Physics Potential of the IceCube DeepCore detector

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Physics Potential of the IceCube DeepCore detector. / Koskinen, D. J.; Icecube Collaboration.

I: Nuclear Physics B - Proceedings Supplements, Bind 229-232, 554, 01.08.2012.

Publikation: Bidrag til tidsskrift › Tidsskriftartikel › Forskning › fagfællebedømt

Harvard

Koskinen, DJ & Icecube Collaboration 2012, 'Physics Potential of the IceCube DeepCore detector', Nuclear Physics B - Proceedings Supplements, bind 229-232, 554. https://doi.org/10.1016/j.nuclphysbps.2012.09.191

APA

Koskinen, D. J., & Icecube Collaboration (2012). Physics Potential of the IceCube DeepCore detector. Nuclear Physics B - Proceedings Supplements, 229-232, [554]. https://doi.org/10.1016/j.nuclphysbps.2012.09.191

Vancouver

Koskinen DJ, Icecube Collaboration. Physics Potential of the IceCube DeepCore detector. Nuclear Physics B - Proceedings Supplements. 2012 aug. 1;229-232. 554. https://doi.org/10.1016/j.nuclphysbps.2012.09.191

Author

Koskinen, D. J. ; Icecube Collaboration. / Physics Potential of the IceCube DeepCore detector. I: Nuclear Physics B - Proceedings Supplements. 2012 ; Bind 229-232.

Bibtex

@article{87281c915be8485cb71b1463c2be6260,
title = "Physics Potential of the IceCube DeepCore detector",
abstract = "The recent commissioning of the full DeepCore sub-array, a low-energy extension of the IceCube neutrino observatory, offers opportunities for neutrino physics in the energy region of 10 GeV to 1 TeV. The improved energy reach, use of the surrounding IceCube detector as an active veto and immense size of DeepCore will produce one of the largest all-sky neutrino datasets ever acquired. DeepCore will provide sensitivity to neutrinos from possible neutralino dark matter annihilations in the Earth, Sun and galactic center, down to neutralino masses in the region of ~ 50 GeV. Tens of thousands of atmospheric neutrinos will be detected annually after oscillating over a baseline of up to one Earth diameter, opening the possibilities for muon neutrino disappearance and tau neutrino appearance measurements.",
keywords = "IceCube, Neutrino astronomy, Neutrino oscillation",
author = "Koskinen, {D. J.} and {Icecube Collaboration}",
year = "2012",
month = aug,
day = "1",
doi = "10.1016/j.nuclphysbps.2012.09.191",
language = "English",
volume = "229-232",
journal = "Nuclear and Particle Physics Proceedings",
issn = "2405-6014",
publisher = "Elsevier",

}

RIS

TY - JOUR

T1 - Physics Potential of the IceCube DeepCore detector

AU - Koskinen, D. J.

AU - Icecube Collaboration

PY - 2012/8/1

Y1 - 2012/8/1

N2 - The recent commissioning of the full DeepCore sub-array, a low-energy extension of the IceCube neutrino observatory, offers opportunities for neutrino physics in the energy region of 10 GeV to 1 TeV. The improved energy reach, use of the surrounding IceCube detector as an active veto and immense size of DeepCore will produce one of the largest all-sky neutrino datasets ever acquired. DeepCore will provide sensitivity to neutrinos from possible neutralino dark matter annihilations in the Earth, Sun and galactic center, down to neutralino masses in the region of ~ 50 GeV. Tens of thousands of atmospheric neutrinos will be detected annually after oscillating over a baseline of up to one Earth diameter, opening the possibilities for muon neutrino disappearance and tau neutrino appearance measurements.

AB - The recent commissioning of the full DeepCore sub-array, a low-energy extension of the IceCube neutrino observatory, offers opportunities for neutrino physics in the energy region of 10 GeV to 1 TeV. The improved energy reach, use of the surrounding IceCube detector as an active veto and immense size of DeepCore will produce one of the largest all-sky neutrino datasets ever acquired. DeepCore will provide sensitivity to neutrinos from possible neutralino dark matter annihilations in the Earth, Sun and galactic center, down to neutralino masses in the region of ~ 50 GeV. Tens of thousands of atmospheric neutrinos will be detected annually after oscillating over a baseline of up to one Earth diameter, opening the possibilities for muon neutrino disappearance and tau neutrino appearance measurements.

KW - IceCube

KW - Neutrino astronomy

KW - Neutrino oscillation

UR - http://www.scopus.com/inward/record.url?scp=84870166902&partnerID=8YFLogxK

U2 - 10.1016/j.nuclphysbps.2012.09.191

DO - 10.1016/j.nuclphysbps.2012.09.191

M3 - Journal article

AN - SCOPUS:84870166902

VL - 229-232

JO - Nuclear and Particle Physics Proceedings

JF - Nuclear and Particle Physics Proceedings

SN - 2405-6014

M1 - 554

ER -

ID: 217647007