Observation and Characterization of a Cosmic Muon Neutrino Flux from the Northern Hemisphere using six years of IceCube data
- Publikationstyp:
- Zeitschriftenaufsatz
- Metadaten:
-
- Autoren
- MG Aartsen
- K Abraham
- M Ackermann
- J Adams
- JA Aguilar
- M Ahlers
- M Ahrens
- D Altmann
- K Andeen
- T Anderson
- I Ansseau
- G Anton
- M Archinger
- C Argueelles
- J Auffenberg
- S Axani
- X Bai
- SW Barwick
- V Baum
- R Bay
- JJ Beatty
- J Becker Tjus
- K-H Becker
- S Benzvi
- P Berghaus
- D Berley
- E Bernardini
- A Bernhard
- DZ Besson
- G Binder
- D Bindig
- M Bissok
- E Blaufuss
- S Blot
- C Bohm
- M Boerner
- F Bos
- D Bose
- S Boeser
- O Botner
- J Braun
- L Brayeur
- H-P Bretz
- A Burgman
- T Carver
- M Casier
- E Cheung
- D Chirkin
- A Christov
- K Clark
- L Classen
- S Coenders
- GH Collin
- JM Conrad
- DF Cowen
- R Cross
- M Day
- JPAM de Andre
- C De Clercq
- E del Pino Rosendo
- H Dembinski
- S De Ridder
- P Desiati
- KD de Vries
- G de Wasseige
- M de With
- T DeYoung
- JC Diaz-Velez
- V di Lorenzo
- H Dujmovic
- JP Dumm
- M Dunkman
- B Eberhardt
- T Ehrhardt
- B Eichmann
- P Eller
- S Euler
- PA Evenson
- S Fahey
- AR Fazely
- J Feintzeig
- J Felde
- K Filimonov
- C Finley
- S Flis
- C-C Foesig
- A Franckowiak
- E Friedman
- T Fuchs
- TK Gaisser
- J Gallagher
- L Gerhardt
- K Ghorbani
- W Giang
- L Gladstone
- M Glagla
- T Gluesenkamp
- A Goldschmidt
- G Golup
- JG Gonzalez
- D Grant
- Z Griffith
- C Haack
- A Haj Ismail
- A Hallgren
- F Halzen
- E Hansen
- B Hansmann
- T Hansmann
- K Hanson
- D Hebecker
- D Heereman
- K Helbing
- R Hellauer
- S Hickford
- J Hignight
- GC Hill
- KD Hoffman
- R Hoffmann
- K Holzapfel
- K Hoshina
- F Huang
- M Huber
- K Hultqvist
- S In
- A Ishihara
- E Jacobi
- GS Japaridze
- M Jeong
- K Jero
- BJP Jones
- M Jurkovic
- A Kappes
- T Karg
- A Karle
- U Katz
- M Kauer
- A Keivani
- JL Kelley
- J Kemp
- A Kheirandish
- M Kim
- T Kintscher
- J Kiryluk
- T Kittler
- SR Klein
- G Kohnen
- R Koirala
- H Kolanoski
- R Konietz
- L Koepke
- C Kopper
- S Kopper
- DJ Koskinen
- M Kowalski
- K Krings
- M Kroll
- G Krueckl
- C Krueger
- J Kunnen
- S Kunwar
- N Kurahashi
- T Kuwabara
- M Labare
- JL Lanfranchi
- MJ Larson
- F Lauber
- D Lennarz
- M Lesiak-Bzdak
- M Leuermann
- J Leuner
- L Lu
- J Luenemann
- J Madsen
- G Maggi
- KBM Mahn
- S Mancina
- M Mandelartz
- R Maruyama
- K Mase
- R Maunu
- F McNally
- K Meagher
- M Medici
- M Meier
- A Meli
- T Menne
- G Merino
- T Meures
- S Miarecki
- L Mohrmann
- T Montaruli
- M Moulai
- R Nahnhauer
- U Naumann
- G Neer
- H Niederhausen
- SC Nowicki
- DR Nygren
- A Obertacke Pollmann
- A Olivas
- A O'Murchadha
- T Palczewski
- H Pandya
- DV Pankova
- P Peiffer
- Oe Penek
- JA Pepper
- C Perez de los Heros
- D Pieloth
- E Pinat
- PB Price
- GT Przybylski
- M Quinnan
- C Raab
- L Raedel
- M Rameez
- K Rawlins
- R Reimann
- B Relethford
- M Relich
- E Resconi
- W Rhode
- M Richman
- B Riedel
- S Robertson
- M Rongen
- C Rott
- T Ruhe
- D Ryckbosch
- D Rysewyk
- L Sabbatini
- SE Sanchez Herrera
- A Sandrock
- J Sandroos
- S Sarkar
- K Satalecka
- M Schimp
- P Schlunder
- T Schmidt
- S Schoenen
- S Schoeneberg
- L Schumacher
- D Seckel
- S Seunarine
- D Soldin
- M Song
- GM Spiczak
- C Spiering
- M Stahlberg
- T Stanev
- A Stasik
- A Steuer
- T Stezelberger
- RG Stokstad
- A Stoessl
- R Stroem
- NL Strotjohann
- GW Sullivan
- M Sutherland
- H Taavola
- I Taboada
- J Tatar
- F Tenholt
- S Ter-Antonyan
- A Terliuk
- G Tesic
- S Tilav
- PA Toale
- MN Tobin
- S Toscano
- D Tosi
- M Tselengidou
- A Turcati
- E Unger
- M Usner
- J Vandenbroucke
- N van Eijndhoven
- S Vanheule
- M van Rossem
- J van Santen
- J Veenkamp
- M Vehring
- M Voge
- M Vraeghe
- C Walck
- A Wallace
- M Wallraff
- N Wandkowsky
- Ch Weaver
- MJ Weiss
- C Wendt
- S Westerhoff
- BJ Whelan
- S Wickmann
- K Wiebe
- CH Wiebusch
- L Wille
- DR Williams
- L Wills
- M Wolf
- TR Wood
- E Woolsey
- K Woschnagg
- DL Xu
- XW Xu
- Y Xu
- JP Yanez
- G Yodh
- S Yoshida
- M Zoll
- Autoren-URL
- https://www.webofscience.com/api/gateway?GWVersion=2&SrcApp=fis-test-1&SrcAuth=WosAPI&KeyUT=WOS:000400503100003&DestLinkType=FullRecord&DestApp=WOS_CPL
- DOI
- 10.3847/0004-637X/833/1/3
- eISSN
- 1538-4357
- Externe Identifier
- Clarivate Analytics Document Solution ID: ET7UA
- ISSN
- 0004-637X
- Ausgabe der Veröffentlichung
- 1
- Zeitschrift
- ASTROPHYSICAL JOURNAL
- Schlüsselwörter
- astroparticle physics
- methods: data analysis
- neutrinos
- Artikelnummer
- ARTN 3
- Datum der Veröffentlichung
- 2016
- Status
- Published
- Titel
- OBSERVATION AND CHARACTERIZATION OF A COSMIC MUON NEUTRINO FLUX FROM THE NORTHERN HEMISPHERE USING SIX YEARS OF ICECUBE DATA
- Sub types
- Article
- Ausgabe der Zeitschrift
- 833
Datenquelle: Web of Science (Lite)
- Andere Metadatenquellen:
-
- Abstract
- <jats:title>ABSTRACT</jats:title> <jats:p>The IceCube Collaboration has previously discovered a high-energy astrophysical neutrino flux using neutrino events with interaction vertices contained within the instrumented volume of the IceCube detector. We present a complementary measurement using charged current muon neutrino events where the interaction vertex can be outside this volume. As a consequence of the large muon range the effective area is significantly larger but the field of view is restricted to the Northern Hemisphere. IceCube data from 2009 through 2015 have been analyzed using a likelihood approach based on the reconstructed muon energy and zenith angle. At the highest neutrino energies between <jats:inline-formula> <jats:tex-math> <?CDATA $194\,\mathrm{TeV}$?> </jats:tex-math> <jats:inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="apjaa3e5cieqn1.gif" xlink:type="simple" /> </jats:inline-formula> and <jats:inline-formula> <jats:tex-math> <?CDATA $7.8\,\mathrm{PeV}$?> </jats:tex-math> <jats:inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="apjaa3e5cieqn2.gif" xlink:type="simple" /> </jats:inline-formula> a significant astrophysical contribution is observed, excluding a purely atmospheric origin of these events at <jats:inline-formula> <jats:tex-math> <?CDATA $5.6\sigma $?> </jats:tex-math> <jats:inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="apjaa3e5cieqn3.gif" xlink:type="simple" /> </jats:inline-formula> significance. The data are well described by an isotropic, unbroken power-law flux with a normalization at <jats:inline-formula> <jats:tex-math> <?CDATA $100\,\mathrm{TeV}$?> </jats:tex-math> <jats:inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="apjaa3e5cieqn4.gif" xlink:type="simple" /> </jats:inline-formula> neutrino energy of <jats:inline-formula> <jats:tex-math> <?CDATA $({0.90}_{-0.27}^{+0.30})\times {10}^{-18}\,{\mathrm{GeV}}^{-1}\,{\mathrm{cm}}^{-2}\,{{\rm{s}}}^{-1}\,{\mathrm{sr}}^{-1}$?> </jats:tex-math> <jats:inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="apjaa3e5cieqn5.gif" xlink:type="simple" /> </jats:inline-formula> and a hard spectral index of <jats:inline-formula> <jats:tex-math> <?CDATA $\gamma =2.13\pm 0.13$?> </jats:tex-math> <jats:inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="apjaa3e5cieqn6.gif" xlink:type="simple" /> </jats:inline-formula>. The observed spectrum is harder in comparison to previous IceCube analyses with lower energy thresholds which may indicate a break in the astrophysical neutrino spectrum of unknown origin. The highest-energy event observed has a reconstructed muon energy of <jats:inline-formula> <jats:tex-math> <?CDATA $(4.5\pm 1.2)\,\mathrm{PeV}$?> </jats:tex-math> <jats:inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="apjaa3e5cieqn7.gif" xlink:type="simple" /> </jats:inline-formula> which implies a probability of less than <jats:inline-formula> <jats:tex-math> <?CDATA $0.005 \% $?> </jats:tex-math> <jats:inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="apjaa3e5cieqn8.gif" xlink:type="simple" /> </jats:inline-formula> for this event to be of atmospheric origin. Analyzing the arrival directions of all events with reconstructed muon energies above <jats:inline-formula> <jats:tex-math> <?CDATA $200\,\mathrm{TeV}$?> </jats:tex-math> <jats:inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="apjaa3e5cieqn9.gif" xlink:type="simple" /> </jats:inline-formula> no correlation with known <jats:italic>γ</jats:italic>-ray sources was found. Using the high statistics of atmospheric neutrinos we report the current best constraints on a prompt atmospheric muon neutrino flux originating from charmed meson decays which is below 1.06 in units of the flux normalization of the model in Enberg et al.</jats:p>
- Autoren
- MG Aartsen
- K Abraham
- M Ackermann
- J Adams
- JA Aguilar
- M Ahlers
- M Ahrens
- D Altmann
- K Andeen
- T Anderson
- I Ansseau
- G Anton
- M Archinger
- C Argüelles
- J Auffenberg
- S Axani
- X Bai
- SW Barwick
- V Baum
- R Bay
- JJ Beatty
- J Becker Tjus
- K-H Becker
- S BenZvi
- P Berghaus
- D Berley
- E Bernardini
- A Bernhard
- DZ Besson
- G Binder
- D Bindig
- M Bissok
- E Blaufuss
- S Blot
- C Bohm
- M Börner
- F Bos
- D Bose
- S Böser
- O Botner
- J Braun
- L Brayeur
- H-P Bretz
- A Burgman
- T Carver
- M Casier
- E Cheung
- D Chirkin
- A Christov
- K Clark
- L Classen
- S Coenders
- GH Collin
- JM Conrad
- DF Cowen
- R Cross
- M Day
- JPAM de André
- C De Clercq
- E del Pino Rosendo
- H Dembinski
- S De Ridder
- P Desiati
- KD de Vries
- G de Wasseige
- M de With
- T DeYoung
- JC Díaz-Vélez
- V di Lorenzo
- H Dujmovic
- JP Dumm
- M Dunkman
- B Eberhardt
- T Ehrhardt
- B Eichmann
- P Eller
- S Euler
- PA Evenson
- S Fahey
- AR Fazely
- J Feintzeig
- J Felde
- K Filimonov
- C Finley
- S Flis
- C-C Fösig
- A Franckowiak
- E Friedman
- T Fuchs
- TK Gaisser
- J Gallagher
- L Gerhardt
- K Ghorbani
- W Giang
- L Gladstone
- M Glagla
- T Glüsenkamp
- A Goldschmidt
- G Golup
- JG Gonzalez
- D Grant
- Z Griffith
- C Haack
- A Haj Ismail
- A Hallgren
- F Halzen
- E Hansen
- B Hansmann
- T Hansmann
- K Hanson
- D Hebecker
- D Heereman
- K Helbing
- R Hellauer
- S Hickford
- J Hignight
- GC Hill
- KD Hoffman
- R Hoffmann
- K Holzapfel
- K Hoshina
- F Huang
- M Huber
- K Hultqvist
- S In
- A Ishihara
- E Jacobi
- GS Japaridze
- M Jeong
- K Jero
- BJP Jones
- M Jurkovic
- A Kappes
- T Karg
- A Karle
- U Katz
- M Kauer
- A Keivani
- JL Kelley
- J Kemp
- A Kheirandish
- M Kim
- T Kintscher
- J Kiryluk
- T Kittler
- SR Klein
- G Kohnen
- R Koirala
- H Kolanoski
- R Konietz
- L Köpke
- C Kopper
- S Kopper
- DJ Koskinen
- M Kowalski
- K Krings
- M Kroll
- G Krückl
- C Krüger
- J Kunnen
- S Kunwar
- N Kurahashi
- T Kuwabara
- M Labare
- JL Lanfranchi
- MJ Larson
- F Lauber
- D Lennarz
- M Lesiak-Bzdak
- M Leuermann
- J Leuner
- L Lu
- J Lünemann
- J Madsen
- G Maggi
- KBM Mahn
- S Mancina
- M Mandelartz
- R Maruyama
- K Mase
- R Maunu
- F McNally
- K Meagher
- M Medici
- M Meier
- A Meli
- T Menne
- G Merino
- T Meures
- S Miarecki
- L Mohrmann
- T Montaruli
- M Moulai
- R Nahnhauer
- U Naumann
- G Neer
- H Niederhausen
- SC Nowicki
- DR Nygren
- A Obertacke Pollmann
- A Olivas
- A O’Murchadha
- T Palczewski
- H Pandya
- DV Pankova
- P Peiffer
- Ö Penek
- JA Pepper
- C Pérez de los Heros
- D Pieloth
- E Pinat
- PB Price
- GT Przybylski
- M Quinnan
- C Raab
- L Rädel
- M Rameez
- K Rawlins
- R Reimann
- B Relethford
- M Relich
- E Resconi
- W Rhode
- M Richman
- B Riedel
- S Robertson
- M Rongen
- C Rott
- T Ruhe
- D Ryckbosch
- D Rysewyk
- L Sabbatini
- SE Sanchez Herrera
- A Sandrock
- J Sandroos
- S Sarkar
- K Satalecka
- M Schimp
- P Schlunder
- T Schmidt
- S Schoenen
- S Schöneberg
- L Schumacher
- D Seckel
- S Seunarine
- D Soldin
- M Song
- GM Spiczak
- C Spiering
- M Stahlberg
- T Stanev
- A Stasik
- A Steuer
- T Stezelberger
- RG Stokstad
- A Stößl
- R Ström
- NL Strotjohann
- GW Sullivan
- M Sutherland
- H Taavola
- I Taboada
- J Tatar
- F Tenholt
- S Ter-Antonyan
- A Terliuk
- G Tešić
- S Tilav
- PA Toale
- MN Tobin
- S Toscano
- D Tosi
- M Tselengidou
- A Turcati
- E Unger
- M Usner
- J Vandenbroucke
- N van Eijndhoven
- S Vanheule
- M van Rossem
- J van Santen
- J Veenkamp
- M Vehring
- M Voge
- M Vraeghe
- C Walck
- A Wallace
- M Wallraff
- N Wandkowsky
- Ch Weaver
- MJ Weiss
- C Wendt
- S Westerhoff
- BJ Whelan
- S Wickmann
- K Wiebe
- CH Wiebusch
- L Wille
- DR Williams
- L Wills
- M Wolf
- TR Wood
- E Woolsey
- K Woschnagg
- DL Xu
- XW Xu
- Y Xu
- JP Yanez
- G Yodh
- S Yoshida
- M Zoll
- DOI
- 10.3847/0004-637x/833/1/3
- eISSN
- 1538-4357
- ISSN
- 0004-637X
- Ausgabe der Veröffentlichung
- 1
- Zeitschrift
- The Astrophysical Journal
- Online publication date
- 2016
- Paginierung
- 3 - 3
- Datum der Veröffentlichung
- 2016
- Status
- Published
- Herausgeber
- American Astronomical Society
- Herausgeber URL
- http://dx.doi.org/10.3847/0004-637x/833/1/3
- Datum der Datenerfassung
- 2024
- Titel
- OBSERVATION AND CHARACTERIZATION OF A COSMIC MUON NEUTRINO FLUX FROM THE NORTHERN HEMISPHERE USING SIX YEARS OF ICECUBE DATA
- Ausgabe der Zeitschrift
- 833
Datenquelle: Crossref
- Autoren
- MG Aartsen
- others
- DOI
- 10.3847/0004-637X/833/1/3
- Zeitschrift
- Astrophys. J.
- Notes
- collaboration: IceCube archiveprefix: arXiv primaryclass: astro-ph.HE
- Artikelnummer
- 1
- Paginierung
- 3 - 3
- Datum der Veröffentlichung
- 2016
- Datum der Datenerfassung
- 2020
- Titel
- Observation and Characterization of a Cosmic Muon Neutrino Flux from the Northern Hemisphere using six years of IceCube data
- Sub types
- article
- Ausgabe der Zeitschrift
- 833
Datenquelle: Manual
- Beziehungen:
- Eigentum von