Search results for "Beyond standard model"

showing 10 items of 92 documents

Minimal flavour seesaw models

2009

26 pages, 8 figures.-- ArXiv pre-print available at: http://arxiv.org/abs/0906.1461

PhysicsNuclear and High Energy PhysicsParticle physicsFlavourHigh Energy Physics::PhenomenologyFOS: Physical sciencesInverseFísicaLepton numberHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometrySimple (abstract algebra)Beyond Standard ModelHigh Energy Physics::ExperimentNeutrino PhysicsNeutrinoMixing (physics)Lepton
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Lepton jets from radiating dark matter

2015

Journal of High Energy Physics 2015.7 (2015): 045 reproduced by permission of Scuola Internazionale Superiore di Studi Avanzati (SISSA)

PhysicsParticle physicsGauge bosonNuclear and High Energy PhysicsToy modelPhotonElectromagnetic Processes and PropertiesDark matterHigh Energy Physics::PhenomenologyFísicaFOS: Physical sciencesFermionAstrophysics::Cosmology and Extragalactic AstrophysicsDark photonStandard ModelHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Parton ModelBeyond Standard ModelHigh Energy Physics::ExperimentLeptonJournal of High Energy Physics
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Searching for Physics Beyond the Standard Model in an Off-Axis DUNE Near Detector

2021

Next generation neutrino oscillation experiments like DUNE and T2HK are multi-purpose observatories, with a rich physics program beyond oscillation measurements. A special role is played by their near detector facilities, which are particularly well-suited to search for weakly coupled dark sector particles produced in the primary target. In this paper, we demonstrate this by estimating the sensitivity of the DUNE near detectors to the scattering of sub-GeV DM particles and to the decay of sub-GeV sterile neutrinos ("heavy neutral leptons"). We discuss in particular the importance of the DUNE-PRISM design, which allows some of the near detectors to be moved away from the beam axis. At such o…

Nuclear and High Energy Physics530 Physicshep-ex010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFOS: Physical scienceshep-ph10192 Physics InstituteQC770-79801 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Nuclear and particle physics. Atomic energy. RadioactivityBeyond Standard Model0103 physical sciencesNeutrino PhysicsHigh Energy Physics::Experiment3106 Nuclear and High Energy Physics010306 general physicsParticle Physics - ExperimentParticle Physics - Phenomenology
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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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Dijets at Tevatron Cannot Constrain SMEFT Four-Quark Operators

2019

We explore the sensitivity of Tevatron data to heavy new physics effects in differential dijet production rates using the SMEFT in light of the fact that consistent and conservative constraints from the LHC cannot cover relatively low cutoff scales in the EFT. In contrast to the results quoted by the experimental collaborations and other groups, we find that, once consistency of the perturbation expansion is enforced and reasonable estimates of theoretical errors induced by the SMEFT series in $\frac{E}{\Lambda}$ are included, there is no potential to constrain four-quark contact interactions using Tevatron data. This shows the general difficulty of constraining physics model-independently …

QuarkPhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderLuminosity (scattering theory)Physics beyond the Standard ModelHigh Energy Physics::PhenomenologyTevatronFOS: Physical sciencesEffective Field TheoriesLambdaComputer Science::Digital LibrariesHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Beyond Standard ModelComputer Science::Mathematical SoftwareCutofflcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityHigh Energy Physics::ExperimentSensitivity (control systems)
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Cuckoo's Eggs in Neutron Stars: Can LIGO Hear Chirps from the Dark Sector?

2018

We explore in detail the possibility that gravitational wave signals from binary inspirals are affected by a new force that couples only to dark matter particles. We discuss the impact of both the new force acting between the binary partners as well as radiation of the force carrier. We identify numerous constraints on any such scenario, ultimately concluding that observable effects on the dynamics of binary inspirals due to such a force are not possible if the dark matter is accrued during ordinary stellar evolution. Constraints arise from the requirement that the astronomical body be able to collect and bind at small enough radius an adequate number of dark matter particles, from the requ…

Nuclear and High Energy PhysicsAstrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)General relativitymedia_common.quotation_subjectgr-qcDark matterFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsStellar evolutionmedia_commonParticle Physics - PhenomenologyPhysics010308 nuclear & particles physicsStar formationGravitational wavehep-exGeneral Relativity and CosmologyFifth forcehep-phCosmology of Theories beyond the SMUniverseHigh Energy Physics - PhenomenologyNeutron starBeyond Standard Modelastro-ph.COlcsh:QC770-798Particle Physics - ExperimentAstrophysics - Cosmology and Nongalactic Astrophysics
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Sensitivity to charged scalars in B → D(*)τν and B → τν decays

2013

We analyze the recent experimental evidence for an excess of $\tau$-lepton production in several exclusive semileptonic $B$-meson decays in the context of two-Higgs-doublet models. These decay modes are sensitive to the exchange of charged scalars and constrain strongly their Yukawa interactions. While the usual Type-II scenario cannot accommodate the recent BaBar data, this is possible within more general models in which the charged-scalar couplings to up-type quarks are not as suppressed. Both the $B\to D^{(*)}\tau\nu_\tau$ and the $B\to\tau\nu_\tau$ data can be fitted within the framework of the Aligned Two-Higgs-Doublet Model, but the resulting parameter ranges are in conflict with the …

QuarkPhysicsParticle physicsNuclear and High Energy PhysicsB-Physics; Beyond Standard Model; High Energy Physics - Phenomenology; High Energy Physics - Phenomenology; High Energy Physics - Experiment; Nuclear and High Energy PhysicsPhysics beyond the Standard ModelB-PhysicsHigh Energy Physics::PhenomenologyScalar (mathematics)Yukawa potentialContext (language use)FermionHigh Energy Physics - ExperimentHigh Energy Physics - PhenomenologyBeyond Standard ModelHigh Energy Physics::ExperimentProduction (computer science)Charm (quantum number)
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Minimal supersymmetric inverse seesaw: neutrino masses, lepton flavour violation and LHC phenomenology

2009

We study neutrino masses in the framework of the supersymmetric inverse seesaw model. Different from the non-supersymmetric version a minimal realization with just one pair of singlets is sufficient to explain all neutrino data. We compute the neutrino mass matrix up to 1-loop order and show how neutrino data can be described in terms of the model parameters. We then calculate rates for lepton flavour violating (LFV) processes, such as mu -> e gamma and chargino decays to singlet scalar neutrinos. The latter decays are potentially observable at the LHC and show a characteristic decay pattern dictated by the same parameters which generate the observed large neutrino angles.

Nuclear and High Energy PhysicsParticle physicsSupersymmetric Standard ModelPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)CharginoSeesaw molecular geometry0103 physical sciencesNeutrino Physics010306 general physicsParticle Physics - PhenomenologyPhysicsLarge Hadron Collider010308 nuclear & particles physicsRare DecaysHigh Energy Physics::PhenomenologyFísicaObservableMass matrixHigh Energy Physics - PhenomenologyBeyond Standard ModelHigh Energy Physics::ExperimentNeutrinoPhenomenology (particle physics)Lepton
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Lepton-flavour violation in hadronic tau decays and μ-τ conversion in nuclei

2021

Within the Standard Model Effective Field Theory framework, with operators up to dimension 6, we perform a model-independent analysis of the lepton-flavour-violating processes involving tau leptons. Namely, we study hadronic tau decays and $\ell$--$\tau$ conversion in nuclei, with $\ell = e,\mu$. Based on available experimental limits, we establish constraints on the Wilson coefficients of the operators contributing to these processes. Our work paves the way to extract the related information from Belle II and foreseen future experiments.

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsFlavourHadronHigh Energy Physics::PhenomenologyEffective Field Theories01 natural sciencesPartícules (Física nuclear)High Energy Physics - ExperimentStandard ModelHigh Energy Physics - PhenomenologyDimension (vector space)Beyond Standard Model0103 physical sciencesEffective field theorylcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityHigh Energy Physics::Experiment010306 general physicsLepton
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Flavour violation at the LHC: type-I versus type-II seesaw in minimal supergravity

2009

20 pages, 13 figures.-- ISI article identifier:000267789100003.-- ArXiv pre-print avaible at:http://arxiv.org/abs/0903.1408

Nuclear and High Energy PhysicsParticle physicsFOS: Physical sciences01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometry0103 physical sciencesNeutrino Physics010306 general physicsNeutrino oscillationPhysicsLarge Hadron Collider010308 nuclear & particles physicsSupergravityMass generationHigh Energy Physics::PhenomenologyFísicaRare decaysHigh Energy Physics - PhenomenologySeesaw mechanismHigh Energy Physics::ExperimentBeyond standard modelNeutrinoLeptonSupersymmetric standard model
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