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000434628 005__ 20250729150051.0
000434628 0247_ $$2doi$$a10.1140/epjc/s10052-019-7555-0
000434628 0247_ $$2INSPIRETeX$$aAartsen:2020myq
000434628 0247_ $$2inspire$$ainspire:1774280
000434628 0247_ $$2ISSN$$a1434-6044
000434628 0247_ $$2ISSN$$a1434-6052
000434628 0247_ $$2altmetric$$aaltmetric:73591454
000434628 0247_ $$2WOS$$aWOS:000511722800001
000434628 0247_ $$2datacite_doi$$a10.3204/PUBDB-2020-00189
000434628 0247_ $$2openalex$$aopenalex:W2997107489
000434628 037__ $$aPUBDB-2020-00189
000434628 041__ $$aEnglish
000434628 082__ $$a530
000434628 1001_ $$aAartsen, M. G.$$b0
000434628 245__ $$aDevelopment of an analysis to probe the neutrino mass ordering with atmospheric neutrinos using three years of IceCube DeepCore data
000434628 260__ $$aHeidelberg$$bSpringer$$c2020
000434628 3367_ $$2DRIVER$$aarticle
000434628 3367_ $$2DataCite$$aOutput Types/Journal article
000434628 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$bjournal$$mjournal$$s1587070134_31771
000434628 3367_ $$2BibTeX$$aARTICLE
000434628 3367_ $$2ORCID$$aJOURNAL_ARTICLE
000434628 3367_ $$00$$2EndNote$$aJournal Article
000434628 500__ $$a© The Author(s)
000434628 520__ $$aThe Neutrino Mass Ordering (NMO) remains one of the outstanding questions in the field of neutrino physics. One strategy to measure the NMO is to observe matter effects in the oscillation pattern of atmospheric neutrinos above $\sim 1\,\mathrm {GeV}$, as proposed for several next-generation neutrino experiments. Moreover, the existing IceCube DeepCore detector can already explore this type of measurement. We present the development and application of two independent analyses to search for the signature of the NMO with three years of DeepCore data. These analyses include a full treatment of systematic uncertainties and a statistically-rigorous method to determine the significance for the NMO from a fit to the data. Both analyses show that the dataset is fully compatible with both mass orderings. For the more sensitive analysis, we observe a preference for normal ordering with a p-value of $p_\mathrm {IO} = 15.3\%$ and $\mathrm {CL}_\mathrm {s}=53.3\%$ for the inverted ordering hypothesis, while the experimental results from both analyses are consistent within their uncertainties. Since the result is independent of the value of $\delta _\mathrm {CP}$ and obtained from energies $E_\nu \gtrsim 5\,\mathrm {GeV}$, it is complementary to recent results from long-baseline experiments. These analyses set the groundwork for the future of this measurement with more capable detectors, such as the IceCube Upgrade and the proposed PINGU detector.
000434628 536__ $$0G:(DE-HGF)POF3-613$$a613 - Matter and Radiation from the Universe (POF3-613)$$cPOF3-613$$fPOF III$$x0
000434628 588__ $$aDataset connected to CrossRef, INSPIRE
000434628 650_7 $$2autogen$$aneutrino: atmosphere
000434628 650_7 $$2autogen$$aneutrino: mass
000434628 650_7 $$2autogen$$aIceCube: upgrade
000434628 650_7 $$2autogen$$amatter: effect
000434628 650_7 $$2autogen$$aexperimental results
000434628 650_7 $$2autogen$$aoscillation
000434628 650_7 $$2autogen$$asignature
000434628 650_7 $$2autogen$$aPINGU
000434628 650_7 $$2autogen$$a5/3
000434628 693__ $$0EXP:(DE-H253)IceCube-20150101$$5EXP:(DE-H253)IceCube-20150101$$eIceCube South Pole Neutrino Observatory$$x0
000434628 7001_ $$0P:(DE-H253)PIP1014130$$aAckermann, Markus$$b1$$udesy
000434628 7001_ $$aAdams, J.$$b2
000434628 7001_ $$aAguilar, J. A.$$b3
000434628 7001_ $$aAhlers, M.$$b4
000434628 7001_ $$aAhrens, M.$$b5
000434628 7001_ $$aAlispach, C.$$b6
000434628 7001_ $$aAndeen, K.$$b7
000434628 7001_ $$aAnderson, T.$$b8
000434628 7001_ $$aAnsseau, I.$$b9
000434628 7001_ $$aAnton, G.$$b10
000434628 7001_ $$aArgüelles, C.$$b11
000434628 7001_ $$aAuffenberg, J.$$b12
000434628 7001_ $$aAxani, S.$$b13
000434628 7001_ $$aBackes, P.$$b14
000434628 7001_ $$aBagherpour, H.$$b15
000434628 7001_ $$aBai, X.$$b16
000434628 7001_ $$aBarbano, A.$$b17
000434628 7001_ $$aBarwick, S. W.$$b18
000434628 7001_ $$aBaum, V.$$b19
000434628 7001_ $$aBay, R.$$b20
000434628 7001_ $$aBeatty, J. J.$$b21
000434628 7001_ $$aBecker, K. H.$$b22
000434628 7001_ $$aTjus, J. Becker$$b23
000434628 7001_ $$aBenZvi, S.$$b24
000434628 7001_ $$aBerley, D.$$b25
000434628 7001_ $$0P:(DE-H253)PIP1003794$$aBernardini, E.$$b26
000434628 7001_ $$aBesson, D. Z.$$b27
000434628 7001_ $$aBinder, G.$$b28
000434628 7001_ $$aBindig, D.$$b29
000434628 7001_ $$aBlaufuss, E.$$b30
000434628 7001_ $$aBlot, S.$$b31
000434628 7001_ $$aBohm, C.$$b32
000434628 7001_ $$aBörner, M.$$b33
000434628 7001_ $$aBöser, S.$$b34
000434628 7001_ $$aBotner, O.$$b35
000434628 7001_ $$aBourbeau, E.$$b36
000434628 7001_ $$aBourbeau, J.$$b37
000434628 7001_ $$0P:(DE-H253)PIP1022296$$aBradascio, F.$$b38$$udesy
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000434628 7001_ $$0P:(DE-H253)PIP1025604$$aBrostean-Kaiser, J.$$b42$$udesy
000434628 7001_ $$aBurgman, A.$$b43
000434628 7001_ $$aBusse, R. S.$$b44
000434628 7001_ $$aCarver, T.$$b45
000434628 7001_ $$aChen, C.$$b46
000434628 7001_ $$aCheung, E.$$b47
000434628 7001_ $$aChirkin, D.$$b48
000434628 7001_ $$aClark, K.$$b49
000434628 7001_ $$aClassen, L.$$b50
000434628 7001_ $$aCollin, G. H.$$b51
000434628 7001_ $$aConrad, J. M.$$b52
000434628 7001_ $$aCoppin, P.$$b53
000434628 7001_ $$aCorrea, P.$$b54
000434628 7001_ $$aCowen, D. F.$$b55
000434628 7001_ $$aCross, R.$$b56
000434628 7001_ $$aDave, P.$$b57
000434628 7001_ $$aAndré, J. P. A. M.$$b58
000434628 7001_ $$aClercq, C.$$b59
000434628 7001_ $$aDeLaunay, J. J.$$b60
000434628 7001_ $$aDembinski, H.$$b61
000434628 7001_ $$aDeoskar, K.$$b62
000434628 7001_ $$aRidder, S.$$b63
000434628 7001_ $$aDesiati, P.$$b64
000434628 7001_ $$aVries, K. D.$$b65
000434628 7001_ $$aWasseige, G.$$b66
000434628 7001_ $$aWith, M.$$b67
000434628 7001_ $$aDeYoung, T.$$b68
000434628 7001_ $$aDiaz, A.$$b69
000434628 7001_ $$aDíaz-Vélez, J. C.$$b70
000434628 7001_ $$aDujmovic, H.$$b71
000434628 7001_ $$aDunkman, M.$$b72
000434628 7001_ $$aDvorak, E.$$b73
000434628 7001_ $$aEberhardt, B.$$b74
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000434628 7001_ $$aEller, P.$$b77
000434628 7001_ $$0P:(DE-HGF)0$$aEvans, J. J.$$b78$$eCorresponding author
000434628 7001_ $$aEvenson, P. A.$$b79
000434628 7001_ $$aFahey, S.$$b80
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000434628 7001_ $$aFritz, A.$$b87
000434628 7001_ $$aGaisser, T. K.$$b88
000434628 7001_ $$aGallagher, J.$$b89
000434628 7001_ $$aGanster, E.$$b90
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000434628 7001_ $$aGerhardt, L.$$b92
000434628 7001_ $$aGhorbani, K.$$b93
000434628 7001_ $$aGlauch, T.$$b94
000434628 7001_ $$aGlüsenkamp, T.$$b95
000434628 7001_ $$aGoldschmidt, A.$$b96
000434628 7001_ $$aGonzalez, J. G.$$b97
000434628 7001_ $$aGrant, D.$$b98
000434628 7001_ $$aGriffith, Z.$$b99
000434628 7001_ $$aGünder, M.$$b100
000434628 7001_ $$aGündüz, M.$$b101
000434628 7001_ $$aHaack, C.$$b102
000434628 7001_ $$aHallgren, A.$$b103
000434628 7001_ $$aHalve, L.$$b104
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000434628 7001_ $$aXu, D. L.$$b329
000434628 7001_ $$aXu, X. W.$$b330
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000434628 7001_ $$aYanez, J. P.$$b332
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000434628 7001_ $$aYoshida, S.$$b334
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000434628 7001_ $$0P:(DE-HGF)0$$aIcecube collaboration$$b336$$eCollaboration author
000434628 773__ $$0PERI:(DE-600)1459069-4$$a10.1140/epjc/s10052-019-7555-0$$gVol. C80, no. 1, p. 9$$n1$$p9$$tThe European physical journal / C$$vC80$$x1434-6052$$y2020
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