Search results for "Astrophysics"

showing 10 items of 8341 documents

Decaying sterile neutrinos and the short baseline oscillation anomalies

2019

The MiniBooNE experiment has observed a significant excess of electron neutrinos in a muon neutrino beam at source-detector distances too short to be compatible with standard neutrino oscillations. The most straightforward explanation for this signal in terms of oscillations between Standard Model neutrinos and a new, sterile, neutrino, is disfavored by null results from experiments looking for muon neutrino disappearance. Here, we discuss the possibility that MiniBooNE data are instead explained by a sterile neutrino that decays quickly back into active neutrinos plus a light boson. The flavor composition of the secondary neutrinos is determined by the sterile neutrino mixing angles, and w…

Sterile neutrinoParticle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesElectron7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentMiniBooNEHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesMuon neutrino010306 general physicsNeutrino oscillationParticle Physics - PhenomenologyBosonPhysicshep-ex010308 nuclear & particles physicsOscillationHigh Energy Physics::Phenomenologyhep-ph3. Good healthHigh Energy Physics - PhenomenologyHigh Energy Physics::ExperimentNeutrinoParticle Physics - ExperimentPhysical Review D
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Recent Borexino results and prospects for the near future

2015

The Borexino experiment, located in the Gran Sasso National Laboratory, is an organic liquid scintillator detector conceived for the real time spectroscopy of low energy solar neutrinos. The data taking campaign phase I (2007 - 2010) has allowed the first independent measurements of 7Be, 8B and pep fluxes as well as the first measurement of anti-neutrinos from the earth. After a purification of the scintillator, Borexino is now in phase II since 2011. We review here the recent results achieved during 2013, concerning the seasonal modulation in the 7Be signal, the study of cosmogenic backgrounds and the updated measurement of geo-neutrinos. We also review the upcoming measurements from phase…

Sterile neutrinoPhysics - Instrumentation and Detectorsneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoQC1-999Astrophysics::High Energy Astrophysical Phenomenascintillation counter: liquidFOS: Physical sciencesScintillator53001 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Physics and Astronomy (all)Low energy[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physics[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]BorexinoPhysics010308 nuclear & particles physicsneutrino: energy: lowgeophysicsbackgroundPhysicsDetectorneutrino: flux: measuredHigh Energy Physics::PhenomenologyInstrumentation and Detectors (physics.ins-det)neutrino: particle sourceneutrino: sterileantineutrinoGran SassoNEUTRINOS13. Climate actionBorexinoHigh Energy Physics::ExperimentNeutrinoNational laboratory
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EV-Scale Sterile Neutrino Search Using Eight Years of Atmospheric Muon Neutrino Data from the IceCube Neutrino Observatory

2020

Physical review letters 125(14), 141801 (1-11) (2020). doi:10.1103/PhysRevLett.125.141801

Sterile neutrinoPhysics::Instrumentation and DetectorsGeneral Physics and Astronomysterile [neutrino]01 natural sciencesCosmologyIceCubeHigh Energy Physics - ExperimentSubatomär fysikHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Astronomi astrofysik och kosmologiSubatomic PhysicsTOOLAstronomy Astrophysics and Cosmologyatmosphere [muon]Muon neutrinoPhysicsPhysicsoscillation [neutrino]Astrophysics::Instrumentation and Methods for Astrophysicshep-phneutrino: sterilemass difference [neutrino]ddc:muon: atmosphereobservatoryHigh Energy Physics - PhenomenologyPhysique des particules élémentairessignatureParticle physicsdata analysis methodScale (ratio)Astrophysics::High Energy Astrophysical Phenomenaneutrino: mass differenceFOS: Physical sciences530IceCube Neutrino Observatorystatistical analysis0103 physical sciencesOSCILLATIONSddc:530010306 general physicshep-exICEHigh Energy Physics::Phenomenologyneutrino: mixing angleCONVERSIONPhysics and AstronomyCOSMOLOGYHigh Energy Physics::Experimentneutrino: oscillationBAYESIAN-INFERENCEmixing angle [neutrino]experimental results
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"Table 1" of "D_s meson production at central rapidity in proton--proton collisions at sqrt(s) = 7 TeV"

2014

pT-differential inclusive cross section in |y| < 0.5 for prompt D_s^+ meson production in pp collisions at sqrt(s) = 7 TeV.

Strange productionHigh Energy Physics::LatticeAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::Phenomenology7000.0P P --> D/S+ XInclusiveSingle Differential Cross SectionProton-Proton ScatteringCharm productionHigh Energy Physics::ExperimentDSIG/DPTNuclear ExperimentTransverse Momentum Dependence
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"Table 2" of "D_s meson production at central rapidity in proton--proton collisions at sqrt(s) = 7 TeV"

2014

pT-integrated inclusive cross section in |y| < 0.5 for prompt D_s^+ meson production in pp collisions at sqrt(s) = 7 TeV. The latter three systematic uncertainties arise from extrapolating the visible cross section to the full pT range, luminosity, and the branching ratio, respectively.

Strange productionHigh Energy Physics::LatticeAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyIntegrated Cross Section7000.0P P --> D/S+ XCross SectionSIGInclusiveProton-Proton ScatteringCharm productionHigh Energy Physics::ExperimentNuclear Experiment
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"Table 2" of "A study of strange particle production in nu/mu charged current interactions in the NOMAD experiment."

2002

Measured yields as a function of E, the neutrino energy.

Strange productionPhysics::Instrumentation and DetectorsNUMU NUCLEON --> MU- KS XAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyDeep Inelastic ScatteringNUMU NUCLEON --> MU- LAMBDA XMuon productionMULTInclusive3.203-16.801NUMU NUCLEON --> MU- LAMBDABAR XHigh Energy Physics::ExperimentCharged Current
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"Table 6" of "Identified Charged Particles in Quark and Gluon Jets"

2003

Jet flavor tagging is used. (C=DUSCB), (C=DUSC), (C=UDS) mean quark-jet flavors. CONST(C=GLUON/JET) is the ratio gluon/jet for all charged particles. 'Mercedes' events, three-fold symmetric events, the angle between three jets is 120 +- 15 deg.

Strange productionQUARK --> K+ XAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::LatticeNuclear TheoryHigh Energy Physics::PhenomenologyQUARK --> K- XE+ E- --> QUARK QUARKBAR GLUON91.2MULTInclusiveGLUON --> K- XQUARKBAR --> K+ XE+ E- ScatteringExclusiveHigh Energy Physics::ExperimentGLUON --> K+ XQUARKBAR --> K- XMULT/MULT
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"Table 2" of "Identified Charged Particles in Quark and Gluon Jets"

2003

Jet flavor tagging is used. (C=DUSCB), (C=DUSC), (C=UDS) mean quark-jet flavors. CONST(C=GLUON/JET) is the ratio gluon/jet for all charged particles. 'Y' events, mirror symmetric events, the angle between the most energetic jet and other two jets is 150 +- 15 deg.

Strange productionQUARK --> K+ XHigh Energy Physics::LatticeAstrophysics::High Energy Astrophysical PhenomenaNuclear TheoryHigh Energy Physics::PhenomenologyQUARK --> K- XE+ E- --> QUARK QUARKBAR GLUON91.2MULTInclusiveGLUON --> K- XQUARKBAR --> K+ XE+ E- ScatteringExclusiveHigh Energy Physics::ExperimentGLUON --> K+ XQUARKBAR --> K- XMULT/MULT
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Narrow Bound States of the DNN System

2012

We report on a recent calculation of the properties of the $DNN$ system, a charmed meson with two nucleons. The system is analogous to the $\bar K NN$ system substituting a strange quark by a charm quark. Two different methods are used to evaluate the binding and width, the Fixed Center approximation to the Faddeev equations and a variational calculation. In both methods we find that the system is bound by about 200 MeV and the width is smaller than 40 MeV, a situation opposite to the one of the $\bar K NN$ system and which makes this state well suited for experimental observation.

Strange quarkFaddeev equationsParticle physicsMesonNuclear TheoryBar (music)Nuclear TheoryFOS: Physical sciences01 natural sciencesCharm quarkNuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesBound stateNuclear Experiment010303 astronomy & astrophysicsPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaState (functional analysis)16. Peace & justiceAtomic and Molecular Physics and OpticsHigh Energy Physics - PhenomenologyHigh Energy Physics::ExperimentNucleon
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Cosmological origin of anomalous radio background

2012

The ARCADE 2 collaboration has reported a significant excess in the isotropic radio background, whose homogeneity cannot be reconciled with clustered sources. This suggests a cosmological origin prior to structure formation. We investigate several potential mechanisms and show that injection of relativistic electrons through late decays of a metastable particle can give rise to the observed excess radio spectrum through synchrotron emission. However, constraints from the cosmic microwave background (CMB) anisotropy, on injection of charged particles and on the primordial magnetic field, present a challenge. The simplest scenario is with a greater than or similar to 9 GeV particle decaying i…

Structure formationCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaDark matterCosmic microwave backgroundCosmic background radiationFOS: Physical sciencesAstrophysicsElectronAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesParticle decayHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010303 astronomy & astrophysicsPhysicsdark matter theory010308 nuclear & particles physicsFísicaAstronomy and AstrophysicsCosmology of Theories beyond the SMRedshiftCharged particleHigh Energy Physics - Phenomenologyextragalactic magnetic fieldsAstrophysics - Cosmology and Nongalactic Astrophysics
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