0000000000293410

AUTHOR

Pablo Martínez-miravé

showing 4 related works from this author

Sterile neutrinos with altered dispersion relations revisited

2020

In this paper we investigate neutrino oscillations with altered dispersion relations in the presence of sterile neutrinos. Modified dispersion relations represent an agnostic way to parameterize new physics. Models of this type have been suggested to explain global neutrino oscillation data, including deviations from the standard three-neutrino paradigm as observed by a few experiments. We show that, unfortunately, in this type of models new tensions arise turning them incompatible with global data.

PhysicsNuclear and High Energy PhysicsParticle physicsSterile neutrino010308 nuclear & particles physicsPhysics beyond the Standard ModelHigh Energy Physics::PhenomenologyFOS: Physical sciences01 natural sciencesHigh Energy Physics - Experiment3. Good healthHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Dispersion relationBeyond Standard Model0103 physical scienceslcsh:QC770-798Neutrino Physicslcsh:Nuclear and particle physics. Atomic energy. RadioactivityHigh Energy Physics::Experiment010306 general physicsNeutrino oscillationJournal of High Energy Physics
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Signatures of primordial black hole dark matter at DUNE and THEIA

2021

Primordial black holes (PBHs) are a potential dark matter candidate whose masses can span over many orders of magnitude. If they have masses in the $10^{15}-10^{17}$ g range, they can emit sizeable fluxes of MeV neutrinos through evaporation via Hawking radiation. We explore the possibility of detecting light (non-)rotating PBHs with future neutrino experiments. We focus on two next generation facilities: the Deep Underground Neutrino Experiment (DUNE) and THEIA. We simulate the expected event spectra at both experiments assuming different PBH mass distributions and spins, and we extract the expected 95% C.L. sensitivities to these scenarios. Our analysis shows that future neutrino experime…

PhysicsPhotonCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterFOS: Physical sciencesAstronomy and AstrophysicsPrimordial black holeAstrophysicsParameter spaceHigh Energy Physics - ExperimentHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Orders of magnitude (time)Deep Underground Neutrino ExperimentNeutrinoAstrophysics - Cosmology and Nongalactic AstrophysicsHawking radiation
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Cosmological radiation density with non-standard neutrino-electron interactions

2021

Neutrino non-standard interactions (NSI) with electrons are known to alter the picture of neutrino decoupling from the cosmic plasma. NSI modify both flavour oscillations through matter effects, and the annihilation and scattering between neutrinos and electrons and positrons in the thermal plasma. In view of the forthcoming cosmological observations, we perform a precision study of the impact of non-universal and flavour-changing NSI on the effective number of neutrinos, $N_{eff}$. We present the variation of $N_{eff}$ arising from the different NSI parameters and discuss the existing degeneracies among them, from cosmology alone and in relation to the current bounds from terrestrial exper…

PhysicsNuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)CosmologiaAnnihilationNeutrino interactionsScatteringNeutrino oscillationsPhysicsQC1-999FOS: Physical sciencesFísicaElectronNeutrino decouplingPlasmaCosmologyCosmologyHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Astrophysical plasmaHigh Energy Physics::ExperimentNon-standard neutrino interactionsNeutrinoAstrophysics - 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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