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000291928 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2014-04/84
000291928 037__ $$aPUBDB-2015-05662
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000291928 0881_ $$aDESY-PROC-2014-04
000291928 088__ $$2DESY$$aDESY-PROC-2014-04
000291928 1001_ $$aPalczewski, Tomasz$$b0
000291928 1112_ $$aPanic2014$$cHamburg$$d2014-08-25 - 2014-08-29$$gPanic2014$$wGermany
000291928 245__ $$aNeutrino Physics with the Precision IceCube Next Generation Upgrade (PINGU)
000291928 260__ $$aHamburg$$bDeutsches Elektronen-Synchrotron, DESY$$c2014
000291928 300__ $$a313-316
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000291928 3367_ $$0PUB:(DE-HGF)8$$2PUB:(DE-HGF)$$aContribution to a conference proceedings$$bcontrib$$mcontrib$$s1450087271_7046
000291928 3367_ $$0PUB:(DE-HGF)15$$2PUB:(DE-HGF)$$aInternal Report$$mintrep
000291928 3367_ $$2BibTeX$$aINPROCEEDINGS
000291928 520__ $$aThe IceCube Neutrino Observatory at the geographic South Pole is the largest neutrino telescope on Earth. IceCube and its low energy extension, DeepCore, were fully assembled at the end of 2010. DeepCore lowered the IceCube neutrino energy threshold to about 10 GeV, allowing access to a rich variety of atmospheric neutrino oscillation physics, and further improving sensitivity to indirect searches for WIMP dark matter and other phenomena.The recent measurements of a relatively large $\theta_{13}$ mixing angle and the first observations of atmospheric neutrino oscillations in the tens of GeV region in DeepCore open the possibility to determine the Neutrino Mass Hierarchy (NMH) in the proposed new in-fill array called Precision IceCube Next Generation Upgrade (PINGU).PINGU would lower the neutrino energy threshold and significantly increase the sensitivity to the NMH. For every year of the PINGU detector operation, on the order of one hundred thousand atmospheric neutrinos will be collected. These high statistics will allow PINGU to distinguish between the normal and inverted NMH at 3$\sigma$ significance with an estimated 3.5 years of data.
000291928 536__ $$0G:(DE-HGF)POF3-611$$a611 - Fundamental Particles and Forces (POF3-611)$$cPOF3-611$$fPOF III$$x0
000291928 588__ $$aDataset connected to DataCite, INSPIRE
000291928 650_7 $$2INSPIRE$$aneutrino: atmosphere
000291928 650_7 $$2INSPIRE$$aneutrino: energy
000291928 650_7 $$2INSPIRE$$aenergy: threshold
000291928 650_7 $$2INSPIRE$$aneutrino: oscillation
000291928 650_7 $$2INSPIRE$$aneutrino: detector
000291928 650_7 $$2INSPIRE$$aenergy: low
000291928 650_7 $$2INSPIRE$$aWIMP: dark matter
000291928 650_7 $$2INSPIRE$$amass: hierarchy
000291928 650_7 $$2INSPIRE$$aIceCube
000291928 650_7 $$2INSPIRE$$asensitivity
000291928 650_7 $$2INSPIRE$$aupgrade
000291928 650_7 $$2INSPIRE$$amixing angle
000291928 650_7 $$2INSPIRE$$aobservatory
000291928 650_7 $$2INSPIRE$$astatistics
000291928 650_7 $$2INSPIRE$$apole
000291928 693__ $$0EXP:(DE-MLZ)NOSPEC-20140101$$5EXP:(DE-MLZ)NOSPEC-20140101$$eNo specific instrument$$x0
000291928 7001_ $$0P:(DE-HGF)0$$aIceCube/PINGU Collaboration$$b1$$eCollaboration Author
000291928 773__ $$a10.3204/DESY-PROC-2014-04/84
000291928 7870_ $$0PUBDB-2015-03603$$aSchmidt, Alexander et.al.$$dHamburg : Deutsches Elektronen-Synchrotron, DESY, Hamburg, 2014$$iIsPartOf$$rDESY-PROC-2014-04$$tProceedings, 20th International Conference on Particles and Nuclei (PANIC 14)
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