Search for Extremely-High-Energy Neutrinos and First Constraints on the Ultrahigh-Energy Cosmic-Ray Proton Fraction with IceCube
Artikel i vetenskaplig tidskrift, 2025
We present a search for the diffuse extremely-high-energy neutrino flux using 12.6 years of IceCube data. The nonobservation of neutrinos with energies well above 10 PeV constrains the all-flavor neutrino flux at 1018 eV to a level of E2φνe+νμ+ντ≃10-8 GeV cm-2 s-1 sr-1, the most stringent limit to date. Using these data, we constrain the proton fraction of ultrahigh-energy cosmic rays (UHECRs) above ≃30 EeV to be ≲70% (at 90% CL) if the cosmological evolution of the sources is comparable to or stronger than the star formation rate. This is the first result to disfavor the "proton-only"hypothesis for UHECR in this evolution regime using neutrino data. This result complements direct air-shower measurements by being insensitive to uncertainties associated with hadronic interaction models. We also evaluate the tension between IceCube-s nonobservation and the ∼200 PeV KM3NeT neutrino candidate (KM3-230213A), finding it to be ∼2.9σ based on a joint-livetime fit between neutrino datasets.
Författare
R. Abbasi
Loyola University of Chicago
M. Ackermann
Deutsches Elektronen-Synchrotron (DESY)
J. Adams
University of Canterbury
S. K. Agarwalla
University of Wisconsin Madison
Institute of Physics Bhubaneswar
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
C. Argüelles
Harvard University
Y. Ashida
University of Utah
S. Athanasiadou
Deutsches Elektronen-Synchrotron (DESY)
S. N. Axani
University of Delaware
R. Babu
Michigan State University
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
S. Bash
Technische Universität München
V. Basu
University of Wisconsin Madison
R. Bay
University of California
J.J. Beatty
Ohio State University
Julia Tjus
Ruhr-Universität Bochum
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
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
E. Blaufuss
University of Maryland
L. Bloom
University of Alabama
S. Blot
Deutsches Elektronen-Synchrotron (DESY)
F. Bontempo
Karlsruher Institut für Technologie (KIT)
J.Y. Book Motzkin
Harvard University
C. Boscolo Meneguolo
Università di Padova
S. Böser
Johannes Gutenberg-Universität Mainz
O. Botner
Uppsala universitet
J. Böttcher
RWTH Aachen University
J. Braun
University of Wisconsin Madison
B. Brinson
Georgia Institute of Technology
Z. Brisson-Tsavoussis
Queen's University
J. Brostean-Kaiser
Deutsches Elektronen-Synchrotron (DESY)
L. Brusa
RWTH Aachen University
R. T. Burley
University of Adelaide
D. Butterfield
University of Wisconsin Madison
M.A. Campana
Drexel University
I. Caracas
Johannes Gutenberg-Universität Mainz
K. Carloni
Harvard University
J. Carpio
University of Nevada, Las Vegas
S. Chattopadhyay
Institute of Physics Bhubaneswar
University of Wisconsin Madison
N. Chau
Université libre de Bruxelles (ULB)
Z. Chen
Stony Brook University
D. Chirkin
University of Wisconsin Madison
S. Choi
Sungkyunkwan University
B.A. Clark
University of Maryland
A. Coleman
Uppsala universitet
P. Coleman
RWTH Aachen University
G.H. Collin
Massachusetts Institute of Technology (MIT)
A. Connolly
Ohio State University
J.M. Conrad
Massachusetts Institute of Technology (MIT)
R. Corley
University of Utah
D. F. Cowen
Pennsylvania State University
Eberly College of Science
C. De Clercq
Vrije Universiteit Brüssel (VUB)
J.J. Delaunay
University of Alabama
D. Delgado
Harvard University
S. Deng
RWTH Aachen University
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
P. Dierichs
RWTH Aachen University
M. Dittmer
Universität Münster
A. Domi
Friedrich-Alexander-Universität Erlangen Nurnberg (FAU)
L. Draper
University of Utah
H. Dujmovic
University of Wisconsin Madison
D. Durnford
University of Alberta
K. Dutta
Johannes Gutenberg-Universität Mainz
M. A. Duvernois
University of Wisconsin Madison
T. Ehrhardt
Johannes Gutenberg-Universität Mainz
L. Eidenschink
Technische Universität München
A. Eimer
Friedrich-Alexander-Universität Erlangen Nurnberg (FAU)
P. Eller
Technische Universität München
E. Ellinger
Bergische Universität Wuppertal
S. El Mentawi
RWTH Aachen University
D. Elsaesser
Technische Universität Dortmund
R. Engel
Karlsruher Institut für Technologie (KIT)
H. Erpenbeck
University of Wisconsin Madison
W. Esmail
Universität Münster
J. Evans
University of Maryland
P.A. Evenson
University of Delaware
K.L. Fan
University of Maryland
K. Fang
University of Wisconsin Madison
K. Farrag
Chiba University
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)
Physical Review Letters
0031-9007 (ISSN) 1079-7114 (eISSN)
Vol. 135 3 031001Ämneskategorier (SSIF 2025)
Astronomi, astrofysik och kosmologi
Subatomär fysik
DOI
10.1103/PhysRevLett.135.031001