Home > Publications database > Development of an analysis to probe the neutrino mass ordering with atmospheric neutrinos using three years of IceCube DeepCore data > print

001     434628
005     20250729150051.0
024 7 _ |a 10.1140/epjc/s10052-019-7555-0
|2 doi
024 7 _ |a Aartsen:2020myq
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024 7 _ |a inspire:1774280
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024 7 _ |a 1434-6044
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024 7 _ |a 1434-6052
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024 7 _ |a altmetric:73591454
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024 7 _ |a WOS:000511722800001
|2 WOS
024 7 _ |a 10.3204/PUBDB-2020-00189
|2 datacite_doi
024 7 _ |a openalex:W2997107489
|2 openalex
037 _ _ |a PUBDB-2020-00189
041 _ _ |a English
082 _ _ |a 530
100 1 _ |a Aartsen, M. G.
|b 0
245 _ _ |a Development of an analysis to probe the neutrino mass ordering with atmospheric neutrinos using three years of IceCube DeepCore data
260 _ _ |a Heidelberg
|c 2020
|b Springer
336 7 _ |a article
|2 DRIVER
336 7 _ |a Output Types/Journal article
|2 DataCite
336 7 _ |a Journal Article
|b journal
|m journal
|0 PUB:(DE-HGF)16
|s 1587070134_31771
|2 PUB:(DE-HGF)
336 7 _ |a ARTICLE
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336 7 _ |a JOURNAL_ARTICLE
|2 ORCID
336 7 _ |a Journal Article
|0 0
|2 EndNote
500 _ _ |a © The Author(s)
520 _ _ |a The 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.
536 _ _ |a 613 - Matter and Radiation from the Universe (POF3-613)
|0 G:(DE-HGF)POF3-613
|c POF3-613
|f POF III
|x 0
588 _ _ |a Dataset connected to CrossRef, INSPIRE
650 _ 7 |a neutrino: atmosphere
|2 autogen
650 _ 7 |a neutrino: mass
|2 autogen
650 _ 7 |a IceCube: upgrade
|2 autogen
650 _ 7 |a matter: effect
|2 autogen
650 _ 7 |a experimental results
|2 autogen
650 _ 7 |a oscillation
|2 autogen
650 _ 7 |a signature
|2 autogen
650 _ 7 |a PINGU
|2 autogen
650 _ 7 |a 5/3
|2 autogen
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700 1 _ |a Ackermann, Markus
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773 _ _ |a 10.1140/epjc/s10052-019-7555-0
|g Vol. C80, no. 1, p. 9
|0 PERI:(DE-600)1459069-4
|n 1
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|t The European physical journal / C
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|y 2020
|x 1434-6052
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