Search results for "massless"

showing 10 items of 191 documents

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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Inflation might be caused by the right

2009

15 pages, 4 figures.-- ISI article identifier: 000265600800102.-- ArXiv pre-print avaible at: http://arxiv.org/abs/0811.2998

Inflation (cosmology)PhysicsNuclear and High Energy PhysicsParticle physicsBeyond Standard ModelAstrophysics (astro-ph)FOS: Physical sciencesElementary particleFermionInflatonAstrophysicsMassless particleHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Neutrino PhysicsNeutrinoScalar fieldComputer Science::DatabasesLeptonCosmology of Theories beyond the SM
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Neutrino masses, Majorons, and muon decay

1987

5 páginas, 3 figuras.

Massless particleNuclear physicsPhysicsParticle physicsMAJORANAMuonHigh Energy Physics::PhenomenologyHigh Energy Physics::ExperimentElementary particleFermionNeutrinoLeptonMajoron
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Hyperchargeless triplet Majoron model.

1989

We study the general conditions to maintain the scale of the lepton-number-breaking vacuum expectation value at the electroweak scale. It is shown that the only possibilities are if the main component of the resulting Majoron is a hyperchargeless complex triplet or a neutral singlet. Models with a hyperchargeless triplet, even though phenomenologically more interesting, seem to be very difficult to build because they like to break charge conservation. However, we have found a particular extension, by adding an additional neutral singlet, that solves this problem. The model can give a Majorana mass to the neutrinos in the eV range, ..mu -->..e..gamma.. can proceed with branching ratios at th…

Massless particlePhysicsMAJORANAParticle physicsBranching fractionHigh Energy Physics::PhenomenologyElementary particleSinglet stateElectroweak scalePartícules (Física nuclear)Vacuum expectation valueMajoronPhysical review. D, Particles and fields
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The Boson Fermion Correspondence

1989

In 1932 Louis de Broglie suggested that photons could be constructed from pairs of neutrinos [de Broglie, 1932]. Both are massless particles (except for some recent unconfirmed experiments according to which the neutrino could have a very small mass) and are electrically neutral. The main difference between free photons and free neutrinos is that the former obeys Bose statistics and the second Fermi statistics. The spin of a photon is 1 and the spin of a neutrino is 1/2 and therefore kinematically it should be possible to think of a photon as a neutrino pair. However, this old formulation of boson fermion equivalence has not been very fruitful in particle physics. Instead, there has been a …

Massless particlePhysicsParticle physicsFermion doublingHigh Energy Physics::PhenomenologyMatter waveFermionScalar bosonNeutrinoInteracting boson modelBoson
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Singletons on AdSn

2000

We define the singletons for the invariance group \( {\overline S _n} = {\overline {SO} _0}\left( {2,n - 1} \right) \)) of the AdS n space-time. We write down some of their important properties and characterizations. It is found that the tensor product of singletons of spin 0 or 1/2 decomposes into representations that are a kind of massless representations of S n . Other kinds of massless representations, related to singletons, are also studied and a comparison is made. Various Gupta-Bleuler triplets are constructed for singletons and for massless representations.

Massless particlePhysicsTensor productGroup (mathematics)High Energy Physics::PhenomenologyAnti-de Sitter spaceMathematical physicsSpin-½
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The next-to-ladder approximation for linear Dyson–Schwinger equations

2007

We solve the linear Dyson Schwinger equation for a massless vertex in Yukawa theory, iterating the first two primitive graphs.

Massless particleVertex (graph theory)PhysicsGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryNuclear and High Energy PhysicsHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyYukawa potentialLinear approximationMathematical physicsDyson seriesPhysics Letters B
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Probing non-standard neutrino interactions with supernova neutrinos

2007

17 pages, 12 figures.-- PACS nrs.: 13.15.+g; 14.60.Lm; 14.60.St; 97.60.Bw.-- ISI Article Identifier: 000249786800015.-- ArXiv pre-print available at: http://arxiv.org/abs/0704.0032

Matter densityNuclear and High Energy PhysicsParticle physicsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaSolar neutrinosFOS: Physical sciencesElectronStandard ModelScatteringHigh Energy Physics - Phenomenology (hep-ph)Core-collapse supernovaeMassless neutrinosElectroweak parametersNeutrino oscillationEnvelope (waves)PhysicsNeutrino oscillationsHigh Energy Physics::PhenomenologyFísicaSupernovaHigh Energy Physics - PhenomenologyNeutrino detectorResonant amplificationHigh Energy Physics::ExperimentNeutrino
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The Multiscale Stochastic Model of Fractional Hereditary Materials (FHM)

2013

Abstract In a recent paper the authors proposed a mechanical model corresponding, exactly, to fractional hereditary materials (FHM). Fractional derivation index 13 E [0,1/2] corresponds to a mechanical model composed by a column of massless newtonian fluid resting on a bed of independent linear springs. Fractional derivation index 13 E [1/2, 1], corresponds, instead, to a mechanical model constituted by massless, shear-type elastic column resting on a bed of linear independent dashpots. The real-order of derivation is related to the exponent of the power-law decay of mechanical characteristics. In this paper the authors aim to introduce a multiscale fractance description of FHM in presence …

Multiscale FractanceRandom modelsStochastic modellingMathematical analysisModel parametersGeneral MedicineFractional HereditarinessDashpotFractional calculusMassless particleFractional DerivativesFractional Derivatives; Fractional Hereditariness; Multiscale Fractance; Random modelsFractional HereditarineCalculusExponentNewtonian fluidLinear independenceFractional DerivativeMathematicsProcedia IUTAM
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Constraints on the extremely-high energy cosmic neutrino flux with the IceCube 2008-2009 data

2011

We report on a search for extremely-high energy neutrinos with energies greater than $10^6$ GeV using the data taken with the IceCube detector at the South Pole. The data was collected between April 2008 and May 2009 with the half completed IceCube array. The absence of signal candidate events in the sample of 333.5 days of livetime significantly improves model independent limit from previous searches and allows to place a limit on the diffuse flux of cosmic neutrinos with an $E^{-2}$ spectrum in the energy range $2.0 \times 10^{6}$ $-$ $6.3 \times 10^{9}$ GeV to a level of $E^2 \phi \leq 3.6 \times 10^{-8}$ ${\rm GeV cm^{-2} sec^{-1}sr^{-1}}$.

Nuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaFluxFOS: Physical sciencesCosmic rayRaysAstrophysicsParticle detectorHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Spectrumddc:530Instrumentation and Methods for Astrophysics (astro-ph.IM)PhysicsSPECTRUMCOSMIC cancer databaseRAYS004Massless particleNeutrino detectorPhysics and AstronomyNeutrinoAstrophysics - Instrumentation and Methods for Astrophysicsinfo:eu-repo/classification/ddc/004Astrophysics - Cosmology and Nongalactic AstrophysicsLepton
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