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2026-05-07
Sensitivity Projections for Low-Mass Dark Matter Annihilation with the IceCube Upgrade
R. AbbasiM. AckermannJ. AdamsJ. A. AguilarM. AhlersJ. M. AlameddineS. AliN. M. AminK. AndeenC. ArgüellesY. AshidaS. AthanasiadouS. N. AxaniR. BabuX. BaiA. Balagopal V.S. W. BarwickV. BasuR. BayJ. J. BeattyJ. Becker TjusP. BehrensJ. BeiseC. BellenghiS. BenkelS. BenZviD. BerleyE. BernardiniD. Z. BessonE. BlaufussL. BloomS. BlotF. BontempoJ. Y. Book MotzkinC. Boscolo MeneguoloS. BöserO. BotnerJ. BöttcherJ. BraunB. BrinsonZ. Brisson-TsavoussisR. T. BurleyD. ButterfieldK. CarloniJ. CarpioN. ChauY. C. ChenZ. ChenD. ChirkinS. ChoiA. ChubarovB. A. ClarkG. H. CollinD. A. Coloma BorjaA. ConnollyJ. M. ConradD. F. CowenC. De ClercqJ. J. DeLaunayD. DelgadoT. DelmeulleS. DengP. DesiatiK. D. de VriesG. de WasseigeT. DeYoungJ. C. Díaz-VélezS. DiKerbyT. DingM. DittmerA. DomiL. DraperL. DueserD. DurnfordK. DuttaM. A. DuVernoisT. EhrhardtL. EidenschinkA. EimerC. EldridgeP. EllerE. EllingerD. ElsässerR. EngelH. ErpenbeckW. EsmailS. EuligJ. EvansP. A. EvensonK. L. FanK. FangK. FarragA. R. FazelyA. FedynitchN. FeiglC. FinleyD. FoxA. FranckowiakS. FukamiP. FürstJ. GallagherE. GansterA. GarciaM. GarciaE. GentonL. GerhardtA. GhadimiC. GlaserT. GlüsenkampJ. G. GonzalezS. GoswamiA. GranadosD. GrantS. J. GrayS. GriffinK. M. GrothD. GuevelC. GüntherP. GutjahrC. HaA. HallgrenL. HalveF. HalzenL. HamacherM. HandtK. HansonJ. HardinA. A. HarnischP. HatchA. HaungsJ. HäußlerK. HelbingJ. HellrungB. HenkeL. HennigF. HenningsenL. HeuermannR. HewettN. HeyerS. HickfordA. HidvegiC. HillG. C. HillR. HmaidK. D. HoffmanA. HollnagelD. HooperS. HoriK. HoshinaM. HostertW. HouM. HrywniakT. HuberK. HultqvistK. HymonA. IshiharaW. IwakiriM. JacquartS. JainO. JanikM. JanssonM. JinN. KampD. KangW. KangA. KappesL. KardumT. KargA. KarleA. KatilM. KauerJ. L. KelleyM. KhanalA. Khatee ZathulA. KheirandishT. KimH. KimkuF. KirchnerJ. KirylukC. KleinS. R. KleinY. KobayashiS. KochA. KochockiR. KoiralaH. KolanoskiT. KontrimasL. KöpkeC. KopperD. J. KoskinenP. KoundalM. KowalskiT. KozynetsA. KravkaN. KriegerT. KrishnanK. KruiswijkE. KrupczakA. KumarE. KunN. KurahashiC. Lagunas GualdaL. Lallement ArnaudM. J. LarsonF. LauberJ. P. LazarK. Leonard DeHoltonA. LeszczyńskaC. LiJ. LiaoC. LinQ. R. LiuY. T. LiuM. LiubarskaC. LoveL. LuF. LucarelliW. LuszczakY. LyuM. MacdonaldE. MagnusY. MakinoE. ManaoS. MancinaA. MandI. C. MarişS. MarkaZ. MarkaL. MartenI. Martinez-SolerR. MaruyamaJ. MauroF. MayhewF. McNallyK. MeagherA. MedinaM. MeierY. MerckxL. MertenJ. MitchellL. MolchanyS. MondalT. MontaruliR. W. MooreY. MoriiA. MosbruggerD. MousadiE. MoyauxT. MukherjeeM. NakosU. NaumannL. NesteM. NeumannH. NiederhausenM. U. NisaK. NodaA. NoellA. NovikovA. ObertackeV. O'DellA. OlivasR. OrsoeJ. OsbornE. O'SullivanB. OwensV. PalusovaH. PandyaA. ParentiN. ParkV. ParrishE. N. PaudelL. PaulC. Pérez de los HerosT. PerniceT. C. PetersenJ. PetersonS. PickM. PlumA. PonténV. PoojyamB. PriesR. Procter-MurphyG. T. PrzybylskiL. PyrasC. RaabJ. Rack-HelleisN. RadM. RavnK. RawlinsZ. RechavA. RehmanI. ReistrofferE. ResconiC. D. RhoW. RhodeL. RiccaB. RiedelA. RifaieE. J. RobertsS. RodanM. RongenA. RostedC. RottT. RuheL. RuohanD. RyckboschJ. SafferD. Salazar-GallegosP. SampathkumarA. SandrockG. Sanger-JohnsonM. SantanderS. SarkarM. ScarneraM. SchaufelH. SchielerS. SchindlerL. SchlickmannB. SchlüterF. SchlüterN. SchmeisserT. SchmidtA. ScholzF. G. SchröderS. SchwirnS. SclafaniD. SeckelL. SeenM. SeikhS. SeunarineP. A. Sevle MyhrR. ShahS. ShahS. ShefaliN. ShimizuB. SkrzypekR. SnihurJ. SoedingreksoD. SoldinP. SoldinG. SommaniD. SongC. SpannfellnerG. M. SpiczakC. SpieringJ. StachurskaM. StamatikosT. StanevT. StezelbergerT. StürwaldT. StuttardG. W. SullivanI. TaboadaS. Ter-AntonyanA. TerliukA. ThakuriM. ThiesmeyerW. G. ThompsonJ. ThwaitesS. TilavK. TollefsonJ. A. TorresS. ToscanoD. TosiK. UpshawA. VaidyanathanN. Valtonen-MattilaJ. ValverdeJ. VandenbrouckeT. Van EedenN. van EijndhovenL. Van RootselaarJ. van SantenJ. VaraF. VarsiM. VenugopalM. VereeckenS. Vergara CarrascoS. VerpoestD. VeskeA. VijaiJ. VillarrealC. WalckA. WangE. H. S. WarrickC. WeaverP. WeigelA. WeindlJ. WeldertA. Y. WenC. WendtJ. WerthebachM. WeyrauchN. WhitehornC. H. WiebuschD. R. WilliamsL. WitthausG. WredeX. W. XuJ. P. YanezY. YaoE. YildizciS. YoshidaR. YoungF. YuS. YuT. YuanS. Yun-CárcamoA. Zander JurowitzkiA. ZegarelliS. ZhangZ. ZhangP. ZhelninP. ZilbermanC. Zilleruelo Cañas
文献摘要
The IceCube Upgrade, an extension designed to enhance the IceCube Neutrino Observatory’s detection of neutrinos with energies between 1 GeV and 500 GeV, will markedly improve IceCube’s sensitivity to low-mass dark matter scenarios. In this study, we present sensitivity projections for the IceCube Upgrade to neutrino fluxes arising from dark matter annihilation. In particular, we consider dark matter with masses between 3 GeV to 500 GeV from both the core of the Sun and the Galactic Center. These projections indicate that the IceCube Upgrade will enable stringent limits on dark matter in this parameter space, achieving leading sensitivities to some dark matter models with only three years of data taking.
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