6533b821fe1ef96bd127c3c9

RESEARCH PRODUCT

Searches for Sterile Neutrinos with the IceCube Detector

M. G. AartsenK. AbrahamI. AnsseauD. GóraD. GrantZ. GriffithA. Haj IsmailA. HallgrenF. HalzenE. HansenK. HansonD. HebeckerD. HeeremanG. AntonK. HelbingR. HellauerS. HickfordJ. HignightG. C. HillK. D. HoffmanR. HoffmannK. HolzapfelA. HomeierK. HoshinaM. ArchingerF. HuangM. HuberW. HuelsnitzK. HultqvistS. InA. IshiharaE. JacobiG. S. JaparidzeM. JeongK. JeroC. ArgüellesB. J. P. JonesM. JurkovicA. KappesT. KargA. KarleU. KatzM. KauerA. KeivaniJ. L. KelleyA. KheirandishT. C. ArlenM. KimT. KintscherJ. KirylukT. KittlerS. R. KleinG. KohnenR. KoiralaH. KolanoskiL. KöpkeC. KopperJ. AuffenbergS. KopperD. J. KoskinenM. KowalskiK. KringsM. KrollG. KrücklC. KrügerJ. KunnenS. KunwarN. KurahashiS. AxaniT. KuwabaraM. LabareJ. L. LanfranchiM. J. LarsonD. LennarzM. Lesiak-bzdakM. LeuermannL. LuJ. LünemannJ. MadsenX. BaiG. MaggiK. B. M. MahnS. MancinaM. MandelartzR. MaruyamaK. MaseR. MaunuF. McnallyK. MeagherM. MediciS. W. BarwickM. MeierA. MeliT. MenneG. MerinoT. MeuresS. MiareckiE. MiddellL. MohrmannT. MontaruliM. MoulaiV. BaumR. NahnhauerU. NaumannG. NeerH. NiederhausenS. C. NowickiD. R. NygrenA. Obertacke PollmannA. OlivasA. OmairatA. O’murchadhaM. AckermannR. BayT. PalczewskiH. PandyaD. V. PankovaJ. A. PepperC. Pérez De Los HerosC. PfendnerD. PielothE. PinatJ. PosseltP. B. PriceJ. J. BeattyG. T. PrzybylskiM. QuinnanC. RaabM. RameezK. RawlinsM. RelichE. ResconiW. RhodeM. RichmanB. RiedelJ. Becker TjusS. RobertsonC. RottT. RuheD. RyckboschD. RysewykL. SabbatiniJ. SalvadoS. E. Sanchez HerreraA. SandrockJ. SandroosK.-h. BeckerS. SarkarK. SataleckaP. SchlunderT. SchmidtS. SchönebergA. SchönwaldD. SeckelS. SeunarineD. SoldinM. SongS. BenzviG. M. SpiczakC. SpieringM. StamatikosT. StanevA. StasikA. SteuerT. StezelbergerR. G. StokstadA. StößlR. StrömP. BerghausN. L. StrotjohannG. W. SullivanM. SutherlandH. TaavolaI. TaboadaJ. TatarS. Ter-antonyanA. TerliukG. TešićS. TilavD. BerleyP. A. ToaleM. N. TobinS. ToscanoD. TosiM. TselengidouA. TurcatiE. UngerM. UsnerS. VallecorsaJ. VandenbrouckeE. BernardiniN. Van EijndhovenS. VanheuleM. Van RossemJ. Van SantenJ. VeenkampM. VogeM. VraegheC. WalckA. WallaceN. WandkowskyA. BernhardCh. WeaverC. WendtS. WesterhoffB. J. WhelanK. WiebeL. WilleD. R. WilliamsL. WillsH. WissingM. WolfD. Z. BessonT. R. WoodE. WoolseyK. WoschnaggD. L. XuX. W. XuY. XuJ. P. YanezG. YodhS. YoshidaM. ZollJ. AdamsG. BinderIcecube CollaborationD. BindigE. BlaufussS. BlotD. J. BoersmaC. BohmM. BörnerF. BosD. BoseS. BöserJ. A. AguilarO. BotnerJ. BraunL. BrayeurH.-p. BretzA. BurgmanJ. CaseyM. CasierE. CheungD. ChirkinA. ChristovM. AhlersK. ClarkL. ClassenS. CoendersG. H. CollinJ. M. ConradD. F. CowenA. H. Cruz SilvaJ. DaughheteeJ. C. DavisM. DayM. AhrensJ. P. A. M. De AndréC. De ClercqE. Del Pino RosendoH. DembinskiS. De RidderP. DesiatiK. D. De VriesG. De WasseigeM. De WithT. DeyoungD. AltmannJ. C. Díaz-vélezV. Di LorenzoH. DujmovicJ. P. DummM. DunkmanB. EberhardtT. EhrhardtB. EichmannS. EulerP. A. EvensonK. AndeenS. FaheyA. R. FazelyJ. FeintzeigJ. FeldeK. FilimonovC. FinleyS. FlisC.-c. FösigT. FuchsT. K. GaisserT. AndersonR. GaiorJ. GallagherL. GerhardtK. GhorbaniW. GiangL. GladstoneT. GlüsenkampA. GoldschmidtG. GolupJ. G. Gonzalez

subject

Particle physicsSterile neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Physics and Astronomy01 natural sciencesHigh Energy Physics - ExperimentMiniBooNENuclear physicsHigh Energy Physics - Experiment (hep-ex)Physics and Astronomy (all)0103 physical sciencesOSCILLATIONSddc:550Muon neutrino010306 general physicsNeutrino oscillationZenithHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMuon010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyMODELNeutrino detectorPhysics and Astronomy13. Climate actionHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical PhenomenaEnergy (signal processing)SYSTEM

description

The IceCube neutrino telescope at the South Pole has measured the atmospheric muon neutrino spectrum as a function of zenith angle and energy in the approximate 320 GeV to 20 TeV range, to search for the oscillation signatures of light sterile neutrinos. No evidence for anomalous $\nu_\mu$ or $\bar{\nu}_\mu$ disappearance is observed in either of two independently developed analyses, each using one year of atmospheric neutrino data. New exclusion limits are placed on the parameter space of the 3+1 model, in which muon antineutrinos would experience a strong MSW-resonant oscillation. The exclusion limits extend to $\mathrm{sin}^2 2\theta_{24} \leq$ 0.02 at $\Delta m^2 \sim$ 0.3 $\mathrm{eV}^2$ at the 90\% confidence level. The allowed region from global analysis of appearance experiments, including LSND and MiniBooNE, is excluded at approximately the 99\% confidence level for the global best fit value of $|$U$_{e4}|^2$.

10.1103/physrevlett.117.071801https://doi.org/10.1103/physrevlett.117.071801