactic astrophysical objects that are considered a potential source of high-energy neutrinos. The IceCube Neutrino Observatory's previous FRB analyses have solely used track events. This search utilizes seven years of IceCube cascade events which are statistically independent of track events. This event selection allows probing of a longer range of extended timescales due to the low background rate. No statistically significant clustering of neutrinos was observed. Upper limits are set on the time-integrated neutrino flux emitted by FRBs for a range of extended time windows.
Author
R. Abbasi
Loyola University of Chicago
M. Ackermann
Deutsches Elektronen-Synchrotron (DESY)
J. Adams
University of Canterbury
S. K. Agarwalla
Institute of Physics Bhubaneswar
University of Wisconsin Madison
J. A. Aguilar
Université libre de Bruxelles (ULB)
M. Ahlers
Niels Bohr Institute
J. M. Alameddine
Technische Universität Dortmund
N. M. Amin
University of Delaware
K. Andeen
Marquette University
G. Anton
University of Erlangen-Nuremberg (FAU)
C. Argüelles
Harvard University
Y. Ashida
University of Wisconsin Madison
S. Athanasiadou
Deutsches Elektronen-Synchrotron (DESY)
S. N. Axani
University of Delaware
X. Bai
South Dakota School of Mines & Technology
A. V. Balagopal
University of Wisconsin Madison
M. Baricevic
University of Wisconsin Madison
S. W. Barwick
University of California at Irvine (UCI)
V. Basu
University of Wisconsin Madison
R. Bay
University of California
J. J. Beatty
Ohio State University
K. H. Becker
Bergische Universität Wuppertal
Julia Tjus
Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics
Ruhr-Universität Bochum
J. Beise
Uppsala University
C. Bellenghi
Technical University of Munich
S. Benzvi
University of Rochester
D. Berley
University of Maryland
E. Bernardini
University of Padua
D. Z. Besson
University of Kansas
G. Binder
Lawrence Berkeley National Laboratory
University of California
D. Bindig
Bergische Universität Wuppertal
E. Blaufuss
University of Maryland
S. Blot
Deutsches Elektronen-Synchrotron (DESY)
F. Bontempo
Karlsruhe Institute of Technology (KIT)
J. Y. Book
Harvard University
C. Boscolo Meneguolo
University of Padua
S. Böser
Johannes Gutenberg University Mainz
O. Botner
Uppsala University
J. Böttcher
RWTH Aachen University
E. Bourbeau
Niels Bohr Institute
J. Braun
University of Wisconsin Madison
B. Brinson
Georgia Institute of Technology
J. Brostean-Kaiser
Deutsches Elektronen-Synchrotron (DESY)
R. T. Burley
University of Adelaide
R. S. Busse
University of Münster
D. Butterfield
University of Wisconsin Madison
M. A. Campana
Drexel University
K. Carloni
Harvard University
E. G. Carnie-Bronca
University of Adelaide
S. Chattopadhyay
Institute of Physics Bhubaneswar
University of Wisconsin Madison
C. Chen
Georgia Institute of Technology
Z. Chen
Stony Brook University
D. Chirkin
University of Wisconsin Madison
S. Choi
Sungkyunkwan University
B. A. Clark
University of Maryland
L. Classen
University of Münster
A. Coleman
Uppsala University
G. H. Collin
Massachusetts Institute of Technology (MIT)
A. Connolly
Ohio State University
J. M. Conrad
Massachusetts Institute of Technology (MIT)
P. Coppin
Vrije Universiteit Brussel (VUB)
P. Correa
Vrije Universiteit Brussel (VUB)
S. Countryman
Columbia University
D. F. Cowen
Eberly College of Science
Pennsylvania State University
P. Dave
Georgia Institute of Technology
C. De Clercq
Vrije Universiteit Brussel (VUB)
J. J. Delaunay
University of Alabama
D. Delgado López
Harvard University
H. Dembinski
University of Delaware
K. Deoskar
Oskar Klein Centre
A. Desai
University of Wisconsin Madison
P. Desiati
University of Wisconsin Madison
K. D. De Vries
Vrije Universiteit Brussel (VUB)
G. De Wasseige
Universite catholique de Louvain
T. Deyoung
Michigan State University
A. Diaz
Massachusetts Institute of Technology (MIT)
J. C. Díaz-Vélez
University of Wisconsin Madison
M. Dittmer
University of Münster
A. Domi
University of Erlangen-Nuremberg (FAU)
H. Dujmovic
University of Wisconsin Madison
M. A. Duvernois
University of Wisconsin Madison
T. Ehrhardt
Johannes Gutenberg University Mainz
P. Eller
Technical University of Munich
R. Engel
Karlsruhe Institute of Technology (KIT)
H. Erpenbeck
University of Wisconsin Madison
J. Evans
University of Maryland
P. A. Evenson
University of Delaware
K. L. Fan
University of Maryland
K. Fang
University of Wisconsin Madison
A. R. Fazely
Southern University and A&M College
A. Fedynitch
Academia Sinica
N. Feigl
Humboldt University of Berlin
S. Fiedlschuster
University of Erlangen-Nuremberg (FAU)
C. Finley
Oskar Klein Centre
L. Fischer
Deutsches Elektronen-Synchrotron (DESY)
D. Fox
Pennsylvania State University
A. Franckowiak
Ruhr-Universität Bochum
E. Friedman
University of Maryland
A. Fritz
Johannes Gutenberg University Mainz
P. Fürst
RWTH Aachen University
Astrophysical Journal
0004-637X (ISSN) 1538-4357 (eISSN)
Vol. 946 2 80Subject Categories
Accelerator Physics and Instrumentation
Subatomic Physics
Astronomy, Astrophysics and Cosmology
DOI
10.3847/1538-4357/acbea0