Search results for "NEUTRINOS"

showing 10 items of 206 documents

Probing Planck scale physics with IceCube

2005

Neutrino oscillations can be affected by decoherence induced e.g. by Planck scale suppressed interactions with the space-time foam predicted in some approaches to quantum gravity. We study the prospects for observing such effects at IceCube, using the likely flux of TeV antineutrinos from the Cygnus spiral arm. We formulate the statistical analysis for evaluating the sensitivity to quantum decoherence in the presence of the background from atmospheric neutrinos, as well as from plausible cosmic neutrino sources. We demonstrate that IceCube will improve the sensitivity to decoherence effects of ${\cal O}(E^2/M_{\rm Pl})$ by 17 orders of magnitude over present limits and, moreover, that it ca…

High Energy Physics - TheoryAstrofísicaNuclear and High Energy PhysicsParticle physicsField theory (Physics)Quantum decoherenceAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics7. Clean energy01 natural sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesTeoria quànticaNeutrinsSensitivity (control systems)Neutrinos010306 general physicsNeutrino oscillationPhysicsCOSMIC cancer database010308 nuclear & particles physicsAstrophysics (astro-ph)Teoria de camps (Física)High Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Orders of magnitude (time)13. Climate actionQuantum theoryQuantum gravityNeutrinoPhysical Review D
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Generalized mu-tau reflection symmetry and leptonic CP violation

2016

14 pages.- 9 figures

High Energy Physics - TheoryNOνAPhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFlavor symmetry01 natural sciencesDouble beta decaylcsh:QC1-999High Energy Physics - PhenomenologyMAJORANAReflection (mathematics)Reflection symmetryDouble beta decay0103 physical sciencesCP violationHigh Energy Physics::Experiment010306 general physicsNeutrino oscillationlcsh:PhysicsMajorana neutrinosLepton
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Limits on neutrino Lorentz violation from multimessenger observations of TXS 0506+056

2019

The observation by the IceCube Collaboration of a high-energy ($E \gtrsim 200$ TeV) neutrino from the direction of the blazar TXS 0506+056 and the coincident observations of enhanced $\gamma$-ray emissions from the same object by MAGIC and other experiments can be used to set stringent constraints on Lorentz violation in the propagation of neutrinos that is linear in the neutrino energy: $\Delta v = - E/M_1$, where $\Delta v$ is the deviation from the velocity of light, and $M_1$ is an unknown high energy scale to be constrained by experiment. Allowing for a difference in neutrino and photon propagation times of $\sim 10$ days, we find that $M_1 \gtrsim 3 \times 10^{16}$ GeV. This improves …

High Energy Physics - TheoryNuclear and High Energy PhysicsHigh energyParticle physicsAstrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)Lorentz transformationgr-qcAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesComputer Science::Digital LibrariesGeneral Relativity and Quantum CosmologyIceCubesymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Coincident0103 physical sciences010306 general physicsBlazarParticle Physics - PhenomenologyHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HEMultimessenger010308 nuclear & particles physicsGeneral Relativity and Cosmologyhep-thHigh Energy Physics::PhenomenologyLorentz violationGamma rayhep-phlcsh:QC1-999High Energy Physics - PhenomenologyPhoton propagationHigh Energy Physics - Theory (hep-th)Astrophysical neutrinosVelocity of lightsymbolsastro-ph.COHigh Energy Physics::ExperimentNeutrinoTXS 0506+056Astrophysics - High Energy Astrophysical PhenomenaParticle Physics - Theorylcsh:PhysicsBlazarsAstrophysics - Cosmology and Nongalactic AstrophysicsPhysics Letters
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Reloading the Axion in a 3-3-1 setup

2020

We generalize the idea of the axion to an extended electroweak gauge symmetry setup. We propose a minimal axion extension of the Singer-Valle-Schechter (SVS) theory, in which the standard model fits in $\mathrm{SU(3)_L\otimes U(1)_X}$, the number of families results from anomaly cancellation, and the Peccei-Quinn (PQ) solution to the strong-CP problem is implemented. Neutrino masses arise from a type-I Dirac seesaw mechanism, suppressed by the ratio of SVS and PQ scales, suggesting the existence of new physics at a moderate SVS scale. Novel features include an enhanced axion coupling to photons when compared to the DFSZ axion, as well as flavour-changing axion couplings to quarks.

High Energy Physics - TheoryNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsPhysics beyond the Standard ModelFOS: Physical sciencesStandard ModelHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics::TheoryAxionHigh Energy Physics - Phenomenology (hep-ph)Peccei-Quinn symmetryNeutrinosAxionGauge symmetryPhysicsElectroweak interactionHigh Energy Physics::Phenomenologylcsh:QC1-999High Energy Physics - PhenomenologySeesaw mechanismHigh Energy Physics - Theory (hep-th)Anomaly (physics)Neutrinolcsh:Physics
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Theory and phenomenology of Dirac neutrinos: Symmetry breaking patterns, flavour implications and Dark Matter

2021

El Modelo Estándar (SM en ingles) de interacciones Electro-Débiles (EW en inglés) ha sido un gran éxito desde un punto de vista teórico y experimental. Si bien este éxito no se puede negar, es hora de avanzar y abordar las preguntas que el SM deja sin respuesta, como las masas de neutrinos, la naturaleza de la materia oscura, el problema de la jerarquía o el problema de violación de CP en el sector de las interacciones fuertes, entre otros. De hecho, el SM predice neutrinos sin masa. Sin embargo, los experimentos de oscilación de neutrinos, que ahora alcanzan la era de la precisión, muestran claramente que al menos dos neutrinos son masivos y arrojan luz sobre su patrón de mezcla. Sin embar…

High Energy Physics::Phenomenology:FÍSICA::Física de altas energías::Física teórica altas energías [UNESCO]High Energy Physics::Experimentdirac neutrinosUNESCO::FÍSICA::Física de altas energías::Física teórica altas energías
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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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Overview and accomplishments of the Borexino experiment

2015

International audience; The Borexino experiment is running at the Laboratori del Gran Sasso in Italy since 2007. Its technical distinctive feature is the unprecedented ultralow background of the inner scintillating core, which is the basis of the outstanding achievements accumulated by the experiment. In this talk, after recalling the main features of the detector, the impressive solar data gathered so far by the experiment will be summarized, with special emphasis to the most recent and prominent result concerning the detection of the fundamental pp solar neutrino flux, which is the direct probe of the engine mechanism powering our star. Such a milestone measurement puts Borexino in the un…

Historyneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoreview[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]7. Clean energy01 natural sciencesneutrino: fluxEducationNuclear physicsPhysics and Astronomy (all)energy: solarstar0103 physical sciencesAstrophysics::Solar and Stellar Astrophysicsddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsBorexinoPhysicsSolar energetic particlesbusiness.industrybackgroundAstronomyoscillationSolar energyComputer Science ApplicationsGran SassoMassless particleNEUTRINOSNeutrino detectorPhysics::Space PhysicsBorexinoNeutrinobusinessLepton
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Searches for small-scale anisotropies from neutrino point sources with three years of IceCube data

2015

Recently, IceCube found evidence for a diffuse signal of astrophysical neutrinos in an energy range of $60\,\mathrm{TeV}$ to the $\mathrm{PeV}$-scale. The origin of those events, being a key to understanding the origin of cosmic rays, is still an unsolved question. So far, analyses have not succeeded to resolve the diffuse signal into point-like sources. Searches including a maximum-likelihood-ratio test, based on the reconstructed directions and energies of the detected down- and up-going neutrino candidates, were also performed on IceCube data leading to the exclusion of bright point sources. In this paper, we present two methods to search for faint neutrino point sources in three years o…

J.2Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayScale (descriptive set theory)AstrophysicsIceCubelaw.inventionTelescopelawPoint (geometry)Anisotropyastro-ph.HE2pt-correlationHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsHigh Energy Physics::Phenomenology2pt-correlation; Astrophysical neutrinos; Extraterrestrial neutrinos; IceCube; Multipole analysis; Point sourcesAstrophysics::Instrumentation and Methods for AstrophysicsPoint sourcesAstronomyAstronomy and AstrophysicsMultipole analysis3. Good health85-05Astrophysical neutrinosddc:540Extraterrestrial neutrinosHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaMultipole expansionGamma-ray burstAstroparticle Physics
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Deep sea tests of a prototype of the KM3NeT digital optical module

2014

SIRE(opens in a new window)|View at Publisher| Export | Download | Add to List | More... European Physical Journal C Volume 74, Issue 9, 1 September 2014, 8p Deep sea tests of a prototype of the KM3NeT digital optical module: KM3NeT Collaboration (Article) Adrián-Martínez, S.a, Ageron, M.b, Aharonian, F.c, Aiello, S.d, Albert, A.e, Ameli, F.f, Anassontzis, E.G.g, Anghinolfi, M.h, Anton, G.i, Anvar, S.j, Ardid, M.a, de Asmundis, R.k, Balasi, K.l, Band, H.m, Barbarino, G.kn, Barbarito, E.o, Barbato, F.kn, Baret, B.p, Baron, S.p, Belias, A.lq, Berbee, E.m, van den Berg, A.M.r, Berkien, A.m, Bertin, V.b, Beurthey, S.b, van Beveren, V.m, Beverini, N.st, Biagi, S.uv, Bianucci, S.t, Billault, M.b,…

KM3NeT; digital optical modulePhysics - Instrumentation and Detectors[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Physics and Astronomy (miscellaneous)TELESCOPEPhysics::Instrumentation and Detectorsdigital optical moduleFOS: Physical sciencesNeutrino Telescopesneutrino astrophysics; Cherenkov detector; Neutrino TelescopesKM3NeT; Cherenkov; UnderwaterDESIGNCherenkov[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Instrumentation and Methods for Astrophysics (astro-ph.IM)KM3NeTEngineering (miscellaneous)Astrophysics::Instrumentation and Methods for Astrophysicsneutrino telescopeDATA-ACQUISITIONInstrumentation and Detectors (physics.ins-det)READOUTneutrino astrophysics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]NEUTRINOSUnderwaterAstrophysics - Instrumentation and Methods for AstrophysicsSYSTEMCherenkov detector
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A New Low Background Laboratory in the Pyhäsalmi Mine : Towards 14C free liquid scintillator for low energy neutrino experiments

2017

A new low background laboratory in Pyhäsalmi mine in the Central Finland has been put into operation in the beginning of 2017. The laboratory operates at the depth of 1436 m (~4100 meters of water equivalent). In this paper, we present description of the laboratory’s existing facility and background conditions. In the laboratory, a series of measurements has been started where the 14C concentration is determined from several liquid scintillator samples. A dedicated setup has been designed and constructed with the aim of measuring the 14C/12C ratio smaller than 10-18 . peerReviewed

Low energyta114research equipmentcosmic radiationNuclear engineeringtutkimuslaitteetneutriinotEnvironmental scienceneutrinosNeutrinoScintillatorWater equivalentkosminen säteily
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