A Search for Coincident Neutrino Emission from Fast Radio Bursts with Seven Years of IceCube Cascade Events
Artikel i vetenskaplig tidskrift, 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.

Författare

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

Friedrich-Alexander-Universität Erlangen Nurnberg (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, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik

Ruhr-Universität Bochum

J. Beise

Uppsala universitet

C. Bellenghi

Technische Universität München

S. Benzvi

University of Rochester

D. Berley

University of Maryland

E. Bernardini

Università di Padova

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

Karlsruher Institut für Technologie (KIT)

J. Y. Book

Harvard University

C. Boscolo Meneguolo

Università di Padova

S. Böser

Johannes Gutenberg-Universität Mainz

O. Botner

Uppsala universitet

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

Universität 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

Universität Münster

A. Coleman

Uppsala universitet

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 Brüssel (VUB)

P. Correa

Vrije Universiteit Brüssel (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 Brüssel (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 Brüssel (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

Universität Münster

A. Domi

Friedrich-Alexander-Universität Erlangen Nurnberg (FAU)

H. Dujmovic

University of Wisconsin Madison

M. A. Duvernois

University of Wisconsin Madison

T. Ehrhardt

Johannes Gutenberg-Universität Mainz

P. Eller

Technische Universität München

R. Engel

Karlsruher Institut für Technologie (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-Universität zu Berlin

S. Fiedlschuster

Friedrich-Alexander-Universität Erlangen Nurnberg (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-Universität Mainz

P. Fürst

RWTH Aachen University

Astrophysical Journal

0004-637X (ISSN) 1538-4357 (eISSN)

Vol. 946 2 80

Ämneskategorier

Acceleratorfysik och instrumentering

Subatomär fysik

Astronomi, astrofysik och kosmologi

DOI

10.3847/1538-4357/acbea0

Mer information

Senast uppdaterat

2023-05-29