Detection of a particle shower at the Glashow resonance with IceCube

Publikationstyp:

Zeitschriftenaufsatz

Metadaten:

Autoren

MG Aartsen
R Abbasi
M Ackermann
J Adams
JA Aguilar
M Ahlers
M Ahrens
C Alispach
NM Amin
K Andeen
T Anderson
I Ansseau
G Anton
C Arguelles
J Auffenberg
S Axani
H Bagherpour
X Bai
AV Balagopal
A Barbano
SW Barwick
B Bastian
V Basu
V Baum
S Baur
R Bay
JJ Beatty
K-H Becker
J Becker Tjus
C Bellenghi
S BenZvi
D Berley
E Bernardini
DZ Besson
G Binder
D Bindig
E Blaufuss
S Blot
C Bohm
S Boeser
O Botner
J Boettcher
E Bourbeau
J Bourbeau
F Bradascio
J Braun
S Bron
J Brostean-Kaiser
A Burgman
J Buscher
RS Busse
MA Campana
T Carver
C Chen
E Cheung
D Chirkin
S Choi
BA Clark
K Clark
L Classen
A Coleman
GH Collin
JM Conrad
P Coppin
P Correa
DF Cowen
R Cross
P Dave
C De Clercq
JJ DeLaunay
H Dembinski
K Deoskar
S De Ridder
A Desai
P Desiati
KD de Vries
G de Wasseige
M de With
T DeYoung
S Dharani
A Diaz
JC Diaz-Velez
H Dujmovic
M Dunkman
MA DuVernois
E Dvorak
T Ehrhardt
P Eller
R Engel
PA Evenson
S Fahey
AR Fazely
A Fedynitch
J Felde
AT Fienberg
K Filimonov
C Finley
L Fischer
D Fox
A Franckowiak
E Friedman
A Fritz
TK Gaisser
J Gallagher
E Ganster
S Garrappa
L Gerhardt
A Ghadimi
T Glauch
T Gluesenkamp
A Goldschmidt
JG Gonzalez
S Goswami
D Grant
T Gregoire
Z Griffith
S Griswold
M Guenduez
C Haack
A Hallgren
R Halliday
L Halve
F Halzen
K Hanson
J Hardin
A Haungs
S Hauser
D Hebecker
P Heix
K Helbing
R Hellauer
F Henningsen
S Hickford
J Hignight
C Hill
GC Hill
KD Hoffman
R Hoffmann
T Hoinka
B Hokanson-Fasig
K Hoshina
F Huang
M Huber
T Huber
K Hultqvist
M Huennefeld
R Hussain
S In
N Iovine
A Ishihara
M Jansson
GS Japaridze
M Jeong
BJP Jones
F Jonske
R Joppe
D Kang
W Kang
X Kang
A Kappes
D Kappesser
T Karg
M Karl
A Karle
U Katz
M Kauer
M Kellermann
JL Kelley
A Kheirandish
J Kim
K Kin
T Kintscher
J Kiryluk
T Kittler
SR Klein
R Koirala
H Kolanoski
L Koepke
C Kopper
S Kopper
DJ Koskinen
P Koundal
M Kovacevich
M Kowalski
K Krings
G Krueckl
N Kulacz
N Kurahashi
A Kyriacou
C Lagunas Gualda
JL Lanfranchi
MJ Larson
F Lauber
JP Lazar
K Leonard
A Leszczynska
Y Li
QR Liu
E Lohfink
CJ Lozano Mariscal
L Lu
F Lucarelli
A Ludwig
J Luenemann
W Luszczak
Y Lyu
WY Ma
J Madsen
G Maggi
KBM Mahn
Y Makino
P Mallik
S Mancina
IC Maris
R Maruyama
K Mase
R Maunu
F McNally
K Meagher
M Medici
A Medina
M Meier
S Meighen-Berger
J Merz
J Micallef
D Mockler
G Momente
T Montaruli
RW Moore
R Morse
M Moulai
P Muth
R Naab
R Nagai
U Naumann
J Necker
G Neer
LV Nguyen
H Niederhausen
MU Nisa
SC Nowicki
DR Nygren
A Obertacke Pollmann
M Oehler
A Olivas
E O'Sullivan
H Pandya
DV Pankova
N Park
GK Parker
EN Paudel
P Peiffer
C Perez de Los Heros
S Philippen
D Pieloth
S Pieper
A Pizzuto
M Plum
Y Popovych
A Porcelli
M Prado Rodriguez
PB Price
GT Przybylski
C Raab
A Raissi
M Rameez
L Rauch
K Rawlins
IC Rea
A Rehman
R Reimann
M Relich
M Renschler
G Renzi
E Resconi
S Reusch
W Rhode
M Richman
B Riedel
S Robertson
G Roellinghoff
M Rongen
C Rott
T Ruhe
D Ryckbosch
D Rysewyk Cantu
I Safa
SE Sanchez Herrera
A Sandrock
J Sandroos
M Santander
S Sarkar
S Sarkar
K Satalecka
M Scharf
M Schaufel
H Schieler
P Schlunder
T Schmidt
A Schneider
J Schneider
FG Schroeder
L Schumacher
S Sclafani
D Seckel
S Seunarine
S Shefali
M Silva
B Smithers
R Snihur
J Soedingrekso
D Soldin
M Song
GM Spiczak
C Spiering
J Stachurska
M Stamatikos
T Stanev
R Stein
J Stettner
A Steuer
T Stezelberger
RG Stokstad
NL Strotjohann
T Stuerwald
T Stuttard
GW Sullivan
I Taboada
F Tenholt
S Ter-Antonyan
A Terliuk
S Tilav
K Tollefson
L Tomankova
C Toennis
S Toscano
D Tosi
A Trettin
M Tselengidou
CF Tung
A Turcati
R Turcotte
CF Turley
JP Twagirayezu
B Ty
E Unger
MA Unland Elorrieta
J Vandenbroucke
D van Eijk
N van Eijndhoven
D Vannerom
J van Santen
S Verpoest
M Vraeghe
C Walck
A Wallace
N Wandkowsky
TB Watson
C Weaver
A Weindl
MJ Weiss
J Weldert
C Wendt
J Werthebach
BJ Whelan
N Whitehorn
K Wiebe
CH Wiebusch
DR Williams
M Wolf
TR Wood
K Woschnagg
G Wrede
J Wulff
XW Xu
Y Xu
JP Yanez
S Yoshida
T Yuan
Z Zhang
M Zoecklein

Autoren-URL

https://www.webofscience.com/api/gateway?GWVersion=2&SrcApp=fis-test-1&SrcAuth=WosAPI&KeyUT=WOS:000627422700007&DestLinkType=FullRecord&DestApp=WOS_CPL

DOI

10.1038/s41586-021-03256-1

eISSN

1476-4687

Externe Identifier

Clarivate Analytics Document Solution ID: QU6WY
PubMed Identifier: 33692563

ISSN

0028-0836

Ausgabe der Veröffentlichung

7849

Zeitschrift

NATURE

Paginierung

220 - +

Datum der Veröffentlichung

2021

Status

Published

Titel

Detection of a particle shower at the Glashow resonance with IceCube

Sub types

Article

Ausgabe der Zeitschrift

591

Datenquelle: Web of Science (Lite)

Andere Metadatenquellen:

Autoren

MG Aartsen
R Abbasi
M Ackermann
J Adams
JA Aguilar
M Ahlers
M Ahrens
C Alispach
NM Amin
K Andeen
T Anderson
I Ansseau
G Anton
C Argüelles
J Auffenberg
S Axani
H Bagherpour
X Bai
A Balagopal V.
A Barbano
SW Barwick
B Bastian
V Basu
V Baum
S Baur
R Bay
JJ Beatty
K-H Becker
J Becker Tjus
C Bellenghi
S BenZvi
D Berley
E Bernardini
DZ Besson
G Binder
D Bindig
E Blaufuss
S Blot
C Bohm
S Böser
O Botner
J Böttcher
E Bourbeau
J Bourbeau
F Bradascio
J Braun
S Bron
J Brostean-Kaiser
A Burgman
J Buscher
RS Busse
MA Campana
T Carver
C Chen
E Cheung
D Chirkin
S Choi
BA Clark
K Clark
L Classen
A Coleman
GH Collin
JM Conrad
P Coppin
P Correa
DF Cowen
R Cross
P Dave
C De Clercq
JJ DeLaunay
H Dembinski
K Deoskar
S De Ridder
A Desai
P Desiati
KD de Vries
G de Wasseige
M de With
T DeYoung
S Dharani
A Diaz
JC Díaz-Vélez
H Dujmovic
M Dunkman
MA DuVernois
E Dvorak
T Ehrhardt
P Eller
R Engel
PA Evenson
S Fahey
AR Fazely
A Fedynitch
J Felde
AT Fienberg
K Filimonov
C Finley
L Fischer
D Fox
A Franckowiak
E Friedman
A Fritz
TK Gaisser
J Gallagher
E Ganster
S Garrappa
L Gerhardt
A Ghadimi
T Glauch
T Glüsenkamp
A Goldschmidt
JG Gonzalez
S Goswami
D Grant
T Grégoire
Z Griffith
S Griswold
M Gündüz
C Haack
A Hallgren
R Halliday
L Halve
F Halzen
K Hanson
J Hardin
A Haungs
S Hauser
D Hebecker
P Heix
K Helbing
R Hellauer
F Henningsen
S Hickford
J Hignight
C Hill
GC Hill
KD Hoffman
R Hoffmann
T Hoinka
B Hokanson-Fasig
K Hoshina
F Huang
M Huber
T Huber
K Hultqvist
M Hünnefeld
R Hussain
S In
N Iovine
A Ishihara
M Jansson
GS Japaridze
M Jeong
BJP Jones
F Jonske
R Joppe
D Kang
W Kang
X Kang
A Kappes
D Kappesser
T Karg
M Karl
A Karle
U Katz
M Kauer
M Kellermann
JL Kelley
A Kheirandish
J Kim
K Kin
T Kintscher
J Kiryluk
T Kittler
SR Klein
R Koirala
H Kolanoski
L Köpke
C Kopper
S Kopper
DJ Koskinen
P Koundal
M Kovacevich
M Kowalski
K Krings
G Krückl
N Kulacz
N Kurahashi
A Kyriacou
C Lagunas Gualda
JL Lanfranchi
MJ Larson
F Lauber
JP Lazar
K Leonard
A Leszczyńska
Y Li
QR Liu
E Lohfink
CJ Lozano Mariscal
L Lu
F Lucarelli
A Ludwig
J Lünemann
W Luszczak
Y Lyu
WY Ma
J Madsen
G Maggi
KBM Mahn
Y Makino
P Mallik
S Mancina
IC Mariş
R Maruyama
K Mase
R Maunu
F McNally
K Meagher
M Medici
A Medina
M Meier
S Meighen-Berger
J Merz
J Micallef
D Mockler
G Momenté
T Montaruli
RW Moore
R Morse
M Moulai
P Muth
R Naab
R Nagai
U Naumann
J Necker
G Neer
LV Nguyen
H Niederhausen
MU Nisa
SC Nowicki
DR Nygren
A Obertacke Pollmann
M Oehler
A Olivas
E O’Sullivan
H Pandya
DV Pankova
N Park
GK Parker
EN Paudel
P Peiffer
C Pérez de los Heros
S Philippen
D Pieloth
S Pieper
A Pizzuto
M Plum
Y Popovych
A Porcelli
M Prado Rodriguez
PB Price
GT Przybylski
C Raab
A Raissi
M Rameez
L Rauch
K Rawlins
IC Rea
A Rehman
R Reimann
M Relich
M Renschler
G Renzi
E Resconi
S Reusch
W Rhode
M Richman
B Riedel
S Robertson
G Roellinghoff
M Rongen
C Rott
T Ruhe
D Ryckbosch
D Rysewyk Cantu
I Safa
SE Sanchez Herrera
A Sandrock
J Sandroos
M Santander
S Sarkar
S Sarkar
K Satalecka
M Scharf
M Schaufel
H Schieler
P Schlunder
T Schmidt
A Schneider
J Schneider
FG Schröder
L Schumacher
S Sclafani
D Seckel
S Seunarine
S Shefali
M Silva
B Smithers
R Snihur
J Soedingrekso
D Soldin
M Song
GM Spiczak
C Spiering
J Stachurska
M Stamatikos
T Stanev
R Stein
J Stettner
A Steuer
T Stezelberger
RG Stokstad
NL Strotjohann
T Stürwald
T Stuttard
GW Sullivan
I Taboada
F Tenholt
S Ter-Antonyan
A Terliuk
S Tilav
K Tollefson
L Tomankova
C Tönnis
S Toscano
D Tosi
A Trettin
M Tselengidou
CF Tung
A Turcati
R Turcotte
CF Turley
JP Twagirayezu
B Ty
E Unger
MA Unland Elorrieta
J Vandenbroucke
D van Eijk
N van Eijndhoven
D Vannerom
J van Santen
S Verpoest
M Vraeghe
C Walck
A Wallace
N Wandkowsky
TB Watson
C Weaver
A Weindl
MJ Weiss
J Weldert
C Wendt
J Werthebach
BJ Whelan
N Whitehorn
K Wiebe
CH Wiebusch
DR Williams
M Wolf
TR Wood
K Woschnagg
G Wrede
J Wulff
XW Xu
Y Xu
JP Yanez
S Yoshida
T Yuan
Z Zhang
M Zöcklein

DOI

10.1038/s41586-021-03256-1

eISSN

1476-4687

ISSN

0028-0836

Ausgabe der Veröffentlichung

7849

Zeitschrift

Nature

Sprache

Online publication date

2021

Paginierung

220 - 224

Datum der Veröffentlichung

2021

Status

Published

Herausgeber

Springer Science and Business Media LLC

Herausgeber URL

http://dx.doi.org/10.1038/s41586-021-03256-1

Datum der Datenerfassung

2023

Titel

Detection of a particle shower at the Glashow resonance with IceCube

Ausgabe der Zeitschrift

591

Datenquelle: Crossref

Abstract

The Glashow resonance describes the resonant formation of a W- boson during the interaction of a high-energy electron antineutrino with an electron1, peaking at an antineutrino energy of 6.3 petaelectronvolts (PeV) in the rest frame of the electron. Whereas this energy scale is out of reach for currently operating and future planned particle accelerators, natural astrophysical phenomena are expected to produce antineutrinos with energies beyond the PeV scale. Here we report the detection by the IceCube neutrino observatory of a cascade of high-energy particles (a particle shower) consistent with being created at the Glashow resonance. A shower with an energy of 6.05 ± 0.72 PeV (determined from Cherenkov radiation in the Antarctic Ice Sheet) was measured. Features consistent with the production of secondary muons in the particle shower indicate the hadronic decay of a resonant W- boson, confirm that the source is astrophysical and provide improved directional localization. The evidence of the Glashow resonance suggests the presence of electron antineutrinos in the astrophysical flux, while also providing further validation of the standard model of particle physics. Its unique signature indicates a method of distinguishing neutrinos from antineutrinos, thus providing a way to identify astronomical accelerators that produce neutrinos via hadronuclear or photohadronic interactions, with or without strong magnetic fields. As such, knowledge of both the flavour (that is, electron, muon or tau neutrinos) and charge (neutrino or antineutrino) will facilitate the advancement of neutrino astronomy.

Autoren

IceCube Collaboration

DOI

10.1038/s41586-021-03256-1

eISSN

1476-4687

Externe Identifier

PubMed Identifier: 33692563

Funding acknowledgements

Science and Technology Facilities Council: ST/P000770/1
Villum Fonden: 00018994

Open access

false

ISSN

0028-0836

Ausgabe der Veröffentlichung

7849

Zeitschrift

Nature

Schlüsselwörter

IceCube Collaboration

Sprache

eng

Medium

Print-Electronic

Online publication date

2021

Paginierung

220 - 224

Datum der Veröffentlichung

2021

Status

Published

Datum der Datenerfassung

2021

Titel

Detection of a particle shower at the Glashow resonance with IceCube.

Sub types

Research Support, Non-U.S. Gov't
Research Support, U.S. Gov't, Non-P.H.S.
Journal Article

Ausgabe der Zeitschrift

591

Datenquelle: Europe PubMed Central

Abstract

The Glashow resonance describes the resonant formation of a W- boson during the interaction of a high-energy electron antineutrino with an electron1, peaking at an antineutrino energy of 6.3 petaelectronvolts (PeV) in the rest frame of the electron. Whereas this energy scale is out of reach for currently operating and future planned particle accelerators, natural astrophysical phenomena are expected to produce antineutrinos with energies beyond the PeV scale. Here we report the detection by the IceCube neutrino observatory of a cascade of high-energy particles (a particle shower) consistent with being created at the Glashow resonance. A shower with an energy of 6.05 ± 0.72 PeV (determined from Cherenkov radiation in the Antarctic Ice Sheet) was measured. Features consistent with the production of secondary muons in the particle shower indicate the hadronic decay of a resonant W- boson, confirm that the source is astrophysical and provide improved directional localization. The evidence of the Glashow resonance suggests the presence of electron antineutrinos in the astrophysical flux, while also providing further validation of the standard model of particle physics. Its unique signature indicates a method of distinguishing neutrinos from antineutrinos, thus providing a way to identify astronomical accelerators that produce neutrinos via hadronuclear or photohadronic interactions, with or without strong magnetic fields. As such, knowledge of both the flavour (that is, electron, muon or tau neutrinos) and charge (neutrino or antineutrino) will facilitate the advancement of neutrino astronomy.

Date of acceptance

2021

Autoren

IceCube Collaboration

Autoren-URL

https://www.ncbi.nlm.nih.gov/pubmed/33692563

DOI

10.1038/s41586-021-03256-1

eISSN

1476-4687

Ausgabe der Veröffentlichung

7849

Zeitschrift

Nature

Sprache

eng

Country

England

Paginierung

220 - 224

PII

10.1038/s41586-021-03256-1

Datum der Veröffentlichung

2021

Status

Published

Datum, an dem der Datensatz öffentlich gemacht wurde

2021

Titel

Detection of a particle shower at the Glashow resonance with IceCube.

Sub types

Journal Article
Research Support, Non-U.S. Gov't
Research Support, U.S. Gov't, Non-P.H.S.

Ausgabe der Zeitschrift

591

Datenquelle: PubMed

Beziehungen:

Eigentum von

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Detection of a particle shower at the Glashow resonance with IceCube

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