Search results for " Theorie"

showing 10 items of 303 documents

Probes of the Standard Model effective field theory extended with a right-handed neutrino

2019

If neutrinos are Dirac particles and, as suggested by the so far null LHC results, any new physics lies at energies well above the electroweak scale, the Standard Model effective field theory has to be extended with operators involving the right-handed neutrinos. In this paper, we study this effective field theory and set constraints on the different dimension-six interactions. To that aim, we use LHC searches for associated production of light (and tau) leptons with missing energy, monojet searches, as well as pion and tau decays. Our bounds are generally above the TeV for order one couplings. One particular exception is given by operators involving top quarks. These provide new signals in…

Nuclear and High Energy PhysicsParticle physicsPhysics beyond the Standard ModelFOS: Physical sciencesComputer Science::Digital Libraries01 natural sciencesHigh Energy Physics - ExperimentStandard ModelHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesEffective field theoryNeutrino Physicslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsPhysicsLarge Hadron ColliderMissing energy010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyEffective Field TheoriesNeutrino physicsHigh Energy Physics - PhenomenologyBeyond Standard ModelComputer Science::Mathematical Softwarelcsh:QC770-798High Energy Physics::ExperimentNeutrinoElectroweak scaleLeptonJournal of High Energy Physics
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Quintessence, inflation and baryogenesis from a single pseudo-Nambu-Goldstone boson

2007

15 pages, 3 figures.-- ISI Article Identifier: 000250759700079.-- ArXiv pre-print available at: http://arxiv.org/abs/0707.3999

Nuclear and High Energy PhysicsParticle physicsProton decayCosmic microwave backgroundGenerationFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicssymbols.namesakePlanckBosonPhysicsHigh Energy Physics::PhenomenologyAstrophysics (astro-ph)BaryogenesisFísicaCosmology of Theories beyond the SMWater Cherenkov DetectorBaryogenesisGoldstone bosonLeptogenesissymbolsDark energyHigh Energy Physics::ExperimentQuintessence
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Consistent searches for SMEFT effects in non-resonant dijet events

2018

We investigate the bounds which can be placed on generic new-physics contributions to dijet production at the LHC using the framework of the Standard Model Effective Field Theory, deriving the first consistently-treated EFT bounds from non-resonant high-energy data. We recast an analysis searching for quark compositeness, equivalent to treating the SM with one higher-dimensional operator as a complete UV model. In order to reach consistent, model-independent EFT conclusions, it is necessary to truncate the EFT effects consistently at order $1/\Lambda^2$ and to include the possibility of multiple operators simultaneously contributing to the observables, neither of which has been done in prev…

Nuclear and High Energy PhysicsParticle physicsTevatronFOS: Physical sciencesParameter space01 natural sciencesHigh Energy Physics - ExperimentStandard ModelHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Perturbative QCD0103 physical sciencesEffective field theorylcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsLinear combinationPhysicsLarge Hadron Collider010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyEffective Field TheoriesTechnicolor and Composite ModelsObservableWeinberg angleHigh Energy Physics - PhenomenologyBeyond Standard Modellcsh:QC770-798Journal of High Energy Physics
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The HiggsTools handbook: a beginners guide to decoding the Higgs sector

2018

This report summarises some of the activities of the HiggsTools initial training network working group in the period 2015–2017. The main goal of this working group was to produce a document discussing various aspects of state-of-the-art Higgs physics at the large hadron collider (LHC) in a pedagogic manner. The first part of the report is devoted to a description of phenomenological searches for new physics (NP) at the LHC. All of the available studies of the couplings of the new resonance discovered in 2012 by the ATLAS and CMS experiments (Aad et al (ATLAS Collaboration) 2012 Phys. Lett. B 716 1–29; Chatrchyan et al (CMS Collaboration) 2012 Phys. Lett. B 716 30–61) conclude that it is com…

Nuclear and High Energy PhysicsParticle physicsTop quarkcoupling [Higgs particle]Higgs particle: decayHiggs bosonPhysics beyond the Standard Modelmomentum spectrum [transverse momentum]01 natural sciencesStandard ModelHiggs sectortransverse momentum: momentum spectrumeffective field theoryeffective field theories; Higgs boson; Higgs momentum distributions; LHC physics; new physics searchessearch for [new physics][ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciencesEffective field theory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]effective field theoriesddc:530effective field theorie010306 general physicsMonte CarloPhysicsLHC physicLarge Hadron ColliderHiggs particle: coupling010308 nuclear & particles physicsHiggs momentum distributionsnew physics: search forElectroweak interactionHigh Energy Physics::PhenomenologyLHC physicsnew physics searchedecay [Higgs particle]two-photon [final state]Higgs momentum distributionproduction [Higgs particle]CERN LHC CollHiggs particle: production[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Higgs bosonnew physics searches[ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::Experimentfinal state: two-photon
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Cosmology with a very light Lμ − Lτ gauge boson

2019

In this paper, we explore in detail the cosmological implications of an abelian L − L gauge extension of the Standard Model featuring a light and weakly coupled Z′. Such a scenario is motivated by the longstanding ∼ 4σ discrepancy between the measured and predicted values of the muon’s anomalous magnetic moment, (g − 2) , as well as the tension between late and early time determinations of the Hubble constant. If sufficiently light, the Z′ population will decay to neutrinos, increasing the overall energy density of radiation and altering the expansion history of the early universe. We identify two distinct regions of parameter space in this model in which the Hubble tension can be significa…

Nuclear and High Energy PhysicsParticle physicscosmological modelZ': couplingPopulationNeutrino decoupling01 natural sciences7. Clean energygauge boson: abeliansymbols.namesakeradiation: density0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivityenergy: densityNeutrino Physics010306 general physicseducationPhysicsGauge bosoneducation.field_of_studyMuonHubble constantAnomalous magnetic dipole momentspace-time: expansionmuon: magnetic moment010308 nuclear & particles physicsCoupling (probability)Cosmology of Theories beyond the SMHigh Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Beyond Standard Modelsymbolslcsh:QC770-798Neutrino[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]neutrino: decouplingAstrophysics - Cosmology and Nongalactic AstrophysicsHubble's lawJournal of High Energy Physics
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Dark photon dark matter in the presence of inhomogeneous structure

2020

Dark photon dark matter will resonantly convert into visible photons when the dark photon mass is equal to the plasma frequency of the ambient medium. In cosmological contexts, this transition leads to an extremely efficient, albeit short-lived, heating of the surrounding gas. Existing work in this field has been predominantly focused on understanding the implications of these resonant transitions in the limit that the plasma frequency of the Universe can be treated as being perfectly homogeneous, i.e. neglecting inhomogeneities in the electron number density. In this work we focus on the implications of heating from dark photon dark matter in the presence of inhomogeneous structure (which …

Nuclear and High Energy PhysicsPhotonCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsPlasma oscillation01 natural sciencesDark photon[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]High Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityThermal Field Theory010306 general physicsReionizationPhysicsRange (particle radiation)010308 nuclear & particles physicsStar formationFísicaCosmology of Theories beyond the SMHigh Energy Physics - PhenomenologyOrders of magnitude (time)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]lcsh:QC770-798Astrophysics - Cosmology and Nongalactic AstrophysicsJournal of High Energy Physics
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Editorial: The Future of Nuclear Structure: Challenges and Opportunities in the Microscopic Description of Nuclei

2021

The past two decades have witnessed tremendous progress in the microscopic description of atomic nuclei. The Topical Review `The Future of Nuclear Structure' aims at summarizing the current state-of-the-art microscopic calculations in Nuclear Theory and to give a useful reference for young researches who wish to learn more about this exciting discipline.

Nuclear reactionMaterials Science (miscellaneous)BiophysicsFOS: Physical sciencesGeneral Physics and AstronomyMicroscopic descriptionnuclear reactionNuclear Theory (nucl-th)Theoretical physicsnuclear theoryeffective field theorieseffective field theoriemany-body physicsPhysical and Theoretical ChemistryNuclear theorynuclear reactionsMathematical PhysicsPhysicsAb initio (calculations)Nuclear structurelcsh:QC1-999Topical reviewmany-body physicAtomic nucleusnuclear structurelcsh:Physics
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Spatial risks and complex systems: methodological perspectives

2007

Research on risk and industrial catastrophes question the complexity theories. Besides the concepts of complexity which lead us to reconsider concepts of risk, hazard and vulnerability, we propose to think about more practical aspects, for example the modelling of human behaviour in crisis situations. The link between concepts as critical self-organization, emergence, bifurcation, and the methods in the Distributed Artificial Intelligence (DAI) used to model them is however difficult. In this paper, we present ongoing analysis on the key concepts of risk science, such as hazards and catastrophes. We propose to enrich them with complex systems theories. First, we present methodological persp…

Operations researchComputer science[SHS.GEO] Humanities and Social Sciences/Geographymedia_common.quotation_subject0211 other engineering and technologies0507 social and economic geographyComplex systemVulnerabilitypanicContext (language use)02 engineering and technologyIndustrial Accident[ SHS.GEO ] Humanities and Social Sciences/Geographycomplex systemsresilienceComputingMilieux_MISCELLANEOUSmedia_commonriskcomplexity theoriesStructure (mathematical logic)human behaviour05 social sciencesSpatial risks021107 urban & regional planning[SHS.GEO]Humanities and Social Sciences/GeographyHazardRisk perceptionRisk analysis (engineering)Psychological resilience050703 geography
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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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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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