Search results for "iNOS"

showing 10 items of 2075 documents

Supersymmetric type-III seesaw mechanism: Lepton flavor violation and LHC phenomenology

2013

We study a supersymmetric version of the type-III seesaw mechanism considering two variants of the model: a minimal version for explaining neutrino data with only two copies of 24 superfields and a model with three generations of 24-plets. The latter predicts, in general, rates for mu -> e gamma inconsistent with experimental data. However, this bound can be evaded if certain special conditions within the neutrino sector are fulfilled. In the case of two 24-plets, lepton flavor violation constraints can be satisfied much more easily. After specifying the corresponding regions in the minimal supergravity parameter space, we show that under favorable conditions one can test the corresponding …

Nuclear and High Energy PhysicsParticle physicsMassesPhysics beyond the Standard Model01 natural sciences0103 physical sciencesRoot-S=7 tev010306 general physicsRight-handed neutrinosPhysicsLarge Hadron ColliderElectroweak010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyElectroweak interactionFísicaNon-conservationSupersymmetrySeesaw mechanismUnificationGrand unified theoriesHigh Energy Physics::ExperimentNeutrinoModel higgs-bosonDecaysPhenomenology (particle physics)LeptonStandard model
researchProduct

Observation and studies of double J/psi production at the Tevatron

2014

We present the observation of doubly-produced $J/\psi$ mesons with the D0 detector at Fermilab in $p\bar{p}$ collisions at $\sqrt{s}=1.96$ TeV. The production cross section for both singly and doubly-produced $J/\psi$ mesons is measured using a sample with an integrated luminosity of 8.1fb$^{-1}$. For the first time, the double $J/\psi$ production cross section is separated into contributions due to single and double parton scatterings. Using these measurements, we determine the effective cross section $\sigma_{eff}$, a parameter characterizing an effective spatial area of the parton-parton interactions and related to the parton spatial density inside the nucleon.

Nuclear and High Energy PhysicsParticle physicsMesonDOUBLE-PARTON SCATTERINGP(P)OVER-BAR COLLISIONSTevatronFOS: Physical sciencesPartonPSI-PSI-PRODUCTIONAstronomy & Astrophysics7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentPhysics Particles & FieldsNuclear physicsHigh Energy Physics - Experiment (hep-ex)Cross section (physics)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Fermilab010306 general physicsNuclear ExperimentRUN-IIPhysicsLuminosity (scattering theory)Science & TechnologyPP COLLISIONS010308 nuclear & particles physicshep-exPhysicsHigh Energy Physics::PhenomenologyExperimental High Energy PhysicsPhysical SciencesComputingMethodologies_DOCUMENTANDTEXTPROCESSINGProduction (computer science)High Energy Physics::ExperimentNucleon
researchProduct

A road map to solar neutrino fluxes, neutrino oscillation parameters, and tests for new physics

2003

We analyze all available solar and related reactor neutrino experiments, as well as simulated future 7Be, p-p, pep, and ^8B solar neutrino experiments. We treat all solar neutrino fluxes as free parameters subject to the condition that the total luminosity represented by the neutrinos equals the observed solar luminosity (the `luminosity constraint'). Existing experiments show that the p-p solar neutrino flux is 1.02 +- 0.02 (1 sigma) times the flux predicted by the BP00 standard solar model; the 7Be neutrino flux is 0.93^{+0.25}_{-0.63} the predicted flux; and the ^8B flux is 1.01 +- 0.04 the predicted flux. The neutrino oscillation parameters are: Delta m^2 = 7.3^{+0.4}_{-0.6}\times 10^{-…

Nuclear and High Energy PhysicsParticle physicsNuclear TheoryPhysics beyond the Standard ModelSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaSolar luminosityFOS: Physical sciencesAstrophysics7. Clean energy01 natural sciencesLuminosityHigh Energy Physics - ExperimentNuclear Theory (nucl-th)High Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNuclear fusionAstrophysics::Solar and Stellar AstrophysicsNuclear Experiment (nucl-ex)010306 general physicsNeutrino oscillationNuclear ExperimentParticle Physics - PhenomenologyPhysicsStandard solar model010308 nuclear & particles physicsAstrophysics (astro-ph)FísicaHigh Energy Physics - PhenomenologyHigh Energy Physics::ExperimentAstrophysics::Earth and Planetary AstrophysicsNeutrino
researchProduct

Solar Neutrinos Before and After Neutrino 2004

2004

We compare, using a three neutrino analysis, the allowed neutrino oscillation parameters and solar neutrino fluxes determined by the experimental data available Before and After Neutrino 2004. New data available after Neutrino2004 include refined KamLAND and gallium measurements. We use six different approaches to analyzing the KamLAND data. We present detailed results using all the available neutrino and anti-neutrino data for Delta m^2_{12}, tan^2 theta_{12}, sin^2 theta_{13}, and sin^2 eta (sterile fraction). Using the same complete data sets, we also present Before and After determinations of all the solar neutrino fluxes, which are treated as free parameters, an upper limit to the lumi…

Nuclear and High Energy PhysicsParticle physicsNuclear TheoryPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciences7. Clean energyLuminosityNuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNuclear Experiment (nucl-ex)010306 general physicsNeutrino oscillationNuclear ExperimentPhysicsStandard solar model010308 nuclear & particles physicsScatteringOscillationAstrophysics (astro-ph)High Energy Physics::PhenomenologyFísicaSigmaHigh Energy Physics - Phenomenology13. Climate actionHigh Energy Physics::ExperimentNeutrino
researchProduct

Observation of charmonium pairs produced exclusively in $pp$ collisions

2014

A search is performed for the central exclusive production of pairs of charmonia produced in proton-proton collisions. Using data corresponding to an integrated luminosity of $3{\rm\ fb}^{-1}$ collected at centre-of-mass energies of 7 and 8 TeV, $J/\psi J/\psi$ and $J/\psi\psi(2S)$ pairs are observed, which have been produced in the absence of any other activity inside the LHCb acceptance that is sensitive to charged particles in the pseudorapidity ranges $(-3.5,-1.5)$ and $(1.5,5.0)$. Searches are also performed for pairs of P-wave charmonia and limits are set on their production. The cross-sections for these processes, where the dimeson system has a rapidity between 2.0 and 4.5, are measu…

Nuclear and High Energy PhysicsParticle physicsNuclear TheorydiffractionFOS: Physical sciencesLHCb - Abteilung HofmannHEAVY-ION COLLISIONSQCD diffraction charmoniaNOHigh Energy Physics - ExperimentLuminosityHigh Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Quantum chromodynamiccharmonia; diffraction; QCDcharmonia; diffraction; QCD; Nuclear and High Energy PhysicsRapiditySDG 7 - Affordable and Clean EnergyNuclear ExperimentQCPhysics/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energyhep-ex12.38.-tParticle physicsHadron-induced high- and super-high-energy interactions (energy > 10 GeV): Inclusive production with identified hadronHEAVY-ION COLLISIONS; 450 GEV/C; DIFFRACTION; LHCQCDCromodinàmica quànticaLHCbDifracció450 GEV/CPseudorapidityPhysics::Accelerator PhysicscharmoniaFísica nuclearHigh Energy Physics::ExperimentProduction (computer science)LHCHEAVYFísica de partículesExperiments13.85.NiDiffractionQuantum chromodynamicsParticle Physics - ExperimentJournal of Physics G: Nuclear and Particle Physics
researchProduct

Atmospheric neutrino oscillations and new physics

2004

We study the robustness of the determination of the neutrino masses and mixing from the analysis of atmospheric and K2K data under the presence of different forms of phenomenologically allowed new physics in the nu_mu--nu_tau sector. We focus on vector and tensor-like new physics interactions which allow us to treat, in a model independent way, effects due to the violation of the equivalence principle, violations of the Lorentz invariance both CPT conserving and CPT violating, non-universal couplings to a torsion field and non-standard neutrino interactions with matter. We perform a global analysis of the full atmospheric data from SKI together with long baseline K2K data in the presence of…

Nuclear and High Energy PhysicsParticle physicsOscillationsPhysics beyond the Standard ModelFOS: Physical sciencesLorentz covariance01 natural sciencesTorsion fieldPartícules (Física nuclear)High Energy Physics - Phenomenology (hep-ph)Robustness (computer science)0103 physical sciencesOscil·lacionsNeutrinsNeutrinos010306 general physicsNeutrino oscillationMixing (physics)Particles (Nuclear physics)PhysicsViolació càrrega-paritat (Física nuclear)010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyHigh Energy Physics - PhenomenologyHigh Energy Physics::ExperimentNeutrinoAtmospheric neutrinoCP violation (Nuclear physics)Physical Review D
researchProduct

Gravitino dark matter and neutrino masses with bilinear R-parity violation

2011

Bilinear R-parity violation provides an attractive origin for neutrino masses and mixings. In such schemes the gravitino is a viable decaying dark matter particle whose R-parity violating decays lead to monochromatic photons with rates accessible to astrophysical observations. We determine the parameter region allowed by gamma-ray line searches, dark matter relic abundance and neutrino oscillation data, obtaining a limit on the gravitino mass $m_{\tilde G} \lsim$ 1-10 GeV corresponding to a relatively low reheat temperature $T_R \lsim$ few $\times 10^7-10^8$ GeV. Neutrino mass and mixing parameters may be reconstructed at accelerator experiments like the Large Hadron Collider.

Nuclear and High Energy PhysicsParticle physicsPhotonAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesMasas de neutrinos01 natural sciencesNuclear physicsHigh Energy Physics - Phenomenology (hep-ph)R-paridad bilinealR-parity0103 physical sciences010306 general physicsNeutrino oscillationLine (formation)PhysicsLarge Hadron Collider010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaHigh Energy Physics - PhenomenologyGravitinoHigh Energy Physics::ExperimentNeutrinoGravitino
researchProduct

Search for charginos nearly mass degenerate with the lightest neutralino in e+e− collisions at centre-of-mass energies up to 209 GeV

2002

A search for charginos nearly mass degenerate with the lightest neutralino is performed with the data collected by the ALEPH detector at LEP, at centre-of-mass energies between 189 and 209 GeV, corresponding to an integrated luminosity of 628 pb-1. The analysis is based on the detection of isolated and energetic initial state radiation photons, produced in association with chargino pairs whose decay products have little visible energy. The number of candidate events observed is in agreement with that expected from Standard Model background sources. These results are combined with those of other direct searches for charginos, and a lower limit of 88 GeV/c2 at 95 % confidence level is derived…

Nuclear and High Energy PhysicsParticle physicsPhotonElectron–positron annihilation01 natural sciencesStandard ModelLuminosityNuclear physicsCharginoatomic particle0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsPhysicsenergy transferarticle; atomic particle; energy; energy transfer; luminance; massluminance010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyDegenerate energy levelsarticleSupersymmetryNeutralinomassHigh Energy Physics::ExperimentParticle Physics - ExperimentenergyPhysics Letters B
researchProduct

Resolving the octant of theta(23) with T2K and NOvA

2013

Preliminary results of MINOS experiment indicate that theta(23) is not maximal. Global fits to world neutrino data suggest two nearly degenerate solutions for theta(23): one in the lower octant (LO: theta(23) 45 degrees). v(mu) -> v(e) oscillations in superbeam experiments are sensitive to the octant and are capable of resolving this degeneracy. We study the prospects of this resolution by the current T2K and upcoming NOvA experiments. Because of the hierarchy-delta(CP) degeneracy and the octant delta(CP) degeneracy, the impact of hierarchy on octant resolution has to be taken into account. As in the case of hierarchy determination, there exist favorable (unfavorable) values of delta(CP) fo…

Nuclear and High Energy PhysicsParticle physicsPhysics - Instrumentation and DetectorsFOS: Physical sciencesSilver ChannelOctant (solid geometry)01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)SymmetryHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNeutrino Oscillation ExperimentsNeutrino Physics010306 general physicsNeutrino oscillationPhysicsNOνAMixing Matrix010308 nuclear & particles physicsDegenerate energy levelsCp ViolationInstrumentation and Detectors (physics.ins-det)High Energy Physics - PhenomenologyCP violationMINOSBeyond Standard ModelLine-Experiment-SimulatorMass MatrixCP violationNeutrinoIndraStra Global
researchProduct

Probing neutralino properties in minimal supergravity with bilinear R-parity violation

2012

Supersymmetric models with bilinear R-parity violation (BRPV) can account for the observed neutrino masses and mixing parameters indicated by neutrino oscillation data. We consider minimal supergravity versions of BRPV where the lightest supersymmetric particle (LSP) is a neutralino. This is unstable, with a large enough decay length to be detected at the CERN Large Hadron Collider (LHC). We analyse the LHC potential to determine the LSP properties, such as mass, lifetime and branching ratios, and discuss their relation to neutrino properties.

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsBilinear interpolationFOS: Physical sciencesSupergravity01 natural sciences7. Clean energyLightest Supersymmetric ParticleSupergravitaciónHigh Energy Physics - Phenomenology (hep-ph)R-parity0103 physical sciencesNeutrinos010306 general physicsNeutrino oscillationPhysicsNeutrinesLarge Hadron Collider010308 nuclear & particles physicsSupergravityHigh Energy Physics::PhenomenologyFísicaHigh Energy Physics - PhenomenologyNeutralinoHigh Energy Physics::ExperimentNeutrino
researchProduct