6533b839fe1ef96bd12a5cfb
RESEARCH PRODUCT
Multiyear search for a diffuse flux of muon neutrinos with AMANDA-II
H. LandsmanS. SchlenstedtJ. L. KelleyJohn ClemD. RutledgeC. WiedemannH. LeichD. J. BoersmaR. PorrataKonstancja SataleckaD. HaysJenni AdamsL. GerhardtGeorge JaparidzeJ. AuffenbergC. HaK. RawlinsHakki ÖGelmanS. H. SeoJ.d. ZornozaJ.d. ZornozaD. LeierChristian SpieringKara HoffmanY. SestayoSubir SarkarA. J. SmithR. G. StokstadWolfgang RhodeA. MeliR. WischnewskiB. HommezDelia TosiJames MadsenSoebur RazzaqueP. B. PriceW. WagnerJoseph T. HodgesJustin VandenbrouckeT. BurgessA. PiegsaM. SolarzJ. M. JosephI. LiubarskyPh. HerquetN. KitamuraB. ChristyK. MaseA. IshiharaT. O. B. SchmidtJ. BolmontR. EhrlichKael HansonA. OlivasTeresa MontaruliTeresa MontaruliT. J. SumnerG. KohnenS. GrullonR. M. GunasinghaL. DemirörsElisa ResconiM. RibordyE. BlaufussS. BöserJ. E. HartS. SeunarineF. RothmaierMichael StamatikosMichael StamatikosA. MoreyK. BeattieB. D. FoxKurt WoschnaggPaul EvensonP. BerghausP. BerghausT. KowarikK. HultqvistR. W. EllsworthJ. A. GoodmanFabian KislatN. Van EijndhovenR. MorseK. HelbingA. FranckowiakAlbrecht KarleYi WangPaolo DesiatiGerald PrzybylskiM. InabaD. Z. BessonT. MccauleyA. Van OverloopDmitry ChirkinS. RobbinsM. C. StouferJ. PretzM. KrasbergH. WaldmannS. M. MovitV. ViscomiS. PattonB. VoigtXinhua BaiAlexander KappesAlexander KappesM. HellwigHermann KolanoskiR. GozziniP. MeszarosJ. DreyerK. HanM. LabareA. W. JonesElisa BernardiniK. H. SulankeH. G. SanderP. RothA. TepeTodor StanevS. YoshidaOlga BotnerA. MokhtaraniDawn WilliamsK. HoshinaCarlos Pena-garayC. WendtJohan LundbergGlenn SpiczakO. TarasovaH. MiyamotoJohn S. GallagherM. TluczykontChad FinleyD. BertrandD. F. CowenJ. K. BeckerChristian BohmDavid A. SchneiderJ.p. HulssH. KawaiR. GanugapatiA. C. PohlA. C. PohlJ. E. SopherS. R. KleinD. BerleyG. C. HillA. AchterbergB. HugheyD. SeckelK. KuehnW. R. EdwardsHeiko GeenenA. R. FazelyR. FrankeTyce DeyoungP. A. ToaleM. GurtnerC. WalckT. KargM. M. FoersterS. KlepserH. A. B. JohanssonT. HauschildtThomas K. GaisserG. B. YodhIgnacio TaboadaAdam BouchtaC.p. De Los HerosAllan HallgrenT. CastermansR. J. LauerC. De ClercqD. R. NygrenS. HundertmarkMarek KowalskiMarkus AckermannT. StezelbergerS. W. BarwickG. W. SullivanH. S. MatisM. V. D'agostinoC. SongD. TurcanF. DescampsFrancis HalzenO. FadiranC. T. DayM. WalterA. RizzoE. A. StrahlerT. MessariusA. GrossA. SilvestriKaren AndeenR. NahnhauerJ. AhrensAnna DavourJ. BraunJanet JacobsenP. O. HulthJ. EischB. SemburgDamian PielothD. HubertH. WissingL. KöpkeKirill FilimonovT. StraszheimM. R. DuvoortB. BaretS. TilavY. HasegawaK. H. KampertC. P. McparlandJ. LünemannA. GoldschmidtD. HardtkeR. C. BayK.-h. BeckerJuan Carlos Diaz-velezS. StoyanovDirk RyckboschCarsten RottK. MünichJ. W. NamL. ThollanderXianwu XuJ. P. DummReina H. MaruyamaH. WiebuschR. HardtkeP. NiessenJohn HeiseT. BeckaG. WikströmT. Grieselsubject
Astroparticle physicsPhysicsNuclear and High Energy PhysicsRange (particle radiation)MuonPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)High Energy Physics::PhenomenologyFOS: Physical sciencesFluxCosmic rayAstrophysicsAstrophysicsSpectral lineAstronomiaNeutron detectionddc:530High Energy Physics::ExperimentNeutrinodescription
A search for TeV - PeV muon neutrinos from unresolved sources was performed on AMANDA-II data collected between 2000 and 2003 with an equivalent livetime of 807 days. This diffuse analysis sought to find an extraterrestrial neutrino flux from sources with non-thermal components. The signal is expected to have a harder spectrum than the atmospheric muon and neutrino backgrounds. Since no excess of events was seen in the data over the expected background, an upper limit of E^{2}\Phi_{90% C.L.} < 7.4 x 10^{-8} GeV cm^{-2} s^{-1} sr^{-1} is placed on the diffuse flux of muon neutrinos with a \Phi \propto E^{-2} spectrum in the energy range 16 TeV to 2.5 PeV. This is currently the most sensitive \Phi \propto E^{-2} diffuse astrophysical neutrino limit. We also set upper limits for astrophysical and prompt neutrino models, all of which have spectra different than \Phi \propto E^{-2}.
year | journal | country | edition | language |
---|---|---|---|---|
2007-05-09 |