Search results for " Standard Model"

showing 10 items of 645 documents

Results of the NA31 Experiment on K0Decays

1989

Decays of neutral kaons are of high interest in high energy physics. The discovery of CP violation1 opened up a field of new physics. Today, interest is concentrated on precision measurements of CP-violating parameters as well as on searches for rare decays that are suppressed or forbidden in the standard model.

Nuclear physicsPhysicsHistory and Philosophy of ScienceHigh interestField (physics)General NeurosciencePhysics beyond the Standard ModelHigh Energy Physics::ExperimentAstrophysicsGeneral Biochemistry Genetics and Molecular BiologyStandard ModelAnnals of the New York Academy of Sciences
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Cosmological promising parameters of stau in the minimal supersymmetric standard model

2009

We find that we can account for the possible descrepancy of the primordial abundance of 7 Li between the observation and the prediction of the Big-Bang Nucleosynthesis in a scenario of the Big-Bang Nucleosynthesis with the Minimal Supersymmetric Standard Model. This scenario is consistent with a stau-neutralino coannihilation scenario to explain the relic abundance of dark matter. The solution to the discrepancy is given by taking the values of parameters; the mass of the neutralino as 300 GeV and the mass difference between the stau and the neutralino as (100 – 120) MeV.

Nuclear physicsPhysicsNuclear and High Energy PhysicsParticle physicsNucleosynthesisHigh Energy Physics::PhenomenologyNeutralinoDark matterHigh Energy Physics::ExperimentAstronomy and AstrophysicsAstrophysics::Galaxy AstrophysicsAtomic and Molecular Physics and OpticsMinimal Supersymmetric Standard Model
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Search for a light Higgs resonance in radiative decays of theϒ(1S)with a charm tag

2015

A search is presented for the decay Υ(1S)→ γA^0, A^0 → cc[bar], where A^0 is a candidate for the CP-odd Higgs boson of the next-to-minimal supersymmetric standard model. The search is based on data collected with the BABAR detector at the Υ(2S) resonance. A sample of Υ(1S) mesons is selected via the decay Υ(2S)→π + π − Υ(1S). The A^0 → cc[bar] decay is identified through the reconstruction of hadronic D^0, D^+, and D^∗ (2010)^+ meson decays. No significant signal is observed. The measured 90% confidence-level upper limits on the product branching fraction B(Υ(1S) → γA^0 ) × B(A^0 → cc[bar] ) range from 7.4×10^(−5) to 2.4×10^(−3) for A^0 masses from 4.00 to 8.95  GeV/c^2 and 9.10 to 9.25  Ge…

Nuclear physicsPhysicsNuclear and High Energy PhysicsParticle physicsPionMesonBranching fractionElectron–positron annihilationHadronHiggs bosonResonanceMinimal Supersymmetric Standard ModelPhysical Review D
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Constraints to new physics models for the proton charge radius puzzle from the decayK+→μ++ν+e−+e+

2014

A possible explanation for the discrepancy between electronic and muonic hydrogen measurements of the proton charge radius are new, lepton-universality violating interactions. Several new couplings and particles have been suggested that account for this discrepancy. At present, these explanations are poorly constrained. Experiments such as the upcoming kaon decay experiment at JPARC may constrain or eliminate some explanations by sensitivity to the decay channel $K^+ \rightarrow \mu^+ +\nu + e^- + e^+$. We calculate the predicted contributions of the various explanations to this channel. The predicted signals, if present, should be large enough to be resolved in the experiment.

Nuclear physicsPhysicsNuclear and High Energy PhysicsParticle physicsProtonCharge radiusPhysics beyond the Standard ModelHigh Energy Physics::ExperimentExotic atomPhysical Review D
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Inclusive B ¯ → X s ℓ + ℓ − $$ \overline{B}\to {X}_s{\ell}^{+}{\ell}^{-} $$ : complete angular analysis and a thorough study of collinear photons

2015

We investigate logarithmically enhanced electromagnetic corrections of all angular observables in inclusive $$ \overline{B}\to {X}_s{\ell}^{+}{\ell}^{-} $$ . We present analytical results, which are supplemented by a dedicated Monte Carlo study on the treatment of collinear photons in order to determine the size of the electromagnetic logarithms. We then give the Standard Model predictions of all observables, considering all available NNLO QCD, NLO QED and power corrections, and investigate their sensitivity to New Physics. Since the structure of the double differential decay rate is modified in the presence of QED corrections, we also propose new observables which vanish if only QCD correc…

Nuclear physicsPhysicsQuantum chromodynamicsParticle physicsNuclear and High Energy PhysicsPhotonPhysics beyond the Standard ModelMonte Carlo methodHigh Energy Physics::PhenomenologyOrder (ring theory)ObservableSensitivity (control systems)Standard Model
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VBFNLO: A parton level Monte Carlo for processes with electroweak bosons

2009

VBFNLO is a fully flexible parton level Monte Carlo program for the simulation of vector boson fusion, double and triple vector boson production in hadronic collisions at next-to-leading order in the strong Coupling constant. VBFNLO includes Higgs and vector boson decays with full spin correlations and all off-shell effects. In addition, VBFNLO implements CP-even and CP-odd Higgs boson via gluon fusion, associated with two jets, at the leading-order one-loop level with the full top- and bottom-quark mass dependence in a generic two-Higgs-doublet model. A variety of effects arising from beyond the Standard Model physics are implemented for selected processes. This includes anomalous coupling…

Particle physics530 PhysicsPhysics beyond the Standard ModelMonte Carlo methodGeneral Physics and AstronomyFOS: Physical sciencesPartonVector bosonHigh Energy Physics - Phenomenology (hep-ph)Electroweak bosonsloop QCD correctionsVBFNLOOne-loop QCD correctionsBosonPhysics1708 Hardware and ArchitectureHadronic collisionsElectroweak interactionHigh Energy Physics::Phenomenology3100 General Physics and AstronomyGluonHigh Energy Physics - PhenomenologyNLO Monte Carlo programHardware and Architecture10231 Institute for Computational ScienceHiggs bosonOneHigh Energy Physics::Experiment
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Observational constraints on decoupled hidden sectors

2016

We consider an extension of the Standard Model with a singlet sector consisting of a real (pseudo)scalar and a Dirac fermion coupled with the Standard Model only via the scalar portal. We assume that the portal coupling is weak enough for the singlet sector not to thermalize with the Standard Model allowing the production of singlet particles via the freeze-in mechanism. If the singlet sector interacts with itself sufficiently strongly, it may thermalize within itself, resulting in dark matter abundance determined by the freeze-out mechanism operating within the singlet sector. We investigate this scenario in detail. In particular, we show that requiring the absence of inflationary isocurva…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterScalar (mathematics)FOS: Physical sciencesParameter space114 Physical sciences01 natural sciencesStandard Modeldecouplingsymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)ABELL 38270103 physical sciencesSinglet state010306 general physicsdark matter abundanceInflation (cosmology)PhysicsINTERACTING DARK-MATTERta114010308 nuclear & particles physicsHigh Energy Physics::Phenomenologyextensions of the Standard ModelHidden sectorHigh Energy Physics - Phenomenologysinglet sectorCOSMOLOGICAL SIMULATIONSDirac fermionGALAXY CLUSTER 1E-0657-56symbols3.5 KEV LINEINTERACTION CROSS-SECTIONAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review D
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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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Toward (finally!) ruling out Z and Higgs mediated dark matter models

2016

In recent years, direct detection, indirect detection, and collider experiments have placed increasingly stringent constraints on particle dark matter, exploring much of the parameter space associated with the WIMP paradigm. In this paper, we focus on the subset of WIMP models in which the dark matter annihilates in the early universe through couplings to either the Standard Model $Z$ or the Standard Model Higgs boson. Considering fermionic, scalar, and vector dark matter candidates within a model-independent context, we find that the overwhelming majority of these dark matter candidates are already ruled out by existing experiments. In the case of $Z$ mediated dark matter, the only scenari…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics beyond the Standard Modelmedia_common.quotation_subjectDark matterScalar (mathematics)FOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energy01 natural sciencesStandard ModelHigh Energy Physics - Phenomenology (hep-ph)WIMP0103 physical sciences010306 general physicsmedia_commonPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsUniversePseudoscalarHigh Energy Physics - PhenomenologyHiggs bosonHigh Energy Physics::ExperimentAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Early Universe Higgs dynamics in the presence of the Higgs-inflaton and non-minimal Higgs-gravity couplings

2017

Apparent metastability of the electroweak vacuum poses a number of cosmological questions. These concern evolution of the Higgs field to the current vacuum, and its stability during and after inflation. Higgs-inflaton and non-minimal Higgs-gravity interactions can make a crucial impact on these considerations potentially solving the problems. In this work, we allow for these couplings to be present simultaneously and study their interplay. We find that different combinations of the Higgs-inflaton and non-minimal Higgs-gravity couplings induce effective Higgs mass during and after inflation. This crucially affects the Higgs stability considerations during preheating. In particular, a wide ra…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics beyond the Standard Modelmedia_common.quotation_subjectHigh Energy Physics::LatticeFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences114 Physical sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)Metastability0103 physical sciencesphysics of the early universeinflationparticle physicscosmology connectionELECTROWEAK VACUUM010306 general physicscosmology of theories beyond the SMmedia_commonInflation (cosmology)PhysicsSTABILITY010308 nuclear & particles physicsElectroweak interactionHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsBOSONInflaton115 Astronomy Space scienceUniverseHigh Energy Physics - PhenomenologyHiggs fieldHiggs bosonHigh Energy Physics::ExperimentAstrophysics - Cosmology and Nongalactic Astrophysics
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