Search results for " Standard Model"

showing 10 items of 645 documents

Consistent QFT description of non-standard neutrino interactions

2019

Neutrino oscillations are precision probes of new physics beyond the Standard Model. Apart from neutrino masses and mixings, they are also sensitive to possible deviations of low-energy interactions between quarks and leptons from the Standard Model predictions. In this paper we develop a systematic description of such non-standard interactions (NSI) in oscillation experiments within the quantum field theory framework. We calculate the event rate and oscillation probability in the presence of general NSI, starting from the effective field theory (EFT) in which new physics modifies the flavor or Lorentz structure of charged-current interactions between leptons and quarks. We also provide the…

High Energy Physics - TheoryQuarkNuclear and High Energy PhysicsParticle physicsPhysics beyond the Standard Modelfield theory01 natural sciencesStandard Modeleffective field theory0103 physical sciencesEffective field theorylcsh:Nuclear and particle physics. Atomic energy. RadioactivityNeutrino Physicsneutrino: massQuantum field theory010306 general physicsNeutrino oscillationnumerical calculationsneutrino: interactionPhysics010308 nuclear & particles physicsnew physicsHigh Energy Physics::Phenomenologyquantum mechanicsEffective Field Theories3. Good healthHigh Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]lcsh:QC770-798neutrino: oscillationNeutrinoneutrino: mixingLepton
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Measuring lepton flavor violation at LHC with a long-lived slepton in the coannihilation region

2008

When the mass difference between the lightest slepton, the NLSP, and the lightest neutralino, the LSP, is smaller than the tau mass, the lifetime of the lightest slepton increases in many orders of magnitude with respect to typical lifetimes of other supersymmetric particles. These small mass differences are possible in the MSSM and, for instance, they correspond to the coannihilation region of the CMSSM for $M_{1/2} \gsim 700$ GeV. In a general gravity-mediated MSSM, where the lightest supersymmetric particle is the neutralino, the lifetime of the lightest slepton is inversely proportional to the square of the intergenerational mixing in the slepton mass matrices. Such a long-lived slepton…

HistoryNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsHigh Energy Physics::LatticeFlavourFOS: Physical sciencesLightest Supersymmetric ParticleEducationStandard ModelNuclear physicsHigh Energy Physics - Phenomenology (hep-ph)Atlas (anatomy)medicinePhysicsLarge Hadron ColliderHigh Energy Physics::PhenomenologySuperpartnerSupersymmetryComputer Science ApplicationsHigh Energy Physics - Phenomenologymedicine.anatomical_structureNeutralinoHigh Energy Physics::ExperimentMinimal Supersymmetric Standard ModelLeptonPhysical Review D
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Indirect dark matter search with the ANTARES neutrino telescope

2012

Using the data recorded by the ANTARES neutrino telescope during 2007 and 2008, a search for high energy neutrinos coming from the direction of the Sun has been performed. The neutrino selection criteria have been chosen so as to maximize the rejection of the atmospheric background with respect to possible signals produced by the self-annihilation of weakly interactive massive particles accumulated in the centre of the Sun. After data unblinding, the number of neutrinos observed was found to be compatible with background expectations. The results obtained were compared to the fluxes predicted by the Constrained Minimal Supersymmetric Standard Model, and 90% upper limits for this model were …

HistoryParticle physicsHigh energyAstrophysics::High Energy Astrophysical PhenomenaScalar (mathematics)Neutrino telescopeDark matterCompact dimensionFOS: Physical sciencesScale (descriptive set theory)EducationStandard ModelHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Direct searchInstrumentation and Methods for Astrophysics (astro-ph.IM)PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)MuonHigh Energy Physics::PhenomenologyGauginoAstrophysics::Instrumentation and Methods for AstrophysicsComputer Science ApplicationsHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsMinimal Supersymmetric Standard Model
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Discrete Symmetries CP, T, CPT

2016

The role of Symmetry Breaking mechanisms to search for New Physics is of highest importance. We discuss the status and prospects of the Discrete Symmetries CP, T, CPT looking for their separate Violation in LHC experiments and meson factories.

HistoryParticle physicsMeson productionMesonCPT symmetryQC1-999Physics beyond the Standard ModelGeneral Physics and AstronomyFOS: Physical sciencesQuantum entanglement01 natural sciencesEducationHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesSymmetry breaking010306 general physicsPhysicsLarge Hadron Collider010308 nuclear & particles physicsCabibbo–Kobayashi–Maskawa matrixPhysicsOperator (physics)High Energy Physics::PhenomenologyTime evolutionComputer Science ApplicationsB-factoryBaryogenesisStandard Model (mathematical formulation)High Energy Physics - PhenomenologyHomogeneous spaceCP violationHigh Energy Physics::ExperimentEPJ Web of Conferences
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Inflation might be caused by the right

2009

15 pages, 4 figures.-- ISI article identifier: 000265600800102.-- ArXiv pre-print avaible at: http://arxiv.org/abs/0811.2998

Inflation (cosmology)PhysicsNuclear and High Energy PhysicsParticle physicsBeyond Standard ModelAstrophysics (astro-ph)FOS: Physical sciencesElementary particleFermionInflatonAstrophysicsMassless particleHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Neutrino PhysicsNeutrinoScalar fieldComputer Science::DatabasesLeptonCosmology of Theories beyond the SM
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Upper bound on the tensor-to-scalar ratio in GUT-scale supersymmetric hybrid inflation

2014

We explore the upper bound on the tensor-to-scalar ratio r in supersymmetric (F-term) hybrid inflation models with the gauge symmetry breaking scale set equal to the value 2.86⋅1016 GeV2.86⋅1016 GeV, as dictated by the unification of the MSSM gauge couplings. We employ a unique renormalizable superpotential and a quasi-canonical Kähler potential, and the scalar spectral index nsns is required to lie within the two-sigma interval from the central value found by the Planck satellite. In a sizable region of the parameter space the potential along the inflationary trajectory is a monotonically increasing function of the inflaton, and for this case, r≲2.9⋅10−4r≲2.9⋅10−4, while the spectral index…

Inflation (cosmology)PhysicsNuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)SuperpotentialScalar (mathematics)High Energy Physics::PhenomenologyFOS: Physical sciencesSupersymmetryInflatonUpper and lower boundsHigh Energy Physics - PhenomenologyGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)Astrophysics - Cosmology and Nongalactic AstrophysicsMinimal Supersymmetric Standard ModelGauge symmetryPhysics Letters B
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Searches for B0 decays to combinations of charmless isoscalar mesons

2004

We search for B meson decays into two-body combinations of eta, eta', omega, and phi mesons from 89 million B B-bar pairs collected with the BaBar detector at the PEP-II asymmetric-energy e+e- collider at SLAC. We find the branching fraction BF(B0 -> eta omega) = (4.0^{+1.3}_{-1.2} +- 0.4) x 10^-6 with a significance of 4.3 sigma. For all the other decay modes we set the following 90% confidence level upper limits on the branching fractions, in units of 10^-6 : BF(B0 -> eta eta)<2.8, BF(B0 -> eta eta')<4.6, BF(B0 -> eta' eta')<10, BF(B0 -> eta'omega)<2.8, BF(B0 -> eta phi)<1.0, BF(B0 -> eta' phi)<4.5, BF(B0 -> phi phi)<1.5.

IsoscalarElectron–positron annihilationBABARGeneral Physics and AstronomyQCD FACTORIZATION01 natural sciencesOmega13.25.Hw 11.30.Er 12.15.HhHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Mathematical modelProbability density function[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]PEP2B mesonNuclear ExperimentQCD FACTORIZATION; STANDARD MODEL; BABAR; SLACPhysicsQuantum chromodynamicsSigmaHamiltonianMonte Carlo methodSensitivity analysiPARTICLE PHYSICSBranching fractionSLACParticle physicsMesonSTANDARD MODELQCD FACTORIZATION STANDARD MODELFOS: Physical sciencesLikelihood distributionPARTICLE PHYSICS; PEP2; BABARSolenoidHigh energy physicNuclear physicsPhysics and Astronomy (all)ElectromagnetismElectromagnetic calorimeterPseudoscalar meson0103 physical sciencesPerturbation technique010306 general physicsCalorimeterError analysi010308 nuclear & particles physicsBranching fractionHEPMagnetic fieldHigh Energy Physics::Experiment
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μ-e conversion in nuclei versus μ→e γ: an effective field theory point of view

1998

Using an effective lagrangian description we analyze possible new physics contributions to the most relevant muon number violating processes: $\mu \to e \gamma$ and $\mu$--$e$ conversion in nuclei. We identify a general class of models in which those processes are generated at one loop level and in which $\mu$--$e$ conversion is enhanced with respect to $\mu \to e \gamma$ by a large $\ln(m^2_\mu/\Lambda^2),$ where $\Lambda$ is the scale responsible for the new physics. For this wide class of models bounds on $\mu$--$e$ conversion constrain the scale of new physics more stringently than $\mu \to e \gamma$ already at present and, with the expected improvements in $\mu$--$e$ conversion experim…

Loop (topology)PhysicsNuclear and High Energy PhysicsParticle physicsMuonViolació CP (Física nuclear)Physics beyond the Standard ModelScalar (mathematics)Effective field theoryScale (descriptive set theory)Order of magnitudePartícules (Física nuclear)Lepton
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Search for Magnetic Monopoles with the MoEDAL Forward Trapping Detector in 13 TeV Proton-Proton Collisions at the LHC

2017

MoEDAL is designed to identify new physics in the form of long-lived highly-ionising particles produced in high-energy LHC collisions. Its arrays of plastic nuclear-track detectors and aluminium trapping volumes provide two independent passive detection techniques. We present here the results of a first search for magnetic monopole production in 13 TeV proton-proton collisions using the trapping technique, extending a previous publication with 8 TeV data during LHC run-1. A total of 222 kg of MoEDAL trapping detector samples was exposed in the forward region and analysed by searching for induced persistent currents after passage through a superconducting magnetometer. Magnetic charges excee…

Magnetic monopolesProtonMagnetismPhysics beyond the Standard ModelGeneral Physics and Astronomy01 natural sciences7. Clean energyHigh Energy Physics - Experimentlaw.inventionCOLLIDERHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)STOPPING-POWERlawPhysics02 Physical SciencesLarge Hadron ColliderSTABLE MASSIVE PARTICLESPhysicsMagnetismDrell–Yan processhep-phPersistent currents3. Good healthHigh Energy Physics - PhenomenologyPhysical SciencesELECTROWEAK MONOPOLEParticle Physics - ExperimentGeneral PhysicsMagnetometerPhysics MultidisciplinaryMagnetic monopoleFOS: Physical sciencesNuclear track detector114 Physical sciencesNuclear physicsPhysics and Astronomy (all)Tellurium compoundsHigh energy physics Magnetism Magnetometers Highly ionizing particles Magnetic charges Magnetic monopoles Nuclear track detector Passive detection Persistent currents Proton proton collisions Trapping techniques Tellurium compounds0103 physical sciencesHigh energy physics010306 general physicsColliderIONIZING PARTICLESScience & TechnologyProton proton collisionshep-ex010308 nuclear & particles physicsMagnetometers Highly ionizing particlesMagnetic chargesTrapping techniquesPassive detectionSTATES
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Photon events with missing energy at root s=183 to 189 GeV

2000

The production of single photons has been studied in the reaction e+e- -> gamma + invisible particles at centre-of-mass energies of 183 GeV and 189 GeV. A previously published analysis of events with multi-photon final states accompanied by missing energy has been updated with 189 GeV data. The data were collected with the DELPHI detector and correspond to integrated luminosities of about 51 pb^{-1} and 158 pb^{-1} at the two energies. The number of light neutrino families is measured to be 2.84 +/- 0.15(stat) +/- 0.14(syst). The absence of an excess of events beyond that expected from Standard Model processes is used to set limits on new physics as described by supersymmetric and compos…

NEUTRALINOSParticle physicsDIMENSIONSPhotonPhysics and Astronomy (miscellaneous)Physics beyond the Standard ModelAstrophysics::High Energy Astrophysical PhenomenaSTANDARD MODELFOS: Physical sciencesScale (descriptive set theory)7. Clean energy01 natural sciencesPartícules (Física nuclear)Standard ModelHigh Energy Physics - ExperimentGravitationHigh Energy Physics - Experiment (hep-ex)E(+)E(-) COLLISIONSSIGNALSSEARCH0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsNuclear ExperimentEngineering (miscellaneous)DELPHIPhysicsMissing energy010308 nuclear & particles physicsSUPERLIGHT GRAVITINOLEPLARGE ELECTRON POSITRON COLLIDERSINGLE-PHOTONCOLLIDERSPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHIPARTICLE PHYSICSProduction (computer science)Física nuclearHigh Energy Physics::ExperimentNeutrinoE(+)E(-) COLLISIONS; SUPERLIGHT GRAVITINO; STANDARD MODEL; SINGLE-PHOTON; COLLIDERS; SEARCH; LEP; NEUTRALINOS; DIMENSIONS; SIGNALSParticle Physics - Experiment
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