Search results for "SCALAR"

showing 10 items of 1002 documents

The scalar radius of the pion in two-flavor Wilson lattice QCD

2014

PhysicsParticle physicsPionScalar (mathematics)RadiusLattice QCDFlavorProceedings of 31st International Symposium on Lattice Field Theory LATTICE 2013 — PoS(LATTICE 2013)
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Calculation of the kaon B parameter using strictly local sum rules

1991

The kaon B-parameter is computed in the framework of strictly local QCD sum rules for a threepoint function involving pseudoscalar currents. As an application of these sum rules we derive a low energy formula for the B-parameter. We show that strictly local QCD sum rules yield more reliable results than other QCD sum rules, since they need less phenomenological information and do not suffer from stability problems. Our result for the B-parameter isB=0.74±0.17.

PhysicsParticle physicsQCD sum rulesPhysics and Astronomy (miscellaneous)High Energy Physics::LatticeHigh Energy Physics::PhenomenologyElementary particleFunction (mathematics)Stability (probability)PseudoscalarApplied mathematicsHigh Energy Physics::ExperimentField theory (psychology)Sum rule in quantum mechanicsQuantum field theoryEngineering (miscellaneous)Zeitschrift für Physik C Particles and Fields
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Constraints on inflation with an extended neutrino sector

2019

Constraints on inflationary models typically assume only the standard models of cosmology and particle physics. By extending the neutrino sector to include a new interaction with a light scalar mediator (mφ∼MeV), it is possible to relax these constraints, in particular via opening up regions of the parameter space of the spectral index ns. These new interactions can be probed at IceCube via interactions of astrophysical neutrinos with the cosmic neutrino background for nearly all of the relevant parameter space.

PhysicsParticle physicsSpectral index010308 nuclear & particles physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaScalar (mathematics)Parameter space01 natural sciencesCosmologyCosmic neutrino background0103 physical sciencesNeutrino010306 general physics
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Self-interacting dark matter and cosmology of a light scalar mediator

2016

We consider a fermionic dark matter candidate interacting via a scalar mediator coupled with the Standard Model through a Higgs portal. We consider a general setting including both scalar and pseudoscalar interactions between the scalar and fermion, and illustrate the relevant features for dark matter abundance, direct search limits and collider constraints. The case where dark matter has a self-interaction strength $⟨{\ensuremath{\sigma}}_{V}⟩/{m}_{\ensuremath{\psi}}\ensuremath{\sim}0.1--1\text{ }\text{ }{\mathrm{cm}}^{2}/\mathrm{g}$ is strongly constrained, in particular by the big bang nucleosynthesis. We show that these constraints can be alleviated by introducing a new light sterile ne…

PhysicsParticle physicsStandard Modelta114010308 nuclear & particles physicsHot dark matterPhysics beyond the Standard ModelScalar field dark matterscalar mediators01 natural sciencesdark matterStandard ModelPseudoscalarsterile neutrinosWeakly interacting massive particlesfermions0103 physical sciencesGravitino010306 general physicsLight dark matterPhysical Review D
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Dark Radiation and Inflationary Freedom after Planck 2015

2016

The simplest inflationary models predict a primordial power spectrum (PPS) of the curvature fluctuations that can be described by a power-law function that is nearly scale-invariant. It has been shown, however, that the low-multipole spectrum of the CMB anisotropies may hint the presence of some features in the shape of the scalar PPS, which could deviate from its canonical power-law form. We study the possible degeneracies of this non-standard PPS with the neutrino anisotropies, the neutrino masses, the effective number of relativistic species and a sterile neutrino or a thermal axion mass. The limits on these additional parameters are less constraining in a model with a non-standard PPS w…

PhysicsParticle physicsSterile neutrinoCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsScalar (mathematics)Cosmic microwave backgroundSpectral densityFOS: Physical sciences01 natural sciencessymbols.namesakeHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Dark radiation0103 physical sciencessymbolsPlanckNeutrino010306 general physicsAxionAstrophysics - Cosmology and Nongalactic Astrophysics
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Decaying warm dark matter and neutrino masses

2007

Neutrino masses may arise from spontaneous breaking of ungauged lepton number. Due to quantum gravity effects the associated Goldstone boson - the majoron - will pick up a mass. We determine the lifetime and mass required by cosmic microwave background observations so that the massive majoron provides the observed dark matter of the Universe. The majoron DDM scenario fits nicely in models where neutrino masses arise a la seesaw, and may lead to other possible cosmological implications.

PhysicsParticle physicsSterile neutrinoHot dark matterDark matterAstrophysics (astro-ph)High Energy Physics::PhenomenologyScalar field dark matterGeneral Physics and AstronomyFOS: Physical sciencesFísicaAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Mixed dark matterWarm dark matterNeutrinoLight dark matter
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CP phases in the charged current and Higgs sectors for Majorana neutrinos

1986

8 páginas, 2 figuras.-- CERN-TH-4247-85.

PhysicsParticle physicsSterile neutrinoPhysics and Astronomy (miscellaneous)Scalar (mathematics)High Energy Physics::PhenomenologyFísicaHiggs sectorMAJORANAHiggs bosonCP violationHigh Energy Physics::ExperimentNeutrinoEngineering (miscellaneous)Particle Physics - TheoryMajorana equation
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Search for the Scalar Top Quark inpp¯Collisions ats=1.8TeV

2002

We have performed a search for scalar top quark (stop) pair production in the inclusive electron-muon-missing transverse energy final state, using a sample of p (p) over bar events corresponding to 108.3 pb (-1) of data collected with the D0 detector at Fermilab. The search is done in the framework of the minimal supersymmetric standard model assuming that the sneutrino is the lightest supersymmetric particle. For the dominant decays of the lightest stop, (t) over tilde-->b (χ) over tilde (+)(1) and (t) over tilde-->bl (ν) over tilde , no evidence for signal is found. We derive cross-section limits as a function of stop ((t) over tilde), chargino ((χ) over tilde (+)(1)), and sneutrino ((ν) …

PhysicsParticle physicsTop quark010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyScalar (mathematics)General Physics and AstronomySupersymmetry01 natural sciencesLightest Supersymmetric ParticleNuclear physicsCharginoPair production0103 physical sciencesHigh Energy Physics::ExperimentFermilab010306 general physicsMinimal Supersymmetric Standard ModelPhysical Review Letters
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Updated scalar sector constraints in the Higgs triplet model

2016

We show that in the Higgs triplet model, after the Higgs discovery, the mixing angle in the CP-even sector can be strongly constrained from unitarity. We also discuss how large quantum effects in $h\to\gamma\gamma$ may arise in a SM-like scenario and a certain part of the parameter space can be ruled out from the diphoton signal strength. Using $T$-parameter and diphoton signal strength measurements, we update the bounds on the nonstandard scalar masses.

PhysicsParticle physicsUnitarity010308 nuclear & particles physicsScalar (mathematics)High Energy Physics::PhenomenologyFOS: Physical sciencesFísicaParameter space01 natural sciencesHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Signal strength0103 physical sciencesHiggs boson010306 general physicsMixing (physics)
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Charm-beauty meson bound states from B(B*)D(D*) and B(B*)D¯(D¯*) interaction

2017

We evaluate the $s$-wave interaction of pseudoscalar and vector mesons with both charm and beauty to investigate the possible existence of molecular $BD$, ${B}^{*}D$, $B{D}^{*}$, ${B}^{*}{D}^{*}$, $B\overline{D}$, ${B}^{*}\overline{D}$, $B{\overline{D}}^{*}$, or ${B}^{*}{\overline{D}}^{*}$ meson states. The scattering amplitude is obtained implementing unitarity starting from a tree level potential accounting for the dominant vector meson exchange. The diagrams are evaluated using suitable extensions to the heavy flavor sector of the hidden gauge symmetry Lagrangians involving vector and pseudoscalar mesons, respecting heavy quark spin symmetry. We obtain bound states at energies above 7 Ge…

PhysicsParticle physicsUnitarityMeson010308 nuclear & particles physicsHigh Energy Physics::LatticeNuclear TheoryHigh Energy Physics::Phenomenology01 natural sciencesPseudoscalar mesonTree (descriptive set theory)Isospin0103 physical sciencesBound stateHigh Energy Physics::ExperimentVector mesonExotic meson010306 general physicsPhysical Review D
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