Search results for "Electroweak"

showing 10 items of 744 documents

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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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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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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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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Chern-Simons anomaly as polarization effect

2011

The parity violating Chern-Simons term in the epoch before the electroweak phase transition can be interpreted as a polarization effect associated to massless right-handed electrons (positrons) in the presence of a large-scale seed hypermagnetic field. We reconfirm the viability of a unified seed field scenario relating the cosmological baryon asymmetry and the origin of the protogalactic large-scale magnetic fields observed in astronomy.

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectChern–Simons theoryFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAsymmetryBaryon asymmetryHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsmedia_commonPhysics010308 nuclear & particles physicsElectroweak interactionHigh Energy Physics::PhenomenologyFísicaAstronomy and AstrophysicsParity (physics)Massless particleBaryonHigh Energy Physics - PhenomenologyLeptogenesisHigh Energy Physics::ExperimentAstrophysics - Cosmology and Nongalactic Astrophysics
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First Observation of Vector Boson Pairs in a Hadronic Final State at the Tevatron Collider

2009

We present the first observation in hadronic collisions of the electroweak production of vector boson pairs (VV, V=W, Z) where one boson decays to a dijet final state. The data correspond to 3.5 fb(-1) of integrated luminosity of pp collisions at s=1.96 TeV collected by the CDF II detector at the Fermilab Tevatron. We observe 1516 +/- 239(stat)+/- 144(syst) diboson candidate events and measure a cross section sigma(pp -> VV+X) of 18.0 +/- 2.8(stat)+/- 2.4(syst)+/- 1.1(lumi) pb, in agreement with the expectations of the standard model.

Particle physicsFinal stateFermilab TevatronTevatronFOS: Physical sciencesGeneral Physics and AstronomyElementary particleddc:500.27. Clean energy01 natural sciences114 Physical sciencesStandard ModelVector bosonHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Tellurium compounds0103 physical sciences010306 general physicsNuclear ExperimentVECTOR BOSONBosonsBosonPhysicsGauge bosonIntegrated luminosityCross section010308 nuclear & particles physicshep-exPhysicsHadronic collisionsElectroweak interactionHigh Energy Physics::PhenomenologyTevatronVector bosonThe standard modelCDFProduction (computer science)High Energy Physics::ExperimentCollider
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How to discover QCD Instantons at the LHC

2020

Topological Effects in the Standard Model: Instantons, Sphalerons and Beyond at LHC, Geneva, Switzerland, 16 Dec 2020 - 18 Dec 2020; The European physical journal / C 81(7), 624 (2021). doi:10.1140/epjc/s10052-021-09412-1

Particle physicsInstantonp p: scatteringPhysics and Astronomy (miscellaneous)High Energy Physics::LatticeFOS: Physical sciencesquantum [tunneling]QC770-798AstrophysicsComputer Science::Digital Libraries01 natural sciences530Standard Modelvacuum statetopologicalHigh Energy Physics::TheoryCross section (physics)High Energy Physics - Phenomenology (hep-ph)Nuclear and particle physics. Atomic energy. Radioactivityasymmetry [baryon]0103 physical sciencesscattering [p p]ddc:530quantum chromodynamics: instantonLimit (mathematics)010306 general physicsEngineering (miscellaneous)Quantum tunnellingtunneling: quantumQuantum chromodynamicsPhysicsLarge Hadron Colliderelectroweak interaction010308 nuclear & particles physicsHigh Energy Physics::Phenomenologysymmetry breaking: chiralQB460-466High Energy Physics - PhenomenologyCERN LHC Collinstanton [quantum chromodynamics]confinementbaryon: asymmetryComputer Science::Mathematical Softwarechiral [symmetry breaking]Non-perturbativesignature
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Search for diphoton events with large missing transverse energy in 7 TeV proton-proton collisions with the ATLAS detector.

2011

A search for diphoton events with large missing transverse energy is presented. The data were collected with the ATLAS detector in proton-proton collisions at √s=7  TeV at the CERN Large Hadron Collider and correspond to an integrated luminosity of 3.1  pb−1. No excess of such events is observed above the standard model background prediction. In the context of a specific model with one universal extra dimension with compactification radius R and gravity-induced decays, values of 1/R<729  GeV are excluded at 95% C. L., providing the most sensitive limit on this model to date.

Particle physicsMISSING TRANSVERSE ENERGYCiências Naturais::Ciências FísicasAtlas detector:Ciências Físicas [Ciências Naturais]FIS/04 - Fisica Nucleare e SubnucleareGeneral Physics and AstronomyFOS: Physical sciencestransverse energy: missing-energy ; ATLAS ; universal extra dimension ; compactification ; CERN LHC Coll ; background ; p p: interaction ; final state: two-photon ; photon: Kaluza-Klein ; electroweak interaction: standard model: validity test ; experimental results ; 7000 GeV-cmsddc:500.201 natural sciences7. Clean energy530High Energy Physics - ExperimentNuclear physicsUniversal extra dimensionHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesddc:550[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]diphoton; events; transverse energy;proton-proton collisions; Hadron;ddc:530High Energy PhysicsSpecific model010306 general physicsNuclear ExperimentGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)QCPhysicsLarge Hadron ColliderScience & TechnologyCompactification (physics)010308 nuclear & particles physicsAtlas (topology)Settore FIS/01 - Fisica SperimentaleFísicaFIS/01 - Fisica SperimentaleATLASTransverse planeCol·lisions (Física nuclear)Experimental High Energy PhysicsUniversal Extra DimensionsFísica nuclearHigh Energy Physics::ExperimentLHCParticle Physics - ExperimentPhysical review letters
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Observational signatures of Higgs inflation

2016

We investigate the dependency of Higgs inflation on the non-renormalisable matching between the low energy Standard Model limit and the inflationary regime at high energies. We show that for the top mass range $m_t \gtrsim 171.8$ GeV the scenario robustly predicts the spectral index $n_s \simeq 0.97$ and the tensor-to-scalar ratio $r\simeq 0.003$. The matching is however non-trivial, even the best-fit values $m_h=125.09$ GeV and $m_t=173.21$ GeV require a jump $\delta \lambda \sim 0.01$ in the Higgs coupling below the inflationary scale. For $m_t\lesssim 171.8$ GeV, the matching may generate a feature in the inflationary potential. In this case the predicted values of $n_s$ and $r$ vary but…

Particle physicsMatching (statistics)Cosmology and Nongalactic Astrophysics (astro-ph.CO)STANDARD MODELFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics114 Physical sciences01 natural sciencesStandard ModelHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesphysics of the early universeinflationELECTROWEAK VACUUM010306 general physicscosmology of theories beyond the SMBosonInflation (cosmology)PhysicsSpectral index010308 nuclear & particles physicsINDUCED GRAVITY INFLATIONHigh Energy Physics::PhenomenologySpectral densityBOSONAstronomy and Astrophysics115 Astronomy Space scienceHigh Energy Physics - Phenomenologyparticle physics - cosmology connectionJumpHiggs bosonHigh Energy Physics::ExperimentAstrophysics - Cosmology and Nongalactic Astrophysics
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Short-range neutrinoless double beta decay mechanisms

2018

Neutrinoless double beta decay can significantly help to shed light on the issue of non-zero neutrino mass, as observation of this lepton number violating process would imply neutrinos are Majorana particles. However, the underlying interaction does not have to be as simple as the standard neutrino mass mechanism. The entire variety of neutrinoless double beta decay mechanisms can be approached effectively. In this work we focus on a theoretical description of short-range effective contributions to neutrinoless double beta decay, which are equivalent to 9-dimensional effective operators incorporating the appropriate field content. We give a detailed derivation of the nuclear matrix elements…

Particle physicsNuclear TheoryField (physics)Physics beyond the Standard Modeldouble beta decayFOS: Physical sciencesElectron01 natural sciencesneutrinoless double beta decayNuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph)Double beta decay0103 physical sciences010306 general physicsPhysicsta114electroweak interaction010308 nuclear & particles physicsneutrino interactionsHigh Energy Physics::PhenomenologyForm factor (quantum field theory)3. Good healthHigh Energy Physics - PhenomenologyMAJORANAelectroweak interactions in nuclear physicsPhase spaceHigh Energy Physics::ExperimentNeutrinoPhysical Review D
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