Search results for "sterile"

showing 10 items of 164 documents

Heavy sterile neutrinos in stellar core-collapse

2018

We perform spherically symmetric simulations of the core collapse of a single progenitor star of zero age main sequence mass $M_{\rm ZAMS} = 15 \, M_{\odot}$ with two models of heavy sterile neutrinos in the mass range of hundred MeV$/c^2$. According to both models, these hypothetical particles are copiously produced in the center, stream outwards a subsequently decay releasing energy into final states (including neutrinos) of the Standard Model. We find that they can lead to a successful explosion in otherwise non-exploding progenitors. Depending on their unknown parameters (e.g., mass and coupling constants with matter), we obtain either no explosion or an explosion of one of two types, i…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSterile neutrino010308 nuclear & particles physicsStar (game theory)Astrophysics::High Energy Astrophysical PhenomenaCenter (category theory)FOS: Physical sciencesAstrophysicsType (model theory)01 natural sciences7. Clean energyStandard ModelSupernovaHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Astrophysics - Solar and Stellar Astrophysics0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsNeutrinoAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Energy (signal processing)Astrophysics::Galaxy Astrophysics
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Sterile neutrinos and flavor ratios in IceCube

2017

The flavor composition of astrophysical neutrinos observed in neutrino telescopes is a powerful discriminator between different astrophysical neutrino production mechanisms and can also teach us about the particle physics properties of neutrinos. In this paper, we investigate how the possible existence of light sterile neutrinos can affect these flavor ratios. We consider two scenarios: (i) neutrino production in conventional astrophysical sources, followed by partial oscillation into sterile states; (ii) neutrinos from dark matter decay with a primary flavor composition enhanced in tau neutrinos or sterile neutrinos. Throughout the paper, we constrain the sterile neutrino mixing parameters…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSterile neutrinoHigh energyParticle physicsMuonPhysics::Instrumentation and Detectors010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyDark matterFOS: Physical sciencesFluxAstronomy and AstrophysicsBaseline data01 natural sciences3. Good healthHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical Phenomena010306 general physicsFlavorJournal of Cosmology and Astroparticle Physics
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Production of keV sterile neutrinos in supernovae: New constraints and gamma-ray observables

2019

We study the production of sterile neutrinos in supernovae, focusing in particular on the keV--MeV mass range, which is the most interesting range if sterile neutrinos are to account for the dark matter in the Universe. Focusing on the simplest scenario in which sterile neutrinos mixes only with muon or tau neutrino, we argue that the production of keV--MeV sterile neutrinos can be strongly enhanced by a Mikheyev--Smirnov--Wolfenstein (MSW) resonance, so that a substantial flux is expected to emerge from a supernova, even if vacuum mixing angles between active and sterile neutrinos are tiny. Using energetics arguments, this yields limits on the sterile neutrino parameter space that reach do…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSterile neutrinoParticle physicsPhysics::Instrumentation and Detectors010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaSolar neutrinoHigh Energy Physics::PhenomenologyFOS: Physical sciencesSolar neutrino problemComputer Science::Digital Libraries7. Clean energy01 natural sciencesCosmic neutrino backgroundHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Neutrino detector0103 physical sciencesMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino astronomyNeutrinoAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsPhysical Review D
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Sterile neutrinos and B–L symmetry

2017

We revisit the relation between the neutrino masses and the spontaneous breaking of the B-L gauge symmetry. We discuss the main scenarios for Dirac and Majorana neutrinos and point out two simple mechanisms for neutrino masses. In this context the neutrino masses can be generated either at tree level or at quantum level and one predicts the existence of very light sterile neutrinos with masses below the eV scale. The predictions for lepton number violating processes such as mu to e and mu to e gamma are discussed in detail. The impact from the cosmological constraints on the effective number of relativistic degree of freedom is investigated.

High Energy Physics - TheoryNuclear and High Energy PhysicsSterile neutrinoParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesContext (language use)Computer Science::Digital Libraries01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationGauge symmetryPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyLepton numberlcsh:QC1-999High Energy Physics - PhenomenologyMAJORANAHigh Energy Physics - Theory (hep-th)Measurements of neutrino speedHigh Energy Physics::ExperimentNeutrinolcsh:PhysicsAstrophysics - Cosmology and Nongalactic AstrophysicsPhysics Letters B
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Light sterile neutrino from extra dimensions and four-neutrino solutions to neutrino anomalies

1999

We propose a four-neutrino model which can reconcile the existing data coming from underground experiments in terms of neutrino oscillations, together with the hint from the LSND experiment and a possible neutrino contribution to the hot dark matter of the Universe. It applies the idea that extra compact dimensions, probed only by gravity and possibly gauge-singlet fields, can lower the fundamental scales such as the Planck, string or unification scales. Our fourth light neutrino $\nu_s$ ($s$ for sterile) is identified with the zero mode of the Kaluza-Klein states. To first approximation \nu_sterile combines with the nu_mu in order to form a Dirac neutrino with mass in the eV range leaving …

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsParticle physicsSterile neutrinoHot dark matterSolar neutrinoHigh Energy Physics::PhenomenologyFísicaFOS: Physical sciencesMassless particleHigh Energy Physics - PhenomenologyExtra dimensionsHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Measurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationPhysical Review D
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Sterile Neutrinos, Black Hole Vacuum and Holographic Principle

2021

We construct an effective field theory (EFT) model that describes matter field interactions with Schwarzschild mini-black-holes (SBH's), treated as a scalar field, $B_0(x)$. Fermion interactions with SBH's require a random complex spurion field, $\theta_{ij}$, which we interpret as the EFT description of "holographic information," which is correlated with the SBH as a composite system. We consider Hawking's virtual black hole vacuum (VBH) as a Higgs phase, $\langle B_0 \rangle =V$. Integrating sterile neutrino loops, the field $\theta_{ij}$ is promoted to a dynamical field, necessarily developing a tachyonic instability and acquiring a VEV of order the Planck scale. For $N$ sterile neutrino…

High Energy Physics - TheorySterile neutrinoParticle physicsPhysics and Astronomy (miscellaneous)FOS: Physical scienceslcsh:AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:QB460-466Effective field theorylcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsVirtual black holeEngineering (miscellaneous)Physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyOrder (ring theory)Higgs phaseBlack holeHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)lcsh:QC770-798Scalar fieldSchwarzschild radius
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Omnibus experiment: CPT and CP violation with sterile neutrinos

2017

The verification of the sterile neutrino hypothesis and, if confirmed, the determination of the relevant oscillation parameters is one of the goals of the neutrino physics in near future. We propose to search for the sterile neutrinos with a high statistics measurement utilizing the radioactive sources and oscillometric approach with large liquid scintillator detector like LENA, JUNO, or RENO-50. Our calculations indicate that such an experiment is realistic and could be performed in parallel to the main research plan for JUNO, LENA, or RENO-50. Assuming as the starting point the values of the oscillation parameters indicated by the current global fit (in 3 + 1 scenario) and requiring at le…

HistoryCP violationPhysics::Instrumentation and Detectorssterile neutrinosneutrino oscillometryHigh Energy Physics::PhenomenologyneutriinotHigh Energy Physics::ExperimentCPT violationComputer Science ApplicationsEducationJournal of Physics: Conference Series
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Understanding the detector behavior through Montecarlo and calibration studies in view of the SOX measurement

2015

International audience; Borexino is an unsegmented neutrino detector operating at LNGS in central Italy. The experiment has shown its performances through its unprecedented accomplishments in the solar and geoneutrino detection. These performances make it an ideal tool to accomplish a state- of-the-art experiment able to test the existence of sterile neutrinos (SOX experiment). For both the solar and the SOX analysis, a good understanding of the detector response is fundamental. Consequently, calibration campaigns with radioactive sources have been performed over the years. The calibration data are of extreme importance to develop an accurate Monte Carlo code. This code is used in all the n…

HistoryGeoneutrinoCalibration (statistics)Physics::Instrumentation and DetectorsNuclear engineeringMonte Carlo method01 natural sciencesprogrammingParticle detectorEducationPhysics and Astronomy (all)0103 physical sciencesddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsSimulationBorexinoPhysics010308 nuclear & particles physicsDetectorneutrino: sterilecalibrationComputer Science::Computers and SocietyComputer Science ApplicationsNeutrino detectorBorexinoHigh Energy Physics::ExperimentNeutrinonumerical calculations: Monte Carloperformance
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SOX: search for short baseline neutrino oscillations with Borexino

2015

International audience; The Borexino detector has convincingly shown its outstanding performances in the low energy regime through its accomplishments in the observation and study of the solar and geo neutrinos. It is then an ideal tool to perform a state of the art source-based experiment for testing the longstanding hypothesis of a fourth sterile neutrino with ~ eV(2) mass, as suggested by several anomalies accumulated over the past three decades in source, reactor, and accelerator-based experiments. The SOX project aims at successively deploying two intense radioactive sources, made of Cerium (antineutrino) and Chromium (neutrino), respectively, in a dedicated pit located beneath the det…

HistoryParticle physicsSterile neutrinochromium: nuclidePhysics::Instrumentation and DetectorsSolar neutrino[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences7. Clean energyEducationNuclear physicsPhysics and Astronomy (all)0103 physical sciencesddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNeutrino oscillationBorexinoactivity reportPhysics010308 nuclear & particles physicsHigh Energy Physics::Phenomenologyneutrino: particle sourceSolar neutrino problemneutrino: sterilesensitivityComputer Science ApplicationsNeutrino detector13. Climate actioncerium: nuclideMeasurements of neutrino speedHigh Energy Physics::ExperimentBorexinoneutrino: oscillationNeutrinoantineutrino: particle source
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The $^{144}$Ce source for SOX

2015

International audience; The SOX (Short distance neutrino Oscillations with BoreXino) project aims at testing the light sterile neutrino hypothesis. To do so, two artificials sources of antineutrinos and neutrinos respectively will be consecutively deployed at the Laboratori Nazionali del Gran Sasso (LNGS) in close vicinity to Borexino, a large liquid scintillator detector. This document reports on the source production and transportation. The source should exhibit a long lifetime and a high decay energy, a requirement fullfilled by the (144)Ce-(144)Pr pair at secular equilibrium. It will be produced at FSUE “Mayak” PA using spent nuclear fuel. It will then be shielded and packed according t…

HistorySterile neutrinoParticle physicsenergy: decay[PHYS.PHYS.PHYS-ACC-PH]Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph]Scintillator01 natural sciences7. Clean energyEducationNuclear physicsPhysics and Astronomy (all)0103 physical sciencesddc:530010306 general physicsNeutrino oscillationparticle sourceBorexinoPhysicslifetimenucleusSecular equilibriumneutrino: sterileantineutrinosensitivitySpent nuclear fuelComputer Science ApplicationsGran SassoceriumDecay energyradioactivityBorexinoneutrino: oscillationproductionNeutrino
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