Atmospheric neutrino results from IceCube- DeepCore and plans for PINGU

D. Jason Koskinen; M.G. Aartsen; M. Ackermann; J. Adams; J.A. Aguilar; Markus Tobias Ahlers; M. Ahrens; I. Al Samarai; D. Altmann; K. Andeen; T. Anderson; Michael James Larson; Morten Ankersen Medici; M Rameez; Subir Sarkar

doi:10.1088/1742-6596/888/1/012023

Atmospheric neutrino results from IceCube- DeepCore and plans for PINGU

D. Jason Koskinen, M.G. Aartsen, M. Ackermann, J. Adams, J.A. Aguilar, Markus Tobias Ahlers, M. Ahrens, I. Al Samarai, D. Altmann, K. Andeen, T. Anderson, Michael James Larson, Morten Ankersen Medici, M Rameez, Subir Sarkar

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Abstract

The IceCube neutrino observatory at the South Pole is the largest operating neutrino detector in the world and spans a wide range of science topics, from astronomy at the PeV-scale to particle physics at the GeV-scale. We present results from the search for a light, O(1) eV², sterile neutrino using the large IceCube array and, separately, using the lower energy extension DeepCore sub-array. Additionally, we review the atmospheric neutrino results and expected sensitivities related to oscillation physics (ν_μ disappearance and ν_τ appearance) as well as new limits on non-standard interactions. Continuing the success of the IceCube-DeepCore physics program, a proposed next generation in-fill detector with increased sensitivity to neutrinos of O(1) GeV will be covered.

Originalsprog	Engelsk
Artikelnummer	012023
Bogserie	Journal of Physics: Conference Series
Vol/bind	888
Udgave nummer	conference 1
ISSN	1742-6596
DOI	https://doi.org/10.1088/1742-6596/888/1/012023
Status	Udgivet - 20 sep. 2017

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10.1088/1742-6596/888/1/012023Licens: CC BY

Jason_Koskinen_2017_J._Phys.__Conf._Ser._888_012023Forlagets udgivne version, 507 KB

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Koskinen, D. J., Aartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M. T., Ahrens, M., Al Samarai, I., Altmann, D., Andeen, K., Anderson, T., Larson, M. J., Medici, M. A., Rameez, M., & Sarkar, S. (2017). Atmospheric neutrino results from IceCube- DeepCore and plans for PINGU. Journal of Physics: Conference Series, 888(conference 1), Artikel 012023. https://doi.org/10.1088/1742-6596/888/1/012023

Koskinen, DJ, Aartsen, MG, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, MT, Ahrens, M, Al Samarai, I, Altmann, D, Andeen, K, Anderson, T, Larson, MJ, Medici, MA, Rameez, M & Sarkar, S 2017, 'Atmospheric neutrino results from IceCube- DeepCore and plans for PINGU', Journal of Physics: Conference Series, bind 888, nr. conference 1, 012023. https://doi.org/10.1088/1742-6596/888/1/012023

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abstract = "The IceCube neutrino observatory at the South Pole is the largest operating neutrino detector in the world and spans a wide range of science topics, from astronomy at the PeV-scale to particle physics at the GeV-scale. We present results from the search for a light, O(1) eV2, sterile neutrino using the large IceCube array and, separately, using the lower energy extension DeepCore sub-array. Additionally, we review the atmospheric neutrino results and expected sensitivities related to oscillation physics (νμ disappearance and ντ appearance) as well as new limits on non-standard interactions. Continuing the success of the IceCube-DeepCore physics program, a proposed next generation in-fill detector with increased sensitivity to neutrinos of O(1) GeV will be covered.",

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AU - Koskinen, D. Jason

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AU - Ackermann, M.

AU - Adams, J.

AU - Aguilar, J.A.

AU - Ahlers, Markus Tobias

AU - Ahrens, M.

AU - Al Samarai, I.

AU - Altmann, D.

AU - Andeen, K.

AU - Anderson, T.

AU - Larson, Michael James

AU - Medici, Morten Ankersen

AU - Rameez, M

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AB - The IceCube neutrino observatory at the South Pole is the largest operating neutrino detector in the world and spans a wide range of science topics, from astronomy at the PeV-scale to particle physics at the GeV-scale. We present results from the search for a light, O(1) eV2, sterile neutrino using the large IceCube array and, separately, using the lower energy extension DeepCore sub-array. Additionally, we review the atmospheric neutrino results and expected sensitivities related to oscillation physics (νμ disappearance and ντ appearance) as well as new limits on non-standard interactions. Continuing the success of the IceCube-DeepCore physics program, a proposed next generation in-fill detector with increased sensitivity to neutrinos of O(1) GeV will be covered.

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Atmospheric neutrino results from IceCube- DeepCore and plans for PINGU

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