Search results for "Coupling"

showing 10 items of 1862 documents

Postinflationary vacuum instability and Higgs-inflaton couplings

2016

The Higgs-inflaton coupling plays an important role in the Higgs field dynamics in the early Universe. Even a tiny coupling generated at loop level can have a dramatic effect on the fate of the electroweak vacuum. Such Higgs-inflaton interaction is present both at the trilinear and quartic levels in realistic reheating models. In this work, we examine the Higgs dynamics during the preheating epoch, focusing on the effects of the parametric and tachyonic resonances. We use lattice simulations and other numerical tools in our studies. We find that the resonances can induce large fluctuations of the Higgs field which destabilize the electroweak vacuum. Our considerations thus provide an upper …

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)High Energy Physics::LatticePhysics beyond the Standard ModeleducationFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics114 Physical sciences01 natural sciencesUpper and lower boundsInstabilityGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)inflation Higgs0103 physical sciences010306 general physicsPhysicsCoupling010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyElectroweak interactionAstronomy and AstrophysicsInflatonHigh Energy Physics - PhenomenologyHiggs fieldHiggs bosonHigh Energy Physics::ExperimentAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Reheating the Standard Model from a hidden sector

2016

We consider a scenario where the inflaton decays to a hidden sector thermally decoupled from the visible Standard Model sector. A tiny portal coupling between the hidden and the visible sectors later heats the visible sector so that the Standard Model degrees of freedom come to dominate the energy density of the Universe before Big Bang Nucleosynthesis. We find that this scenario is viable, although obtaining the correct dark matter abundance and retaining successful Big Bang Nucleosynthesis is not obvious. We also show that the isocurvature perturbations constituted by a primordial Higgs condensate are not problematic for the viability of the scenario.

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Ultimate fate of the universereheatingmedia_common.quotation_subjectDark matterUNIVERSEFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics114 Physical sciences01 natural sciencesdark matterdecouplingpimeä aineHigh Energy Physics - Phenomenology (hep-ph)INFLATIONBig Bang nucleosynthesis0103 physical sciencesDARK-MATTERELECTROWEAK VACUUM010306 general physicsmedia_commonPhysicsQuintom scenariota114STABILITY010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyDecoupling (cosmology)InflatonHIGGSUniverseHidden sectorextensions of the Standard ModelHigh Energy Physics - Phenomenologyhidden sectorsSCALARAstrophysics - Cosmology and Nongalactic Astrophysics
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Third family of compact stars within a nonlocal chiral quark model equation of state

2019

A class of hybrid compact star equations of state is investigated that joins by a Maxwell construction a low-density phase of hadronic matter, modeled by a relativistic mean-field approach with excluded nucleon volume, with a high-density phase of color superconducting two-flavor quark matter, described within a nonlocal covariant chiral quark model. It is found that the occurrence of a stable branch of hybrid compact stars requires a nonvanishing vector meson coupling in the quark model that exceeds a minimal value which depends on the presence of a diquark condensate. It is shown that these hybrid stars do not form a third family disconnected from the second family of ordinary neutron sta…

Particle physicsEquation of stateNuclear TheoryCiencias FísicasNuclear TheoryFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsCompact starFísica de Partículas y Campos//purl.org/becyt/ford/1 [https]Nuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph)compact starsAstrophysics::Solar and Stellar AstrophysicsVector mesonquark modelsAstrophysics::Galaxy AstrophysicsPhysicsMaxwell construction//purl.org/becyt/ford/1.3 [https]Coupling (probability)Neutron starStarsStrange matterHigh Energy Physics - Phenomenologytwin starsAstrophysics::Earth and Planetary AstrophysicsCIENCIAS NATURALES Y EXACTAS
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Search for Supersymmetry with Gauge-Mediated Breaking in Diphoton Events with Missing Transverse Energy at CDF II

2010

8 páginas, 3 figuras.-- PACS numbers: 12.60.Jv, 13.85.Rm, 13.85.Qk, 14.80.Ly.-- CDF Collaboration: et al.

Particle physicsMODELSFOS: Physical sciencesGeneral Physics and Astronomyddc:500.2GAMMA PRODUCTIONKinetic energy114 Physical sciencesE(+)E(-) COLLISIONS; HADRON COLLIDERS; GAMMA PRODUCTION; QCD CORRECTIONS; PHOTON; COUPLINGS; PHYSICS; MODELS; TEV01 natural sciencesHigh Energy Physics - ExperimentStandard ModelPHYSICSNuclear physicsHigh Energy Physics - Experiment (hep-ex)E(+)E(-) COLLISIONS0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Grand Unified TheoryHADRON COLLIDERSSymmetry breakingQuantum field theory010306 general physicsPhysics010308 nuclear & particles physicsPhysicsHigh Energy Physics::PhenomenologySupersymmetryCOUPLINGSTransverse planePHOTONTEVHigh Energy Physics::ExperimentGravitinoQCD CORRECTIONS13.85.Rm 12.60.Jv 13.85.Qk 14.80.Ly
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Measurement of trilinear gauge couplings in e(+)e(-) collisions at 161 GeV and 172 GeV

1998

Trilinear gauge boson couplings are measured using data taken by DELPHI at 161 GeV and 172 GeV, Values for WWV couplings (V = Z,gamma) are determined from a study of the reactions e(+)e(-) --> W+W- and e(+)e(-) --> We nu, using differential distributions from the WW final state in which one W decays hadronically and the other leptonically, and total cross,section data from other channels, Limits are also derived on neutral ZV gamma couplings from an analysis of the reaction e(+)e(-) --> gamma + invisible particles. (C) 1998 Elsevier Science B.V.

Particle physicsNuclear and High Energy PhysicsElectron–positron annihilation7. Clean energy01 natural sciencesNuclear physics0103 physical sciencesOPTIMAL OBSERVABLES[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsNuclear ExperimentOPTIMAL OBSERVABLES; PHOTON COUPLINGS; ROOT-S=1.8 TEVDELPHIPhysicsGauge boson010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyROOT-S=1.8 TEVGauge (firearms)LARGE ELECTRON POSITRON COLLIDERPHOTON COUPLINGSLarge Electron–Positron ColliderPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHIPARTICLE PHYSICSHigh Energy Physics::ExperimentParticle Physics - Experiment
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A study of the Lorentz structure in tau decays

2000

This paper describes a measurement of the Michel parameters, \eta, \rho, \xi, \xi\delta, and the average \nu_{\tau} helicity, h_{\nu_{\tau}}, in tau lepton decays together with the first measurement of the tensor coupling in the weak charged current. The tau+tau- pairs were produced at the LEP e+e- collider at CERN from 1992 through 1995 in the DELPHI detector. Assuming lepton universality in the decays of the tau the measured values of the parameters were: \eta = -0.005 +/- 0.036 +/- 0.037, \rho = 0.775 +/- 0.023 +/- 0.020, \xi = 0.929 +/- 0.070 +/- 0.030, \xi\delta = 0.779 +/- 0.070 +/- 0.028, h_{\nu_{\tau}} = -0.997 +/- 0.027 +/- 0.011. The strength of the tensor coupling was measured to…

Particle physicsPhysics and Astronomy (miscellaneous)CHARGED WEAK-INTERACTIONSLUND MONTE-CARLOENERGIESLorentz transformationFOS: Physical sciences01 natural sciencesJET FRAGMENTATIONPartícules (Física nuclear)law.inventionHigh Energy Physics - Experimentsymbols.namesakeHigh Energy Physics - Experiment (hep-ex)NEUTRINO HELICITYLUND MONTE-CARLO; CHARGED WEAK-INTERACTIONS; RIGHT-SYMMETRICAL MODEL; MICHEL PARAMETERS; NEUTRINO HELICITY; RADIATIVE-CORRECTIONS; JET FRAGMENTATION; ENERGIES; LEPTON; PARTICLESlaw0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]RADIATIVE-CORRECTIONSPARTICLESTensor010306 general physicsColliderLEPTONEngineering (miscellaneous)Charged currentDELPHIPhysics010308 nuclear & particles physicsMICHEL PARAMETERSCoupling (probability)HelicityLARGE ELECTRON POSITRON COLLIDERRIGHT-SYMMETRICAL MODELPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHIsymbolsMichel parametersPARTICLE PHYSICSFísica nuclearHigh Energy Physics::ExperimentAstrophysics::Earth and Planetary AstrophysicsParticle Physics - ExperimentLeptonEuropean physical journal : C : particles and fields
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Search for Randall-Sundrum gravitons in dilepton and diphoton final states

2005

We report the first direct search for the Kaluza-Klein (KK) modes of Randall-Sundrum gravitons using dielectron, dimuon, and diphoton events observed with the D0 detector operating at the Fermilab Tevatron ppbar Collider at sqrt(s) = 1.96 TeV. No evidence for resonant production of gravitons has been found in the data corresponding to an integrated luminosity of approximately 260 pb^-1. Lower limits on the mass of the first KK mode at the 95% C.L. have been set between 250 and 785 GeV, depending on its coupling to SM particles.

Particle physicsPhysics::General PhysicsTevatronGeneral Physics and AstronomyFOS: Physical sciences13.85.Rm 04.50.+h 12.60.-i7. Clean energy01 natural sciencesStandard Modellaw.inventionHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)law0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Fermilab010306 general physicsColliderNuclear ExperimentPhysicsCouplingLuminosity (scattering theory)010308 nuclear & particles physicsGravitonHigh Energy Physics - PhenomenologyRandall–Sundrum modelHigh Energy Physics::Experiment
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Dark matter-neutrino interactions through the lens of their cosmological implications

2018

Dark matter and neutrinos provide the two most compelling pieces of evidence for new physics beyond the Standard Model of Particle Physics but they are often treated as two different sectors. The aim of this paper is to determine whether there are viable particle physics frameworks in which dark matter can be coupled to active neutrinos. We use a simplified model approach to determine all possible renormalizable scenarios where there is such a coupling, and study their astrophysical and cosmological signatures. We find that dark matter-neutrino interactions have an impact on structure formation and lead to indirect detection signatures when the coupling between dark matter and neutrinos is …

Particle physicsStructure formationdark matter: interactionPhysics beyond the Standard ModelDark matterFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsParameter space01 natural sciencesdark matterdark matter: couplingHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesneutrino: coupling010306 general physicsneutrino: interactionPhysics010308 nuclear & particles physicsnew physicsdark matter: massdark matter: mediationHigh Energy Physics - PhenomenologyCoupling (physics)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Particle[ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]NeutrinoDark fluiddark matter: parameter space
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Effects of triplet Higgs bosons in long baseline neutrino experiments

2018

The triplet scalars $(\Delta=\Delta^{++},\Delta^{+},\Delta^{0})$, utilized in the so-called Type-II seesaw model to explain the lightness of neutrinos, would generate nonstandard interactions (NSI) for neutrino propagating in matter. We investigate the prospects to probe these interactions in long baseline neutrino oscillation experiments. We analyze the upper bounds that the proposed DUNE experiment might set on the nonstandard parameters and numerically derive upper bounds, as function of the lightest neutrino mass, on the ratio the mass $M_\Delta$ of the triplet scalars and strength $|\lambda_\phi|$ of the coupling $\phi\phi\Delta$ of the triplet $\Delta$ and conventional Higgs doublet $…

Particle physicsVIOLATIONPontecorvo–Maki–Nakagawa–Sakata matrixFOS: Physical scienceshiukkasfysiikkaComputer Science::Digital Libraries114 Physical sciences7. Clean energy01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)effective field theory0103 physical sciences010306 general physicsNeutrino oscillationBosonPhysicsLEFT-RIGHT SYMMETRYneutrino oscillationsPARITYta114010308 nuclear & particles physicsHiggsin bosoniHigh Energy Physics::PhenomenologyneutriinotParity (physics)Coupling (probability)extensions of Higgs sectorHigh Energy Physics - PhenomenologyHiggsin bosonitHiggs bosonDOUBLY-CHARGED HIGGSHigh Energy Physics::ExperimentNeutrinoLepton
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Hadronic τ Decays as New Physics Probes in the LHC Era

2019

We analyze the sensitivity of hadronic tau decays to non-standard interactions within the model-independent framework of the Standard Model Effective Field Theory (SMEFT). Both exclusive and inclusive decays are studied, using the latest lattice data and QCD dispersion relations. We show that there are enough theoretically clean channels to disentangle all the effective couplings contributing to these decays, with the $\tau \to \pi\pi\nu_\tau$ channel representing an unexpected powerful New Physics probe. We find that the ratios of non-standard couplings to the Fermi constant are bound at the sub-percent level. These bounds are complementary to the ones from electroweak precision observable…

Particle physicsdata analysis methoddispersion relationPhysics beyond the Standard ModelLattice field theoryGeneral Physics and AstronomyFOS: Physical sciences01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)effective field theoryweak interaction: coupling constant0103 physical sciencesquantum chromodynamicsEffective field theory010306 general physicstau: hadronic decayParticle Physics - PhenomenologyQuantum chromodynamicsPhysicsLarge Hadron Colliderelectroweak interactionnew physicsElectroweak interactionHigh Energy Physics::Phenomenologylattice field theoryhep-phObservablecorrection: vertexsensitivitytau --> pi pi neutrino/tauHigh Energy Physics - PhenomenologyCERN LHC Coll[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Elementary Particles and Fieldslepton: universality: violationHigh Energy Physics::ExperimentLepton
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