Search results for "Standard Model"

showing 10 items of 1206 documents

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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Precision calculations of dark matter relic abundance

2019

The dark matter annihilation channels sometimes involve sharp resonances. In such cases the usual momentum averaged approximations for computing the DM abundance may not be accurate. We develop an easily accessible momentum dependent framework for computing the DM abundance accurately and efficiently near such features. We apply the method to the case of a singlet scalar dark matter $s$ interacting with SM through higgs portal $\lambda_{\rm hs}s^2 h^2$ and compare the results with different momentum averaged methods. The accuracy of the latter depend strongly on the strength of the elastic interactions and corrections are large if WIMP has negligible interactions beyond the main annihilatio…

Particle physicsAstrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)Scalar (mathematics)Dark matterFOS: Physical sciencesKinetic energykosmologia01 natural sciencesStandard ModelMomentumpimeä aineHigh Energy Physics - Phenomenology (hep-ph)WIMP0103 physical sciencesphysics of the early universeCOSMIC ABUNDANCES010306 general physicsParticle Physics - PhenomenologyPhysicsdark matter theoryAnnihilation010308 nuclear & particles physicsdark matter experimentsAstronomy and Astrophysicshep-ph115 Astronomy Space scienceHigh Energy Physics - PhenomenologyHiggs bosonastro-ph.COAstrophysics - Cosmology and Nongalactic Astrophysics
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Combination of Tevatron searches for the standard model Higgs boson in the W+W- decay mode.

2010

11 páginas, 4 figuras, 1 tabla.-- CDF Collaboration: et al.

Particle physicsAstrophysics::High Energy Astrophysical PhenomenaTevatronFOS: Physical sciencesGeneral Physics and AstronomyElementary particleddc:500.2.PARTON DISTRIBUTIONS; HADRON COLLIDERS; QCD; NNLO7. Clean energy01 natural sciences114 Physical sciencesHigh Energy Physics - ExperimentStandard ModelNuclear physicsHigh Energy Physics - Experiment (hep-ex)Particle decay0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Grand Unified TheoryHADRON COLLIDERSFermilabTEVATRONNuclear Experiment010306 general physicsBosonPhysicsHIGGS BOSON010308 nuclear & particles physicsPhysicsHigh Energy Physics::PhenomenologyQCD3. Good healthPARTON DISTRIBUTIONSHiggs bosonCDFPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNNLOAnti-p p: interaction | Higgs particle: search for | gluon gluon: fusion | intermediate boson: fusion | quark antiquark: annihilation | Higgs particle: decay | Higgs particle --> W+ W- | W: pair production | W: leptonic decay | dilepton: final state | jet: multiplicity | cross section: upper limit | mass dependence | Higgs particle: mass | background | DZERO | CDF | Batavia TEVATRON Coll | anti-p p --> Higgs particle anything | anti-p p --> Higgs particle anything intermediate boson anything | anti-p p --> Higgs particle anything quark antiquark anything | 1960 GeV-cmsPhysical review letters
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Dark photon search in the mass range between 1.5 and 3.4 GeV/c2

2017

Physics letters / B 774, 252 - 257 (2017). doi:10.1016/j.physletb.2017.09.067

Particle physicsBESIII; Dark photon search; Initial state radiation; Nuclear and High Energy PhysicsNuclear and High Energy PhysicsPhotonBESIII детекторElectron–positron annihilationFOS: Physical sciences01 natural sciences530Dark photonVector bosonStandard ModelHigh Energy Physics - ExperimentNONuclear physicsHigh Energy Physics - Experiment (hep-ex)Dark photon search0103 physical sciencesInvariant massddc:530Dark photon search; Initial state radiation; BESIII010306 general physicsNuclear ExperimentPhysicsGauge boson010308 nuclear & particles physicsтемные фотоныBESIIIlcsh:QC1-999BEPCII коллайдерMass spectrumHigh Energy Physics::ExperimentInitial state radiationlcsh:PhysicsPhysics Letters B
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A model for dark matter, naturalness and a complete gauge unification

2015

We consider dark matter in a minimal extension of the Standard Model (SM) which breaks electroweak symmetry dynamically and leads to a complete unification of the SM and technicolor coupling constants. The unification scale is determined to be $M_{\rm U} \approx 2.2 \times 10^{15}$ GeV and the unified coupling $\alpha_{\rm U} \approx 0.0304$. Moreover, unification strongly suggest that the technicolor sector of the model must become strong at the scale of ${\cal O}$(TeV). The model also contains a tightly constrained sector of mixing neutral fields stabilized by a discrete symmetry. We find the lightest of these states can be DM with a mass in the range $m_{\rm DM} \approx 30-800$ GeV. We f…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterFOS: Physical sciencesTechnicolorParameter space01 natural sciences7. Clean energyStandard ModelHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsCoupling constantPhysicsdark matter theory010308 nuclear & particles physicsdark matter experimentsElectroweak interactionHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsCoupling (probability)High Energy Physics - Phenomenologyparticle physics - cosmology connectionHigh Energy Physics::ExperimentDiscrete symmetryAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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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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Higgs-like spectator field as the origin of structure

2021

We show that the observed primordial perturbations can be entirely sourced by a light spectator scalar field with a quartic potential, akin to the Higgs boson, provided that the field is sufficiently displaced from vacuum during inflation. The framework relies on the indirect modulation of reheating, which is implemented without any direct coupling between the spectator field and the inflaton and does not require non-renormalisable interactions. The scenario gives rise to local non-Gaussianity with $f_{\rm NL}\simeq 5$ as the typical signal. As an example model where the indirect modulation mechanism is realised for the Higgs boson, we study the Standard Model extended with right-handed neu…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)Field (physics)FOS: Physical sciencesQC770-798Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicskosmologia01 natural sciences7. Clean energy114 Physical sciencesPhysics Particles & FieldsStandard ModelHigh Energy Physics - Phenomenology (hep-ph)Nuclear and particle physics. Atomic energy. RadioactivityQuartic function0103 physical sciences0206 Quantum Physics010303 astronomy & astrophysicsEngineering (miscellaneous)kosminen inflaatioInflation (cosmology)PhysicsScience & Technology010308 nuclear & particles physicsPhysicsHiggsin bosoniHigh Energy Physics::Phenomenologyhiukkasfysiikan standardimallihep-phInflatonPERTURBATIONSNuclear & Particles PhysicsQB460-466High Energy Physics - Phenomenologykosminen taustasäteilyPhysical Sciences0202 Atomic Molecular Nuclear Particle and Plasma Physicsastro-ph.COHiggs bosonNeutrinoScalar fieldAstrophysics - Cosmology and Nongalactic AstrophysicsThe European Physical Journal C
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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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