Search results for "neutrino physic"

showing 10 items of 70 documents

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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Relaxing cosmological neutrino mass bounds with unstable neutrinos

2020

At present, cosmological observations set the most stringent bound on the neutrino mass scale. Within the standard cosmological model ($\Lambda$CDM), the Planck collaboration reports $\sum m_\nu < 0.12\,\text{eV}$ at 95% CL. This bound, taken at face value, excludes many neutrino mass models. However, unstable neutrinos, with lifetimes shorter than the age of the universe $\tau_\nu \lesssim t_U$, represent a particle physics avenue to relax this constraint. Motivated by this fact, we present a taxonomy of neutrino decay modes, categorizing them in terms of particle content and final decay products. Taking into account the relevant phenomenological bounds, our analysis shows that 2-body deca…

Nuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Age of the universeFOS: Physical sciencesLambda-CDM model7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)symbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometry0103 physical sciencesNeutrino Physicslcsh:Nuclear and particle physics. Atomic energy. RadioactivityPlanck010306 general physicsPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyMass generationElectroweak interactionCosmology of Theories beyond the SMHigh Energy Physics - PhenomenologyBeyond Standard ModelGoldstone bosonsymbolslcsh:QC770-798High Energy Physics::ExperimentNeutrinoAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of High Energy Physics
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Shining Light on the Scotogenic Model: Interplay of Colliders and Cosmology

2019

In the framework of the scotogenic model, which features radiative generation of neutrino masses, we explore light dark matter scenario. Throughout the paper we chiefly focus on keV-scale dark matter which can be produced either via freeze-in through the decays of the new scalars, or from the decays of next-to-lightest fermionic particle in the spectrum, which is produced through freeze-out. The latter mechanism is required to be suppressed as it typically produces a hot dark matter component. Constraints from BBN are also considered and in combination with the former production mechanism they impose the dark matter to be light. For this scenario we consider signatures at High Luminosity LH…

Nuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesCosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNeutrino Physicslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsLight dark matterPhysicsLarge Hadron ColliderMissing energy010308 nuclear & particles physicsHot dark matterCosmology of Theories beyond the SMHigh Energy Physics - PhenomenologyBeyond Standard Modellcsh:QC770-798High Energy Physics::ExperimentNeutrinoLeptonAstrophysics - Cosmology and Nongalactic Astrophysics
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2020 global reassessment of the neutrino oscillation picture

2021

We present an updated global fit of neutrino oscillation data in the simplest three-neutrino framework. In the present study we include up-to-date analyses from a number of experiments. Concerning the atmospheric and solar sectors, we give updated analyses of DeepCore and SNO data, respectively. We have also included the latest electron antineutrino data collected by the Daya Bay and RENO reactor experiments, and the long-baseline T2K and NO$\nu$A measurements. These new analyses result in more accurate measurements of $\theta_{13}$, $\theta_{12}$, $\Delta m_{21}^2$ and $|\Delta m_{31}^2|$. The best fit value for the atmospheric angle $\theta_{23}$ lies in the second octant, but first octan…

Nuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciences01 natural sciences7. Clean energyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)CUOREDouble beta decay0103 physical sciencesNeutrino Physicslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsNeutrino oscillationNOνAPhysicsSudbury Neutrino Observatory010308 nuclear & particles physicsHigh Energy Physics - Phenomenology13. Climate actionBeyond Standard Modellcsh:QC770-798CP violationHigh Energy Physics::ExperimentNeutrinoElectron neutrinoAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of High Energy Physics
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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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A model of neutrino mass and dark matter with large neutrinoless double beta decay

2017

We propose a model where neutrino masses are generated at three loop order but neutrinoless double beta decay occurs at one loop. Thus we can have large neutrinoless double beta decay observable in the future experiments even when the neutrino masses are very small. The model receives strong constraints from the neutrino data and lepton flavor violating decays, which substantially reduces the number of free parameters. Our model also opens up the possibility of having several new scalars below the TeV regime, which can be explored at the collider experiments. Additionally, our model also has an unbroken $Z_2$ symmetry which allows us to identify a viable Dark Matter candidate.

Nuclear and High Energy PhysicsParticle physicsHiggs PhysicsDark matterFOS: Physical sciences01 natural scienceslaw.inventionHigh Energy Physics - Phenomenology (hep-ph)lawDouble beta decay0103 physical sciencesNeutrino Physicslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsColliderPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaObservableSymmetry (physics)High Energy Physics - PhenomenologyBeyond Standard Modellcsh:QC770-798High Energy Physics::ExperimentNeutrinoLeptonFree parameterJournal of High Energy Physics
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Resolving the octant of theta(23) with T2K and NOvA

2013

Preliminary results of MINOS experiment indicate that theta(23) is not maximal. Global fits to world neutrino data suggest two nearly degenerate solutions for theta(23): one in the lower octant (LO: theta(23) 45 degrees). v(mu) -> v(e) oscillations in superbeam experiments are sensitive to the octant and are capable of resolving this degeneracy. We study the prospects of this resolution by the current T2K and upcoming NOvA experiments. Because of the hierarchy-delta(CP) degeneracy and the octant delta(CP) degeneracy, the impact of hierarchy on octant resolution has to be taken into account. As in the case of hierarchy determination, there exist favorable (unfavorable) values of delta(CP) fo…

Nuclear and High Energy PhysicsParticle physicsPhysics - Instrumentation and DetectorsFOS: Physical sciencesSilver ChannelOctant (solid geometry)01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)SymmetryHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNeutrino Oscillation ExperimentsNeutrino Physics010306 general physicsNeutrino oscillationPhysicsNOνAMixing Matrix010308 nuclear & particles physicsDegenerate energy levelsCp ViolationInstrumentation and Detectors (physics.ins-det)High Energy Physics - PhenomenologyCP violationMINOSBeyond Standard ModelLine-Experiment-SimulatorMass MatrixCP violationNeutrinoIndraStra Global
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Minimal flavor violation in the see-saw portal

2020

We consider an extension of the Standard Model with two singlet leptons, with masses in the electroweak range, that induce neutrino masses via the see-saw mechanism, plus a generic new physics sector at a higher scale, $\Lambda$. We apply the minimal flavor violation (MFV) principle to the corresponding Effective Field Theory ($\nu$SMEFT) valid at energy scales $E \ll \Lambda$. We identify the irreducible sources of lepton flavor and lepton number violation at the renormalizable level, and apply the MFV ans\"atz to derive the scaling of the Wilson coefficients of the $\nu$SMEFT operators up to dimension six. We highlight the most important phenomenological consequences of this hypothesis in…

Nuclear and High Energy PhysicsParticle physicsPhysics beyond the Standard ModelFOS: Physical sciences01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesEffective field theoryNeutrino Physicslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsPhysics010308 nuclear & particles physicsElectroweak interactionHigh Energy Physics::Phenomenologybeyond standard model; CP violation; neutrino physicsLepton numberStandard Model (mathematical formulation)High Energy Physics - PhenomenologyCP violationBeyond Standard ModelHiggs bosonCP violationlcsh:QC770-798High Energy Physics::ExperimentNeutrinoJournal of High Energy Physics
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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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The seesaw portal in testable models of neutrino masses

2017

A Standard Model extension with two Majorana neutrinos can explain the measured neutrino masses and mixings, and also account for the matter-antimatter asymmetry in a region of parameter space that could be testable in future experiments. The testability of the model relies to some extent on its minimality. In this paper we address the possibility that the model might be extended by extra generic new physics which we parametrize in terms of a low-energy effective theory. We consider the effects of the operators of the lowest dimensionality, $d=5$, and evaluate the upper bounds on the coefficients so that the predictions of the minimal model are robust. One of the operators gives a new produ…

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsPhysics beyond the Standard ModelFOS: Physical sciences01 natural sciencesMinimal modelHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometry0103 physical sciencesEffective field theoryNeutrino Physicslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsParticle Physics - PhenomenologyPhysicsLarge Hadron Collider010308 nuclear & particles physicsHigh Energy Physics::Phenomenologyhep-phMAJORANAHigh Energy Physics - PhenomenologyBeyond Standard ModelHiggs bosonlcsh:QC770-798High Energy Physics::ExperimentNeutrinoJournal of High Energy Physics
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