Search for astrophysical tau neutrinos in three years of IceCube data
- Autores
- Aartsen, M. G.; Abraham, K.; Ackermann, M.; Adams, J.; Aguilar, J. A.; Golup, Geraldina Tamara; Walck, C.; Wallace, A.; Wallraff, M.; Wandkowsky, N.; Weaver, Ch.; Wendt, C.; Westerhoff, S.; Whelan, B. J.; Whitehorn, N.; Wiebe, K.; Wiebusch, C. H.; Wille, L.; Williams, D. R.; Wissing, H.; Wolf, M.; Wood, T. R.; Woschnagg, K.; Xu, D. L.; Xu, X. W.; Xu, Y.; Yanez, J. P.; Yodh, G.; Yoshida, S.; Zoll, M.
- Año de publicación
- 2016
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The IceCube Neutrino Observatory has observed a diffuse flux of TeV-PeV astrophysical neutrinos at 5.7σ significance from an all-flavor search. The direct detection of tau neutrinos in this flux has yet to occur. Tau neutrinos become distinguishable from other flavors in IceCube at energies above a few hundred TeV, when the cascade from the tau neutrino charged current interaction becomes resolvable from the cascade from the tau lepton decay. This paper presents results from the first dedicated search for tau neutrinos with energies between 214 TeV and 72 PeV in the full IceCube detector. The analysis searches for IceCube optical sensors that observe two separate pulses in a single event - one from the tau neutrino interaction and a second from the tau decay. No candidate events were observed in three years of IceCube data. For the first time, a differential upper limit on astrophysical tau neutrinos is derived around the PeV energy region, which is nearly 3 orders of magnitude lower in energy than previous limits from dedicated tau neutrino searches.
Fil: Aartsen, M. G.. University of Adelaide; Australia
Fil: Abraham, K.. Technische Universitat München; Alemania
Fil: Ackermann, M.. Deutsches Elektronen-Synchrotron; Alemania
Fil: Adams, J.. University Of Canterbury; Nueva Zelanda
Fil: Aguilar, J. A.. Université Libre de Bruxelles; Bélgica
Fil: Golup, Geraldina Tamara. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Patagonia Norte; Argentina. Vrije Unviversiteit Brussel; Bélgica
Fil: Walck, C.. Stockholms Universitet; Suecia
Fil: Wallace, A.. University of Adelaide; Australia
Fil: Wallraff, M.. Rwth Aachen University; Alemania
Fil: Wandkowsky, N.. University of Wisconsin; Estados Unidos
Fil: Weaver, Ch.. University of Alberta; Canadá
Fil: Wendt, C.. University of Wisconsin; Estados Unidos
Fil: Westerhoff, S.. University of Wisconsin; Estados Unidos
Fil: Whelan, B. J.. University of Adelaide; Australia
Fil: Whitehorn, N.. University of Wisconsin; Estados Unidos
Fil: Wiebe, K.. University of Mainz; Alemania
Fil: Wiebusch, C. H.. Rwth Aachen University; Alemania
Fil: Wille, L.. University of Wisconsin; Estados Unidos
Fil: Williams, D. R.. University of Alabama at Birmingahm; Estados Unidos
Fil: Wissing, H.. University of Maryland; Estados Unidos
Fil: Wolf, M.. Stockholms Universitet; Suecia
Fil: Wood, T. R.. University of Alberta; Canadá
Fil: Woschnagg, K.. University of California; Estados Unidos
Fil: Xu, D. L.. University of Alabama at Birmingahm; Estados Unidos
Fil: Xu, X. W.. Southern University; Estados Unidos
Fil: Xu, Y.. Stony Brook University; Estados Unidos
Fil: Yanez, J. P.. Deutsches Elektronen-Synchrotron DESY; Alemania
Fil: Yodh, G.. University of California; Estados Unidos
Fil: Yoshida, S.. Chiba University; Japón
Fil: Zoll, M.. Stockholms Universitet; Suecia - Materia
-
Neutrino Astronomy
Neutrino Observatory
Icecube - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/63353
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oai:ri.conicet.gov.ar:11336/63353 |
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spelling |
Search for astrophysical tau neutrinos in three years of IceCube dataAartsen, M. G.Abraham, K.Ackermann, M.Adams, J.Aguilar, J. A.Golup, Geraldina TamaraWalck, C.Wallace, A.Wallraff, M.Wandkowsky, N.Weaver, Ch.Wendt, C.Westerhoff, S.Whelan, B. J.Whitehorn, N.Wiebe, K.Wiebusch, C. H.Wille, L.Williams, D. R.Wissing, H.Wolf, M.Wood, T. R.Woschnagg, K.Xu, D. L.Xu, X. W.Xu, Y.Yanez, J. P.Yodh, G.Yoshida, S.Zoll, M.Neutrino AstronomyNeutrino ObservatoryIcecubehttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The IceCube Neutrino Observatory has observed a diffuse flux of TeV-PeV astrophysical neutrinos at 5.7σ significance from an all-flavor search. The direct detection of tau neutrinos in this flux has yet to occur. Tau neutrinos become distinguishable from other flavors in IceCube at energies above a few hundred TeV, when the cascade from the tau neutrino charged current interaction becomes resolvable from the cascade from the tau lepton decay. This paper presents results from the first dedicated search for tau neutrinos with energies between 214 TeV and 72 PeV in the full IceCube detector. The analysis searches for IceCube optical sensors that observe two separate pulses in a single event - one from the tau neutrino interaction and a second from the tau decay. No candidate events were observed in three years of IceCube data. For the first time, a differential upper limit on astrophysical tau neutrinos is derived around the PeV energy region, which is nearly 3 orders of magnitude lower in energy than previous limits from dedicated tau neutrino searches.Fil: Aartsen, M. G.. University of Adelaide; AustraliaFil: Abraham, K.. Technische Universitat München; AlemaniaFil: Ackermann, M.. Deutsches Elektronen-Synchrotron; AlemaniaFil: Adams, J.. University Of Canterbury; Nueva ZelandaFil: Aguilar, J. A.. Université Libre de Bruxelles; BélgicaFil: Golup, Geraldina Tamara. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Patagonia Norte; Argentina. Vrije Unviversiteit Brussel; BélgicaFil: Walck, C.. Stockholms Universitet; SueciaFil: Wallace, A.. University of Adelaide; AustraliaFil: Wallraff, M.. Rwth Aachen University; AlemaniaFil: Wandkowsky, N.. University of Wisconsin; Estados UnidosFil: Weaver, Ch.. University of Alberta; CanadáFil: Wendt, C.. University of Wisconsin; Estados UnidosFil: Westerhoff, S.. University of Wisconsin; Estados UnidosFil: Whelan, B. J.. University of Adelaide; AustraliaFil: Whitehorn, N.. University of Wisconsin; Estados UnidosFil: Wiebe, K.. University of Mainz; AlemaniaFil: Wiebusch, C. H.. Rwth Aachen University; AlemaniaFil: Wille, L.. University of Wisconsin; Estados UnidosFil: Williams, D. R.. University of Alabama at Birmingahm; Estados UnidosFil: Wissing, H.. University of Maryland; Estados UnidosFil: Wolf, M.. Stockholms Universitet; SueciaFil: Wood, T. R.. University of Alberta; CanadáFil: Woschnagg, K.. University of California; Estados UnidosFil: Xu, D. L.. University of Alabama at Birmingahm; Estados UnidosFil: Xu, X. W.. Southern University; Estados UnidosFil: Xu, Y.. Stony Brook University; Estados UnidosFil: Yanez, J. P.. Deutsches Elektronen-Synchrotron DESY; AlemaniaFil: Yodh, G.. University of California; Estados UnidosFil: Yoshida, S.. Chiba University; JapónFil: Zoll, M.. Stockholms Universitet; SueciaAmerican Physical Society2016-01-15info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/63353Aartsen, M. G.; Abraham, K.; Ackermann, M.; Adams, J.; Aguilar, J. A.; et al.; Search for astrophysical tau neutrinos in three years of IceCube data; American Physical Society; Physical Review D: Particles, Fields, Gravitation and Cosmology; 93; 2; 15-1-2016; 1-11; 0220011550-7998CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://journals.aps.org/prd/abstract/10.1103/PhysRevD.93.022001info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevD.93.022001info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-03T09:46:38Zoai:ri.conicet.gov.ar:11336/63353instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-03 09:46:38.575CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Search for astrophysical tau neutrinos in three years of IceCube data |
title |
Search for astrophysical tau neutrinos in three years of IceCube data |
spellingShingle |
Search for astrophysical tau neutrinos in three years of IceCube data Aartsen, M. G. Neutrino Astronomy Neutrino Observatory Icecube |
title_short |
Search for astrophysical tau neutrinos in three years of IceCube data |
title_full |
Search for astrophysical tau neutrinos in three years of IceCube data |
title_fullStr |
Search for astrophysical tau neutrinos in three years of IceCube data |
title_full_unstemmed |
Search for astrophysical tau neutrinos in three years of IceCube data |
title_sort |
Search for astrophysical tau neutrinos in three years of IceCube data |
dc.creator.none.fl_str_mv |
Aartsen, M. G. Abraham, K. Ackermann, M. Adams, J. Aguilar, J. A. Golup, Geraldina Tamara Walck, C. Wallace, A. Wallraff, M. Wandkowsky, N. Weaver, Ch. Wendt, C. Westerhoff, S. Whelan, B. J. Whitehorn, N. Wiebe, K. Wiebusch, C. H. Wille, L. Williams, D. R. Wissing, H. Wolf, M. Wood, T. R. Woschnagg, K. Xu, D. L. Xu, X. W. Xu, Y. Yanez, J. P. Yodh, G. Yoshida, S. Zoll, M. |
author |
Aartsen, M. G. |
author_facet |
Aartsen, M. G. Abraham, K. Ackermann, M. Adams, J. Aguilar, J. A. Golup, Geraldina Tamara Walck, C. Wallace, A. Wallraff, M. Wandkowsky, N. Weaver, Ch. Wendt, C. Westerhoff, S. Whelan, B. J. Whitehorn, N. Wiebe, K. Wiebusch, C. H. Wille, L. Williams, D. R. Wissing, H. Wolf, M. Wood, T. R. Woschnagg, K. Xu, D. L. Xu, X. W. Xu, Y. Yanez, J. P. Yodh, G. Yoshida, S. Zoll, M. |
author_role |
author |
author2 |
Abraham, K. Ackermann, M. Adams, J. Aguilar, J. A. Golup, Geraldina Tamara Walck, C. Wallace, A. Wallraff, M. Wandkowsky, N. Weaver, Ch. Wendt, C. Westerhoff, S. Whelan, B. J. Whitehorn, N. Wiebe, K. Wiebusch, C. H. Wille, L. Williams, D. R. Wissing, H. Wolf, M. Wood, T. R. Woschnagg, K. Xu, D. L. Xu, X. W. Xu, Y. Yanez, J. P. Yodh, G. Yoshida, S. Zoll, M. |
author2_role |
author author author author author author author author author author author author author author author author author author author author author author author author author author author author author |
dc.subject.none.fl_str_mv |
Neutrino Astronomy Neutrino Observatory Icecube |
topic |
Neutrino Astronomy Neutrino Observatory Icecube |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
The IceCube Neutrino Observatory has observed a diffuse flux of TeV-PeV astrophysical neutrinos at 5.7σ significance from an all-flavor search. The direct detection of tau neutrinos in this flux has yet to occur. Tau neutrinos become distinguishable from other flavors in IceCube at energies above a few hundred TeV, when the cascade from the tau neutrino charged current interaction becomes resolvable from the cascade from the tau lepton decay. This paper presents results from the first dedicated search for tau neutrinos with energies between 214 TeV and 72 PeV in the full IceCube detector. The analysis searches for IceCube optical sensors that observe two separate pulses in a single event - one from the tau neutrino interaction and a second from the tau decay. No candidate events were observed in three years of IceCube data. For the first time, a differential upper limit on astrophysical tau neutrinos is derived around the PeV energy region, which is nearly 3 orders of magnitude lower in energy than previous limits from dedicated tau neutrino searches. Fil: Aartsen, M. G.. University of Adelaide; Australia Fil: Abraham, K.. Technische Universitat München; Alemania Fil: Ackermann, M.. Deutsches Elektronen-Synchrotron; Alemania Fil: Adams, J.. University Of Canterbury; Nueva Zelanda Fil: Aguilar, J. A.. Université Libre de Bruxelles; Bélgica Fil: Golup, Geraldina Tamara. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Patagonia Norte; Argentina. Vrije Unviversiteit Brussel; Bélgica Fil: Walck, C.. Stockholms Universitet; Suecia Fil: Wallace, A.. University of Adelaide; Australia Fil: Wallraff, M.. Rwth Aachen University; Alemania Fil: Wandkowsky, N.. University of Wisconsin; Estados Unidos Fil: Weaver, Ch.. University of Alberta; Canadá Fil: Wendt, C.. University of Wisconsin; Estados Unidos Fil: Westerhoff, S.. University of Wisconsin; Estados Unidos Fil: Whelan, B. J.. University of Adelaide; Australia Fil: Whitehorn, N.. University of Wisconsin; Estados Unidos Fil: Wiebe, K.. University of Mainz; Alemania Fil: Wiebusch, C. H.. Rwth Aachen University; Alemania Fil: Wille, L.. University of Wisconsin; Estados Unidos Fil: Williams, D. R.. University of Alabama at Birmingahm; Estados Unidos Fil: Wissing, H.. University of Maryland; Estados Unidos Fil: Wolf, M.. Stockholms Universitet; Suecia Fil: Wood, T. R.. University of Alberta; Canadá Fil: Woschnagg, K.. University of California; Estados Unidos Fil: Xu, D. L.. University of Alabama at Birmingahm; Estados Unidos Fil: Xu, X. W.. Southern University; Estados Unidos Fil: Xu, Y.. Stony Brook University; Estados Unidos Fil: Yanez, J. P.. Deutsches Elektronen-Synchrotron DESY; Alemania Fil: Yodh, G.. University of California; Estados Unidos Fil: Yoshida, S.. Chiba University; Japón Fil: Zoll, M.. Stockholms Universitet; Suecia |
description |
The IceCube Neutrino Observatory has observed a diffuse flux of TeV-PeV astrophysical neutrinos at 5.7σ significance from an all-flavor search. The direct detection of tau neutrinos in this flux has yet to occur. Tau neutrinos become distinguishable from other flavors in IceCube at energies above a few hundred TeV, when the cascade from the tau neutrino charged current interaction becomes resolvable from the cascade from the tau lepton decay. This paper presents results from the first dedicated search for tau neutrinos with energies between 214 TeV and 72 PeV in the full IceCube detector. The analysis searches for IceCube optical sensors that observe two separate pulses in a single event - one from the tau neutrino interaction and a second from the tau decay. No candidate events were observed in three years of IceCube data. For the first time, a differential upper limit on astrophysical tau neutrinos is derived around the PeV energy region, which is nearly 3 orders of magnitude lower in energy than previous limits from dedicated tau neutrino searches. |
publishDate |
2016 |
dc.date.none.fl_str_mv |
2016-01-15 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/63353 Aartsen, M. G.; Abraham, K.; Ackermann, M.; Adams, J.; Aguilar, J. A.; et al.; Search for astrophysical tau neutrinos in three years of IceCube data; American Physical Society; Physical Review D: Particles, Fields, Gravitation and Cosmology; 93; 2; 15-1-2016; 1-11; 022001 1550-7998 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/63353 |
identifier_str_mv |
Aartsen, M. G.; Abraham, K.; Ackermann, M.; Adams, J.; Aguilar, J. A.; et al.; Search for astrophysical tau neutrinos in three years of IceCube data; American Physical Society; Physical Review D: Particles, Fields, Gravitation and Cosmology; 93; 2; 15-1-2016; 1-11; 022001 1550-7998 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/https://journals.aps.org/prd/abstract/10.1103/PhysRevD.93.022001 info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevD.93.022001 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
American Physical Society |
publisher.none.fl_str_mv |
American Physical Society |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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1842268808271626240 |
score |
13.13397 |