Neutrino oscillation studies with IceCube-DeepCore

M.G. Aartsen; K. Abraham; M. Ackermann; J. Adams; J.A. Aguilar; M. Ahlers; M. Ahrens; D. Altmann; T. Anderson; I. Ansseau; David Jason Koskinen; Morten Ankersen Medici; Michael James Larson; Subir Sarkar; Michael Marc Wolf

doi:10.1016/j.nuclphysb.2016.03.028

Neutrino oscillation studies with IceCube-DeepCore

M.G. Aartsen, K. Abraham, M. Ackermann, J. Adams, J.A. Aguilar, M. Ahlers, M. Ahrens, D. Altmann, T. Anderson, I. Ansseau, David Jason Koskinen, Morten Ankersen Medici, Michael James Larson, Subir Sarkar, Michael Marc Wolf

17 Citationer (Scopus)

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Abstract

IceCube, a gigaton-scale neutrino detector located at the South Pole, was primarily designed to search for astrophysical neutrinos with energies of PeV and higher. This goal has been achieved with the detection of the highest energy neutrinos to date. At the other end of the energy spectrum, the DeepCore extension lowers the energy threshold of the detector to approximately 10 GeV and opens the door for oscillation studies using atmospheric neutrinos. An analysis of the disappearance of these neutrinos has been completed, with the results produced being complementary with dedicated oscillation experiments. Following a review of the detector principle and performance, the method used to make these calculations, as well as the results, is detailed. Finally, the future prospects of IceCube-DeepCore and the next generation of neutrino experiments at the South Pole (IceCube-Gen2, specifically the PINGU sub-detector) are briefly discussed.

Originalsprog	Engelsk
Tidsskrift	Nuclear Physics B
Vol/bind	908
Sider (fra-til)	161-177
Antal sider	17
ISSN	0550-3213
DOI	https://doi.org/10.1016/j.nuclphysb.2016.03.028
Status	Udgivet - 31 jan. 2016

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10.1016/j.nuclphysb.2016.03.028Licens: CC BY

1-s2.0-S0550321316300141-mainForlagets udgivne version, 2,51 MBLicens: CC BY

Citationsformater

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title = "Neutrino oscillation studies with IceCube-DeepCore",

abstract = "IceCube, a gigaton-scale neutrino detector located at the South Pole, was primarily designed to search for astrophysical neutrinos with energies of PeV and higher. This goal has been achieved with the detection of the highest energy neutrinos to date. At the other end of the energy spectrum, the DeepCore extension lowers the energy threshold of the detector to approximately 10 GeV and opens the door for oscillation studies using atmospheric neutrinos. An analysis of the disappearance of these neutrinos has been completed, with the results produced being complementary with dedicated oscillation experiments. Following a review of the detector principle and performance, the method used to make these calculations, as well as the results, is detailed. Finally, the future prospects of IceCube-DeepCore and the next generation of neutrino experiments at the South Pole (IceCube-Gen2, specifically the PINGU sub-detector) are briefly discussed.",

author = "M.G. Aartsen and K. Abraham and M. Ackermann and J. Adams and J.A. Aguilar and M. Ahlers and M. Ahrens and D. Altmann and T. Anderson and I. Ansseau and Koskinen, {David Jason} and Medici, {Morten Ankersen} and Larson, {Michael James} and Subir Sarkar and Wolf, {Michael Marc}",

year = "2016",

month = jan,

day = "31",

doi = "10.1016/j.nuclphysb.2016.03.028",

language = "English",

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T1 - Neutrino oscillation studies with IceCube-DeepCore

AU - Aartsen, M.G.

AU - Abraham, K.

AU - Ackermann, M.

AU - Adams, J.

AU - Aguilar, J.A.

AU - Ahlers, M.

AU - Ahrens, M.

AU - Altmann, D.

AU - Anderson, T.

AU - Ansseau, I.

AU - Koskinen, David Jason

AU - Medici, Morten Ankersen

AU - Larson, Michael James

AU - Sarkar, Subir

AU - Wolf, Michael Marc

PY - 2016/1/31

Y1 - 2016/1/31

N2 - IceCube, a gigaton-scale neutrino detector located at the South Pole, was primarily designed to search for astrophysical neutrinos with energies of PeV and higher. This goal has been achieved with the detection of the highest energy neutrinos to date. At the other end of the energy spectrum, the DeepCore extension lowers the energy threshold of the detector to approximately 10 GeV and opens the door for oscillation studies using atmospheric neutrinos. An analysis of the disappearance of these neutrinos has been completed, with the results produced being complementary with dedicated oscillation experiments. Following a review of the detector principle and performance, the method used to make these calculations, as well as the results, is detailed. Finally, the future prospects of IceCube-DeepCore and the next generation of neutrino experiments at the South Pole (IceCube-Gen2, specifically the PINGU sub-detector) are briefly discussed.

AB - IceCube, a gigaton-scale neutrino detector located at the South Pole, was primarily designed to search for astrophysical neutrinos with energies of PeV and higher. This goal has been achieved with the detection of the highest energy neutrinos to date. At the other end of the energy spectrum, the DeepCore extension lowers the energy threshold of the detector to approximately 10 GeV and opens the door for oscillation studies using atmospheric neutrinos. An analysis of the disappearance of these neutrinos has been completed, with the results produced being complementary with dedicated oscillation experiments. Following a review of the detector principle and performance, the method used to make these calculations, as well as the results, is detailed. Finally, the future prospects of IceCube-DeepCore and the next generation of neutrino experiments at the South Pole (IceCube-Gen2, specifically the PINGU sub-detector) are briefly discussed.

U2 - 10.1016/j.nuclphysb.2016.03.028

DO - 10.1016/j.nuclphysb.2016.03.028

M3 - Journal article

SN - 0550-3213

VL - 908

SP - 161

EP - 177

JO - Nuclear Physics, Section B

JF - Nuclear Physics, Section B

ER -

Neutrino oscillation studies with IceCube-DeepCore

Abstract

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