Search results for "partícules"

showing 10 items of 522 documents

Anomalies in b→s Transitions and Dark Matter

2018

Since 2013, the LHCb collaboration has reported on the measurement of several observables associated to $b \to s$ transitions, finding various deviations from their predicted values in the Standard Model. These include a set of deviations in branching ratios and angular observables, as well as in the observables $R_K$ and $R_{K^\ast}$, specially built to test the possible violation of Lepton Flavor Universality. Even though these tantalizing hints are not conclusive yet, the $b \to s$ anomalies have gained considerable attention in the flavor community. Here we review New Physics models that address these anomalies and explore their possible connection to the dark matter of the Universe. Af…

PhysicsNuclear and High Energy Physics010308 nuclear & particles physicsPhysics beyond the Standard ModelDark matterFOS: Physical sciencesObservable01 natural scienceslcsh:QC1-999Partícules (Física nuclear)Universality (dynamical systems)High Energy Physics - PhenomenologyTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicslcsh:PhysicsLeptonAdvances in High Energy Physics
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Neutrino Bremsstrahlung from electrons in neutron star crusts

2001

The process of v (v) over bar Bremsstrahlung via electron scattering off nuclei in the crust of a cooling neutron star is studied within the Random Phase Approximation. We show that the electromagnetic plasma screens the vector weak coupling of electrons with the neutrino field. This screening effect takes place in both the crystalline and liquid phase of the neutron star crust, when the momentum carried out by the neutrino pair is smaller than the inverse Debye screening distance of the electrons. This condition holds in the crust volume at temperatures and densities where the electron Bremsstrahlung dominates the neutrino production. As a result, the vector weak current contribution to th…

PhysicsNuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaDegenerate energy levelsBremsstrahlungElectronAstrophysicsRadiationPartícules (Física nuclear)Nuclear physicsNeutron starEmissivityFísica nuclearNeutrinoBar (unit)
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Diagnostic Potential of Cosmic-Neutrino Absorption Spectroscopy

2004

Annihilation of extremely energetic cosmic neutrinos on the relic-neutrino background can give rise to absorption lines at energies corresponding to formation of the electroweak gauge boson $Z^{0}$. The positions of the absorption dips are set by the masses of the relic neutrinos. Suitably intense sources of extremely energetic ($10^{21}$ -- $10^{25}$-eV) cosmic neutrinos might therefore enable the determination of the absolute neutrino masses and the flavor composition of the mass eigenstates. Several factors--other than neutrino mass and composition--distort the absorption lines, however. We analyze the influence of the time-evolution of the relic-neutrino density and the consequences of …

PhysicsNuclear and High Energy PhysicsGauge bosonParticle physicsCosmologiaPhysics::Instrumentation and Detectorsmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaDark matterAstrophysics (astro-ph)High Energy Physics::PhenomenologyFOS: Physical sciencesAstrophysicsPartícules (Física nuclear)UniverseCosmic neutrino backgroundHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Measurements of neutrino speedInvariant massHigh Energy Physics::ExperimentAbsorption (logic)Neutrinomedia_common
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Search for B^{+}→τ^{+}ν

2007

We present a search for the decay B + → τ + ν using 383 × 10 6 B ¯¯¯ B pairs collected at the Υ ( 4 S ) resonance with the BABAR detector at the SLAC PEP-II B -Factory. A sample of events with one reconstructed semileptonic B decay ( B − → D 0 ℓ − ¯ ν ℓ X ) is selected, and in the recoil a search for B + → τ + ν is performed. The τ is identified in the following channels: τ + → e + ν ¯ ν , τ + → μ + ν ¯ ν , τ + → π + ¯ ν , and τ + → π + π 0 ¯ ν . We measure a branching fraction of B ( B + → τ + ν ) = ( 0.9 ± 0.6 ( stat . ) ± 0.1 ( syst . ) ) × 10 − 4 . In the absence of a significant signal, we calculate an upper limit at the 90% confidence level of B ( B + → τ + ν ) < 1.7 × 10 − 4 . We cal…

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsBranching fractionElectron–positron annihilationParticle physicsResonanceBABAR detector01 natural sciencesHEPParticle identificationStandard ModelNuclear physicsRecoilBaBar0103 physical sciencesB mesonExponential decay010306 general physicsFísica de partículesExperiments
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Prospects for the Zee-Babu Model at the LHC and low energy experiments

2007

We analyze the viability of the Zee-Babu model as an explanation of observed neutrino masses and mixings and the possibility that the model is confirmed or discarded in experiments planned for the very close future. The allowed parameter space is studied analytically by using some approximations and partial data. Then, a complete scanning of all parameters and constraints is performed numerically by using Monte Carlo methods. The cleanest signal of the model will be the detection of the doubly charged scalar at the LHC and its correlation with measurements of the branching ratio of $\mu\to e\gamma$ at the MEG experiment. In addition, the model offers interesting predictions for $\tau^{-}\to…

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsBranching fractionHadronMonte Carlo methodHigh Energy Physics::PhenomenologyDrell–Yan processFOS: Physical sciencesParameter space7. Clean energy01 natural sciencesPartícules (Física nuclear)Nuclear physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Double beta decay0103 physical sciencesHigh Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillation
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WIMP dark matter as radiative neutrino mass messenger

2013

The minimal seesaw extension of the Standard SU(3)(c)circle times SU(2)(L)circle times U(1)(Y) Model requires two electroweak singlet fermions in order to accommodate the neutrino oscillation parameters at tree level. Here we consider a next to minimal extension where light neutrino masses are generated radiatively by two electroweak fermions: one singlet and one triplet under SU(2)(L). These should be odd under a parity symmetry and their mixing gives rise to a stable weakly interactive massive particle (WIMP) dark matter candidate. For mass in the GeV-TeV range, it reproduces the correct relic density, and provides an observable signal in nuclear recoil direct detection experiments. The f…

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsDark matterElectroweak interactionHigh Energy Physics::PhenomenologyMassive particleFOS: Physical sciencesFermionCosmology of Theories beyond the SM7. Clean energy01 natural sciencesPartícules (Física nuclear)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometryWIMP0103 physical sciencesBeyond Standard ModelHigh Energy Physics::ExperimentNeutrino PhysicsNeutrino010306 general physicsNeutrino oscillation
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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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Testing a lepton quarticity flavor theory of neutrino oscillations with the DUNE experiment

2018

Oscillation studies play a central role in elucidating at least some aspects of the flavor problem. Here we examine the status of the predictions of a lepton quarticity flavor theory of neutrino oscillations against the existing global sample of oscillation data. By performing quantitative simulations we also determine the potential of the upcoming DUNE experiment in narrowing down the currently ill-measured oscillation parameters $\theta_{23}$ and $\delta_{\text{CP}}$. We present the expected improved sensitivity on these parameters for different assumptions.

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsOscillationHigh Energy Physics::PhenomenologyFOS: Physical sciences01 natural scienceslcsh:QC1-999Partícules (Física nuclear)High Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesHigh Energy Physics::ExperimentSensitivity (control systems)010306 general physicsNeutrino oscillationlcsh:PhysicsFlavorLepton
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Exploring the intrinsic Lorentz-violating parameters at DUNE

2018

Neutrinos can push our search for new physics to a whole new level. What makes them so hard to be detected, what allows them to travel humongous distances without being stopped or deflected allows to amplify Planck suppressed effects (or effects of comparable size) to a level that we can measure or bound in DUNE. In this work we analyze the sensitivity of DUNE to CPT and Lorentz-violating interactions in a framework that allows a straightforward extrapolation of the bounds obtained to any phenomenological modification of the dispersion relation of neutrinos.

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsPhysics beyond the Standard ModelLorentz transformationExtrapolationFOS: Physical sciences01 natural sciencesMeasure (mathematics)Partícules (Física nuclear)lcsh:QC1-999High Energy Physics - ExperimentHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)symbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Dispersion relation0103 physical sciencessymbolsSensitivity (control systems)NeutrinoPlanck010306 general physicslcsh:PhysicsPhysics Letters B
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Tau spin correlations and the anomalous magnetic moment

2009

We show that the precise determination of the Tau magnetic properties is possible in the next generation accelerators, specially at B/Flavour factories. We define spin correlation observables suitable to extract the real part of the magnetic form factor that, for the first time, will allow to test the standard model-QED predictions. In particular, the predicted QED-dependence with both the momentum transfer and the lepton mass can be precisely measured. Until now, the most stringent bounds on the $\tau$ magnetic moment $a_\tau$ come from LEP data with strong assumptions on the physics involved on the observed process. In this paper, we find three different combinations of spin correlations …

PhysicsNuclear and High Energy PhysicsParticle physicsAnomalous magnetic dipole momentMagnetic momentAcceleradors de partículesMomentum transferElectromagnetic processes and propertiesFOS: Physical sciencesObservableElectronPartícules (Física nuclear)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)AmplitudeMagnetic form factorHigh Energy Physics::ExperimentLeptonStandard model
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