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000596423 005__ 20250720041100.0
000596423 0247_ $$2doi$$a10.1140/epjc/s10052-023-11679-5
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000596423 0247_ $$2ISSN$$a1434-6044
000596423 0247_ $$2ISSN$$a1434-6052
000596423 0247_ $$2arXiv$$aarXiv:2303.04682
000596423 0247_ $$2datacite_doi$$a10.3204/PUBDB-2023-06151
000596423 0247_ $$2WOS$$aWOS:001063424400001
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000596423 037__ $$aPUBDB-2023-06151
000596423 041__ $$aEnglish
000596423 082__ $$a530
000596423 088__ $$2arXiv$$aarXiv:2303.04682
000596423 1001_ $$aAbbasi, R.$$b0
000596423 245__ $$aObservation of seasonal variations of the flux of high-energy atmospheric neutrinos with IceCube
000596423 260__ $$aHeidelberg$$bSpringer$$c2023
000596423 3367_ $$2DRIVER$$aarticle
000596423 3367_ $$2DataCite$$aOutput Types/Journal article
000596423 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$bjournal$$mjournal$$s1696938255_278285
000596423 3367_ $$2BibTeX$$aARTICLE
000596423 3367_ $$2ORCID$$aJOURNAL_ARTICLE
000596423 3367_ $$00$$2EndNote$$aJournal Article
000596423 500__ $$aPreprint submitted to EPJC
000596423 520__ $$aAtmospheric muon neutrinos are produced by meson decays in cosmic-ray-induced air showers. The flux depends on meteorological quantities such as the air temperature, which affects the density of air. Competition between decay and re-interaction of those mesons in the first particle production generations gives rise to a higher neutrino flux when the air density in the stratosphere is lower, corresponding to a higher temperature. A measurement of a temperature dependence of the atmospheric $\nu _{\mu }$ flux provides a novel method for constraining hadronic interaction models of air showers. It is particularly sensitive to the production of kaons. Studying this temperature dependence for the first time requires a large sample of high-energy neutrinos as well as a detailed understanding of atmospheric properties. We report the significant ($> 10 \; \sigma $) observation of a correlation between the rate of more than 260,000 neutrinos, detected by IceCube between 2012 and 2018, and atmospheric temperatures of the stratosphere, measured by the Atmospheric Infrared Sounder (AIRS) instrument aboard NASA’s AQUA satellite. For the observed 10$\%$ seasonal change of effective atmospheric temperature we measure a 3.5(3)$\%$ change in the muon neutrino flux. This observed correlation deviates by about 2-3 standard deviations from the expected correlation of 4.3$\%$ as obtained from theoretical predictions under the assumption of various hadronic interaction models.
000596423 536__ $$0G:(DE-HGF)POF4-613$$a613 - Matter and Radiation from the Universe (POF4-613)$$cPOF4-613$$fPOF IV$$x0
000596423 588__ $$aDataset connected to CrossRef, INSPIRE, Journals: bib-pubdb1.desy.de
000596423 650_7 $$2INSPIRE$$ainteraction: model
000596423 650_7 $$2INSPIRE$$aatmosphere: temperature
000596423 650_7 $$2INSPIRE$$aneutrino: flux
000596423 650_7 $$2INSPIRE$$ashowers: atmosphere
000596423 650_7 $$2INSPIRE$$atemperature: high
000596423 650_7 $$2INSPIRE$$ameson: decay
000596423 650_7 $$2INSPIRE$$aK: production
000596423 650_7 $$2INSPIRE$$ainteraction
000596423 650_7 $$2INSPIRE$$aair: temperature
000596423 650_7 $$2INSPIRE$$acorrelation
000596423 650_7 $$2INSPIRE$$amuon
000596423 650_7 $$2INSPIRE$$adensity
000596423 650_7 $$2INSPIRE$$atemperature dependence
000596423 650_7 $$2INSPIRE$$aIceCube
000596423 650_7 $$2INSPIRE$$asatellite
000596423 650_7 $$2INSPIRE$$ainfrared
000596423 693__ $$0EXP:(DE-H253)IceCube-20150101$$5EXP:(DE-H253)IceCube-20150101$$eIceCube South Pole Neutrino Observatory$$x0
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000596423 7001_ $$aAdams, J.$$b2
000596423 7001_ $$aAgarwalla, S. K.$$b3
000596423 7001_ $$aAggarwal, N.$$b4
000596423 7001_ $$aAguilar, J. A.$$b5
000596423 7001_ $$aAhlers, M.$$b6
000596423 7001_ $$aAlameddine, J. M.$$b7
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000596423 7001_ $$aAnton, G.$$b10
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000596423 7001_ $$aAxani, S. N.$$b14
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000596423 7001_ $$aBeatty, J. J.$$b21
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000596423 7001_ $$aBecker Tjus, J.$$b23
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