Search results for "PARTICLE PHYSICS"

showing 10 items of 6826 documents

From hybrid to quadratic inflation with high-scale supersymmetry breaking

2014

Motivated by the reported discovery of inflationary gravity waves by the BICEP2 experiment, we propose an inflationary scenario in supergravity, based on the standard superpotential used in hybrid inflation. The new model yields a tensor-to-scalar ratio r ~ 0.14 and scalar spectral index ns ~ 0.964, corresponding to quadratic (chaotic) inflation. The important new ingredients are the high-scale, (1.6-10) x 10^13 GeV, soft supersymmetry breaking mass for the gauge singlet inflaton field and a shift symmetry imposed on the K\"ahler potential. The end of inflation is accompanied, as in the earlier hybrid inflation models, by the breaking of a gauge symmetry at (1.2-7.1) x 10^16 GeV, comparable…

Inflation (cosmology)PhysicsHigh Energy Physics - TheoryParticle physicsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)SupergravitySpontaneous symmetry breakingSuperpotentialHigh Energy Physics::PhenomenologyFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsInflatonSupersymmetry breakingSymmetry (physics)lcsh:QC1-999High Energy Physics - PhenomenologyHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)lcsh:PhysicsGauge symmetryAstrophysics - Cosmology and Nongalactic AstrophysicsPhysics Letters B
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Gravitino dark matter with neutralino NLSP in the constrained NMSSM

2010

The gravitino dark matter with neutralino NLSP hypothesis is investigated in the framework of NMSSM. We have considered both the thermal and non-thermal gravitino production mechanisms, and we have taken into account all the collider and cosmological constraints. The maximum allowed reheating temperature after inflation, as well as the maximum allowed gravitino mass are determined.

Inflation (cosmology)PhysicsHistoryParticle physicsDark matterHigh Energy Physics::PhenomenologyFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsComputer Science ApplicationsEducationlaw.inventionHigh Energy Physics - PhenomenologyGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)lawNeutralinoGravitinoHigh Energy Physics::ExperimentCollider
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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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2017

We show that the dynamics of the Higgs field during inflation is not affected by metric fluctuations if the Higgs is an energetically subdominant light spectator. For Standard Model parameters we find that couplings between Higgs and metric fluctuations are suppressed by $\mathcal{O}(10^{-7})$. They are negligible compared to both pure Higgs terms in the effective potential and the unavoidable non-minimal Higgs coupling to background scalar curvature. The question of the electroweak vacuum instability during high energy scale inflation can therefore be studied consistently using the Jordan frame action in a Friedmann--Lemaitre--Robertson--Walker metric, where the Higgs-curvature coupling en…

Inflation (cosmology)PhysicsParticle physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyElectroweak interactionScalar (mathematics)Astronomy and Astrophysics01 natural sciencesStandard ModelGeneral Relativity and Quantum CosmologyHiggs field0103 physical sciencesMetric (mathematics)Higgs bosonHigh Energy Physics::Experiment010306 general physicsScalar curvatureJournal of Cosmology and Astroparticle Physics
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Isocurvature Constraints on Portal Couplings

2016

We consider portal models which are ultraweakly coupled with the Standard Model, and confront them with observational constraints on dark matter abundance and isocurvature perturbations. We assume the hidden sector to contain a real singlet scalar $s$ and a sterile neutrino $\psi$ coupled to $s$ via a pseudoscalar Yukawa term. During inflation, a primordial condensate consisting of the singlet scalar $s$ is generated, and its contribution to the isocurvature perturbations is imprinted onto the dark matter abundance. We compute the total dark matter abundance including the contributions from condensate decay and nonthermal production from the Standard Model sector. We then use the Planck lim…

Inflation (cosmology)PhysicsSterile neutrinoParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsDark matterScalar (mathematics)High Energy Physics::PhenomenologyFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesStandard ModelPseudoscalarHidden sectorHigh Energy Physics - Phenomenologysymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencessymbolsPlanck010306 general physicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Precision luminosity measurements at LHCb

2014

Measuring cross-sections at the LHC requires the luminosity to be determined accurately at each centre-of-mass energy $\sqrt{s}$. In this paper results are reported from the luminosity calibrations carried out at the LHC interaction point 8 with the LHCb detector for $\sqrt{s}$ = 2.76, 7 and 8 TeV (proton-proton collisions) and for $\sqrt{s_{NN}}$ = 5 TeV (proton-lead collisions). Both the "van der Meer scan" and "beam-gas imaging" luminosity calibration methods were employed. It is observed that the beam density profile cannot always be described by a function that is factorizable in the two transverse coordinates. The introduction of a two-dimensional description of the beams improves sig…

Instrumentation for particle accelerators and storage rings - high energy (linear acceleratorsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)cluster finding[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear Experiment06.20.fbInstrumentationMathematical PhysicsQCPhysicsLuminosity (scattering theory)Large Hadron ColliderPattern recognition cluster finding calibration and fitting methodssynchrotrons)DetectorPattern recognition cluster finding calibration and fitting methodsComputer interfacecalibration and fitting methodsFísica nuclearTracking and position-sensitive detectorLHCParticle Physics - ExperimentParticle physics29.40.GxPattern recognition cluster finding calibration and fitting methods; Instrumentation for particle accelerators and storage rings - high energy (linear accelerators synchrotrons)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsLHCb - Abteilung HofmannPattern recognition cluster finding calibration and fitting methodInstrumentation for particle accelerators and storage rings - high energy (linear accelerators synchrotrons)NOConsistency (statistics)Pattern recognitionCalibrationSDG 7 - Affordable and Clean EnergyInstrumentation for particle accelerators and storage rings - high energy (linear accelerators synchrotrons)/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energyInteraction pointStandards and calibrationFunction (mathematics)29.50.+vLHCbInstrumentation for particle accelerators and storage rings - high energy (linear accelerators synchrotrons); Pattern recognition cluster finding calibration and fitting methods; Instrumentation; Mathematical PhysicsTEVPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentInstrumentation for particle accelerators and storage rings - high energy (linear accelerators synchrotrons); Pattern recognition cluster finding calibration and fitting methodsEnergy (signal processing)
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Update of the Binoth Les Houches Accord for a standard interface between Monte Carlo tools and one-loop programs

2014

We present an update of the Binoth Les Houches Accord (BLHA) to standardise the interface between Monte Carlo programs and codes providing one-loop matrix elements.

Interface (Java)Computer scienceCollider physics530 PhysicsMonte Carlo methodGeneral Physics and AstronomyFOS: Physical sciences10192 Physics Institute01 natural sciencesComputational scienceMatrix (mathematics)AutomationPhysics and Astronomy (all)High Energy Physics - Phenomenology (hep-ph)Collider physic0103 physical sciencesStatistical physics010306 general physicsCollider physicsParticle Physics - PhenomenologyMonte Carlo programNLO computationNLO computationsLOOP (programming language)010308 nuclear & particles physics1708 Hardware and ArchitectureMonte Carlo programsLes Houches Accord3100 General Physics and AstronomyHigh Energy Physics - PhenomenologyHardware and Architecture[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Computer Science::Programming Languagesddc:004
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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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Search for the Lepton Flavor Violation Process J/ψ→eμ at BESIII

2013

We search for the lepton-flavor-violating decay of the $J/\psi$ into an electron and a muon using $(225.3\pm2.8)\times 10^{6}$ $J/\psi$ events collected with the BESIII detector at the BEPCII collider. Four candidate events are found in the signal region, consistent with background expectations. An upper limit on the branching fraction of $\mathcal{B}(J/\psi \to e\mu)< 1.5 \times 10^{-7}$ (90% C.L.) is obtained.

J/psi(3100)Nuclear and High Energy PhysicsParticle physicsflavor: violation [lepton]Electron–positron annihilationElectronannihilation [electron positron]High Energy Physics - ExperimentNuclear physicsJ/psi(3100) --> muon electronR-parityddc:530FlavorE ConversionPhysicsMuonBESBranching fractionbackgroundNumberR-ParitySupersymmetryDecayBeijing StorNucleiConstraintsHigh Energy Physics::ExperimentSupersymmetrybranching ratioleptonic decay [J/psi(3100)]TauLimit3.1 GeV-cmsLeptonexperimental results
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