Search results for "standard model"

showing 10 items of 1206 documents

Searching for Earth/Solar axion halos

2020

We discuss the sensitivity of the present and near-future axion dark matter experiments to a halo of axions or axion-like particles gravitationally bound to the Earth or the Sun. The existence of such halos, assuming they are formed, renders a significant gain in the sensitivity of axion searches while satisfying all the present experimental bounds. The structure and coherence properties of these halos also imply novel signals, which can depend on the latitude or orientation of the detector. We demonstrate this by analysing the sensitivity of several distinct types of axion dark matter experiments.

Nuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Atomic Physics (physics.atom-ph)Physics::Instrumentation and DetectorsDark matterFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesPhysics - Atomic PhysicsHigh Energy Physics::TheoryHigh Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsAxionAstrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyCosmology of Theories beyond the SMHigh Energy Physics - PhenomenologyCP violationBeyond Standard Modellcsh:QC770-798CP violationHaloEarth (classical element)Astrophysics - Cosmology and Nongalactic AstrophysicsCoherence (physics)Journal of High Energy Physics
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Production of dark-matter bound states in the early universe by three-body recombination

2018

The small-scale structure problems of the universe can be solved by self-interacting dark matter that becomes strongly interacting at low energy. A particularly predictive model for the self-interactions is resonant short-range interactions with an S-wave scattering length that is much larger than the range. The velocity dependence of the cross section in such a model provides an excellent fit to self-interaction cross sections inferred from dark-matter halos of galaxies and clusters of galaxies if the dark-matter mass is about 19 GeV and the scattering length is about 17 fm. Such a model makes definite predictions for the few-body physics of weakly bound clusters of the dark-matter particl…

Nuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Nuclear Theorymedia_common.quotation_subjectPhysics beyond the Standard ModelDark matterFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesHigh Energy Physics - ExperimentNuclear Theory (nucl-th)High Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesBound stateEffective field theoryCluster (physics)lcsh:Nuclear and particle physics. Atomic energy. RadioactivityNuclear Experiment (nucl-ex)010306 general physicsNuclear Experimentmedia_commonPhysics010308 nuclear & particles physicsScattering lengthCosmology of Theories beyond the SMUniverseGalaxyHigh Energy Physics - PhenomenologyBeyond Standard Modellcsh:QC770-798Astrophysics - Cosmology and Nongalactic Astrophysics
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A systematic study of hidden sector dark matter: application to the gamma-ray and antiproton excesses

2020

In hidden sector models, dark matter does not directly couple to the particle content of the Standard Model, strongly suppressing rates at direct detection experiments, while still allowing for large signals from annihilation. In this paper, we conduct an extensive study of hidden sector dark matter, covering a wide range of dark matter spins, mediator spins, interaction diagrams, and annihilation final states, in each case determining whether the annihilations are s-wave (thus enabling efficient annihilation in the universe today). We then go on to consider a variety of portal interactions that allow the hidden sector annihilation products to decay into the Standard Model. We broadly class…

Nuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectDark matterFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesHigh Energy Physics - ExperimentStandard ModelHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsmedia_commonPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Annihilation010308 nuclear & particles physicsCosmology of Theories beyond the SMGalaxyUniverseDwarf spheroidal galaxyHidden sectorHigh Energy Physics - PhenomenologyAntiprotonBeyond Standard Modellcsh:QC770-798Astrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic Astrophysics
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Searching for hidden sectors in multiparticle production at the LHC

2016

Most signatures of new physics in colliders have been studied so far on the transverse plane with respect to the beam direction. In this work however we study the impact of a hidden sector beyond the Standard Model (SM) on inclusive (pseudo)rapidity correlations and moments of the multiplicity distributions, with special emphasis in the LHC results.

Nuclear and High Energy PhysicsFactorialParticle physicsPhysics beyond the Standard ModelMultihadron correlationsFOS: Physical sciencesFactorial and cumulant moments01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)pp interactions at LHC0103 physical sciencesProduction (economics)RapidityStatistical physics010306 general physicsCumulantParticle Physics - PhenomenologyPhysicsLarge Hadron Collider010308 nuclear & particles physicsFísicaMultiplicity (mathematics)Hidden Valley modelslcsh:QC1-999Hidden sectorHigh Energy Physics - PhenomenologyTransverse planeMoment (physics)Beam directionPhysics::Accelerator PhysicsModels beyond the Standard Modellcsh:PhysicsNuclear and Particle Physics Proceedings
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Combining data from high-energy p p -reactions and neutrinoless double-beta decay: Limits on the mass of the right-handed boson

2016

From the recently established lower-limits on the nonobservability of the neutrinoless double-beta decay of 76Ge (GERDA collaboration) and 136Xe (EXO-200 and KamLAND-Zen collaborations), combined with the ATLAS and CMS data, we extract limits for the left-right (LR) mixing angle, of the SU(2)L ×SU(2)R electroweak Hamiltonian. For the theoretical analysis, which is a model dependent, we have adopted a minimal extension of the Standard Model (SM) of Electroweak Interactions belonging to the SU(2)L ×SU(2)R representation. The nuclear-structure input of the analysis consists of a set of matrix elements and phase-space factors, and the experimental lower-limits for the half-lives. The other inpu…

Nuclear and High Energy PhysicsHigh energyParticle physicsCiencias AstronómicasPhysics::Instrumentation and DetectorsPhysics beyond the Standard ModelCiencias FísicasGeneral Physics and Astronomy01 natural sciencesRIGHT-HANDED CURRENTS//purl.org/becyt/ford/1 [https]Nuclear physicssymbols.namesakeNEUTRINOLESS DOUBLE-BETA-DECAYDouble beta decay0103 physical sciences010306 general physicsMASS OF THE RIGHT-HANDED BOSONSBosonPhysicsLarge Hadron Colliderta114010308 nuclear & particles physicsAtlas (topology)Electroweak interactionMass of the right-handed bosonsRight-handed currents//purl.org/becyt/ford/1.3 [https]Minimal extension of the standard modelAstronomíasymbolsNeutrinoless double-beta-decayMINIMAL EXTENSION OF THE STANDARD MODELHigh Energy Physics::ExperimentHamiltonian (quantum mechanics)CIENCIAS NATURALES Y EXACTAS
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Light Composite Higgs from Higher Representations versus Electroweak Precision Measurements -- Predictions for LHC

2005

We investigate theories in which the technifermions in higher dimensional representations of the technicolor gauge group dynamically break the electroweak symmetry of the standard model. For the two-index symmetric representation of the gauge group the lowest number of techniflavors needed to render the underlying gauge theory quasi conformal is two. We confront the models with the recent electroweak precision measurements and demonstrate that the two technicolor theory is a valid candidate for a dynamical breaking of the electroweak symmetry. The electroweak precision measurements provide useful constraints on the relative mass splitting of the new leptons needed to cure the Witten anomaly…

Nuclear and High Energy PhysicsHyperchargeParticle physicsSterile neutrinoHigh Energy Physics::LatticeFOS: Physical sciencesTechnicolorAstrophysics01 natural sciencesStandard ModelHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - LatticeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsPhysicsGauge boson010308 nuclear & particles physicsElectroweak interactionHigh Energy Physics::PhenomenologyAstrophysics (astro-ph)High Energy Physics - Lattice (hep-lat)SupersymmetryHigh Energy Physics - PhenomenologyHiggs bosonHigh Energy Physics::Experiment
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Study of the four-jet anomaly observed at LEP centre-of-mass energies of 130 and 136 GeV

1999

The four-jet events collected by DELPHI during the special LEP run at centre-of-mass energies of 130 and 136 GeV in 1997 with an integrated luminosity of 5.9 pb(-1) are analysed. Their rate and the distributions of their di-jet masses, their smallest jet charges, and their di-jet charge separations all agree well with Standard Model predictions. Thus the hypothesis of pair production of a new particle with a sum of di-jet masses around 105 GeV/c(2) is not supported. The combined result of the four LEP collaborations refuting this hypothesis at over 99% confidence level is also given. (C) 1999 Published by Elsevier Science B.V. All rights reserved.

Nuclear and High Energy PhysicsParticle physics4-JET EVENTS; DETECTOR; SEARCHAstrophysics::High Energy Astrophysical PhenomenaJet (particle physics)01 natural sciencesStandard ModelNuclear physicsSEARCH0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Combined result010306 general physicsDETECTORDELPHIPhysicsLuminosity (scattering theory)010308 nuclear & particles physicsCharge (physics)LARGE ELECTRON POSITRON COLLIDER4-JET EVENTSPair productionPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHILarge Electron–Positron ColliderPARTICLE PHYSICSHigh Energy Physics::ExperimentAnomaly (physics)Particle Physics - Experiment
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Effective field theory after a new-physics discovery

2018

When a new heavy particle is discovered at the LHC or at a future high-energy collider, it will be interesting to study its decays into Standard Model particles using an effective field-theory framework. We point out that the proper effective theory can not be constructed as an expansion in local, higher-dimensional operators; rather, it must be based on non-local operators defined in soft-collinear effective theory (SCET). For the interesting case where the new resonance is a gauge-singlet spin-0 boson, which is the first member of a new sector governed by a mass scale $M$, we show how a consistent scale separation between $M$ and the electroweak scale $v$ is achieved up to next-to-next-to…

Nuclear and High Energy PhysicsParticle physics530 PhysicsPhysics beyond the Standard ModelFOS: Physical sciences10192 Physics Institute01 natural sciencesResonance (particle physics)Standard ModelHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesEffective field theoryRenormalization Grouplcsh:Nuclear and particle physics. Atomic energy. Radioactivity3106 Nuclear and High Energy Physics010306 general physicsBosonPhysics010308 nuclear & particles physicsComputer Science::Information RetrievalHigh Energy Physics::PhenomenologyEffective Field TheoriesRenormalization groupHigh Energy Physics - PhenomenologySoft-collinear effective theoryBeyond Standard Modellcsh:QC770-798ResummationElectroweak scaleJournal of High Energy Physics
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Solar Neutrino Observables Sensitive to Matter Effects

2010

We discuss constraints on the coefficient A_{MSW} which is introduced to simulate the effect of weaker or stronger matter potential for electron neutrinos with the current and future solar neutrino data. The currently available solar neutrino data leads to a bound A_{MSW} = 1.47^{-0.42}_{+0.54} (^{-0.82}_{+1.88}) at 1\sigma (3\sigma) CL, which is consistent with the Standard Model prediction A_{MSW} = 1. For weaker matter potential (A_{MSW} 1), the bound is milder and is dominated by the day-night asymmetry of ^8B neutrino flux recently observed by Super-Kamiokande. Among the list of observable of ongoing and future solar neutrino experiments, we find that (1) an improved precision of the d…

Nuclear and High Energy PhysicsParticle physicsArticle SubjectSolar neutrinomedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences7. Clean energy01 natural sciencesAsymmetryStandard ModelHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationBorexinomedia_commonPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaSolar neutrino problemlcsh:QC1-999High Energy Physics - Phenomenology13. Climate actionMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinolcsh:PhysicsAdvances in High Energy Physics
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Searches for atmospheric long-lived particles

2020

Long-lived particles are predicted in extensions of the Standard Model that involve relatively light but very weakly interacting sectors. In this paper we consider the possibility that some of these particles are produced in atmospheric cosmic ray showers, and their decay intercepted by neutrino detectors such as IceCube or Super-Kamiokande. We present the methodology and evaluate the sensitivity of these searches in various scenarios, including extensions with heavy neutral leptons in models of massive neutrinos, models with an extra $U(1)$ gauge symmetry, and a combination of both in a $U(1)_{B-L}$ model. Our results are shown as a function of the production rate and the lifetime of the c…

Nuclear and High Energy PhysicsParticle physicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic ray01 natural sciences7. Clean energyHigh Energy Physics - ExperimentStandard ModelHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNeutrino Physicslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsGauge symmetryPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFunction (mathematics)High Energy Physics - PhenomenologyNeutrino detectorBeyond Standard Modellcsh:QC770-798High Energy Physics::ExperimentSolar and Atmospheric NeutrinosNeutrinoProduction rateLeptonJournal of High Energy Physics
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