6533b7defe1ef96bd127672a
RESEARCH PRODUCT
CNO and pep solar neutrino measurements and perspectives in Borexino
Denis KorablevG. BelliniA. PocarA. VishnevaM. D. SkorokhvatovM. D. SkorokhvatovMichael WurmMatthias LaubensteinD. A. SemenovO. SmirnovE. V. HungerfordAlessandra ReY. SuvorovY. SuvorovM. KaiserCristiano GalbiatiLivia LudhovaJ. ThurnA. SotnikovA. M. GorettiA. S. ChepurnovR. RoncinAndrea IanniD. BickSandra ZavatarelliE. V. UnzhakovL. PerassoS. ManeckiB. LehnertAldo IanniR. TartagliaMatteo AgostiniA.v. EtenkoD. BravoJay Burton BenzigerF. LombardiKai ZuberS. AppelV. N. MuratovaA. RazetoW. ManeschgE. MeroniC. GhianoS. WeinzG. TesteraCaren HagnerD. KrynM. S. MeyerZ. YokleyLino MiramontiG. LukyanchenkoG. LukyanchenkoMarcin WójcikI. S. DrachnevP. J. MosteiroMichele MontuschiP. CavalcanteG. ZuzelA. V. DerbinR. B. VogelaarM. MisiaszekGioacchino RanucciM. GromovLothar OberauerK. JedrzejczakS. SchönertMarco GiammarchiPaolo LombardiE. LitvinovichE. LitvinovichN. RossiAldo RomaniL. Di NotoM. ObolenskyS. DaviniB. CaccianigaI. N. MachulinI. N. MachulinS. MarcocciM. ToropovaA. CaminataMarco PallaviciniD. D'angeloF. GabrieleS. V. SukhotinO. ZaimidorogaH. WangV. V. KobychevG. BonfiniFrank CalapriceHardy SimgenB. NeumairG. KorgaK. FomenkoF. Von FeilitzschL. PappFausto OrticaM. Goeger-neffJ. WinterD. Francosubject
model: solarHistoryneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical Phenomena7. Clean energy01 natural sciencesEducationNuclear physicsPhysics and Astronomy (all)talk: Moscow 2015/10/050103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Astrophysics::Solar and Stellar Astrophysicsddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNeutrino oscillationBorexinoMSW effectPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologySolar neutrino problemComputer Science ApplicationsMassless particleNeutrino detector13. Climate actionHigh Energy Physics::ExperimentBorexinoneutrino: oscillationNeutrinoLeptonexperimental resultsdescription
International audience; The detection of neutrinos emitted in the CNO reactions in the Sun is one of the ambitious goals of Borexino Phase-II. A measurement of CNO neutrinos would be a milestone in astrophysics, and would allow to solve serious issues in current solar models. A precise measurement of the rate of neutrinos from the pep reaction would allow to investigate neutrino oscillations in the MSW transition region. The pep and CNO solar neutrino physics, the measurement in Borexino Phase-I and the perspectives for the new phase are reviewed in this proceeding.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2015-10-05 |