Search results for "Neutrino ma"

showing 10 items of 55 documents

Non-linear evolution of the cosmic neutrino background

2012

We investigate the non-linear evolution of the relic cosmic neutrino background by running large box-size, high resolution N-body simulations which incorporate cold dark matter (CDM) and neutrinos as independent particle species. Our set of simulations explore the properties of neutrinos in a reference Lambda CDM model with total neutrino masses between 0.05-0.60 eV in cold dark matter haloes of mass 10(11) – 10(15) h(-1) M-circle dot, over a redshift range z = 0 – 2. We compute the halo mass function and show that it is reasonably well fitted by the Sheth-Tormen formula, once the neutrino contribution to the total matter is removed. More importantly, we focus on the CDM and neutrino proper…

AstrofísicaCosmology and Nongalactic Astrophysics (astro-ph.CO)Cold dark mattercosmological neutrinosFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics7. Clean energy01 natural sciencesMomentumSettore FIS/05 - Astronomia e Astrofisica0103 physical sciencesPeculiar velocity010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysicsneutrino propertiesPhysicsCosmologia010308 nuclear & particles physicsHalo mass functionAstronomy and Astrophysicsneutrino masses from cosmologyRedshiftCosmic neutrino background13. Climate actionHigh Energy Physics::ExperimentHaloNeutrinoAstrophysics - Cosmology and Nongalactic Astrophysics
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Discovery potential of xenon-based neutrinoless double beta decay experiments in light of small angular scale CMB observations

2013

The South Pole Telescope (SPT) has probed an expanded angular range of the CMB temperature power spectrum. Their recent analysis of the latest cosmological data prefers nonzero neutrino masses, with Sigma m(nu) = (0.32 +/- 0.11) eV. This result, if con firmed by the upcoming Planck data, has deep implications on the discovery of the nature of neutrinos. In particular, the values of the effective neutrino mass m(beta beta) involved in neutrinoless double beta decay (beta beta 0 nu) are severely constrained for both the direct and inverse hierarchy, making a discovery much more likely. In this paper, we focus in xenon-based beta beta 0 nu experiments, on the double grounds of their good perfo…

AstrofísicaPhysics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsCosmic microwave backgroundchemistry.chemical_elementdouble beta decayFOS: Physical sciences7. Clean energy01 natural sciencesPartícules (Física nuclear)High Energy Physics - ExperimentNuclear physicssymbols.namesakeHigh Energy Physics - Experiment (hep-ex)XenonHigh Energy Physics - Phenomenology (hep-ph)Double beta decay0103 physical sciencesPlanck010306 general physicsPhysicsCosmologiaTime projection chamber010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and Astrophysicsneutrino masses from cosmologyInstrumentation and Detectors (physics.ins-det)3. Good healthHigh Energy Physics - PhenomenologyMAJORANASouth Pole Telescopechemistry13. Climate actionsymbolsNeutrino
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(Standard model) universe dominated by the right matter

2009

14 pages, 3 figures. References on late time enthropy release included, several points clarified. PACS numbers: 14.60.Pq, 98.80.Cq. ArXiv pre-print available at http://arxiv.org/abs/0806.4389

AstrofísicaPhysicsNuclear and High Energy PhysicsParticle physicsGrand-Unified-TheoryDark-MatterHigh Energy Physics::PhenomenologyElectroweak interactionDark matterBaryogenesisFísicaAstrophysics::Cosmology and Extragalactic AstrophysicsTime Entropy ProductionBaryogenesisBaryon asymmetryDecaying ParticlesConstraintsHigh Energy Physics::ExperimentGravitinoNeutrinoNeutrino MassNeutrino oscillationPhenomenology (particle physics)Inflationary UniversePhysical Review D
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Electroweak baryogenesis from a dark sector

2017

Adding an extra singlet scalar $S$ to the Higgs sector can provide a barrier at tree level between a false vacuum with restored electroweak symmetry and the true one. This has been demonstrated to readily give a strong phase transition as required for electroweak baryogenesis. We show that with the addition of a fermionic dark matter particle $\chi$ coupling to $S$, a simple UV-complete model can realize successful electroweak baryogenesis. The dark matter gets a CP asymmetry that is transferred to the standard model through a $CP\ portal\ interaction$, which we take to be a coupling of $\chi$ to $\tau$ leptons and an inert Higgs doublet. The CP asymmetry induced in left-handed $\tau$ lepto…

Astrophysics and AstronomyParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)standard model of particle physicsPhysics beyond the Standard ModelSTANDARD MODELFOS: Physical sciences01 natural sciences7. Clean energy114 Physical sciencesdark matterHiggs sectorStandard Modelpimeä aineHigh Energy Physics - Phenomenology (hep-ph)Baryon asymmetry0103 physical sciencesSINGLET010306 general physicsParticle Physics - PhenomenologyPhysicsta114010308 nuclear & particles physicsElectroweak interactionHigh Energy Physics::Phenomenologyhiukkasfysiikan standardimalliRADIATIVE NEUTRINO MASShep-phSphaleronBaryogenesisHigh Energy Physics - Phenomenologyastro-ph.COHiggs bosonPHASE-TRANSITIONHigh Energy Physics::ExperimentMATTERAstrophysics - Cosmology and Nongalactic Astrophysics
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High magnetic fields for fundamental physics

2018

Various fundamental-physics experiments such as measurement of the birefringence of the vacuum, searches for ultralight dark matter (e.g., axions), and precision spectroscopy of complex systems (including exotic atoms containing antimatter constituents) are enabled by high-field magnets. We give an overview of current and future experiments and discuss the state-of-the-art DC- and pulsed-magnet technologies and prospects for future developments.

Astrophysics and AstronomyPhysics - Instrumentation and Detectorsmagnet: designmagnetic field: highAtomic Physics (physics.atom-ph)AxionsDark matterComplex systemOther Fields of PhysicsFOS: Physical sciencesGeneral Physics and Astronomy01 natural sciencesphysics.atom-phNOPhysics - Atomic PhysicsNuclear physicsPhysics and Astronomy (all)Neutrino mass0103 physical sciencesDark matter[ PHYS.PHYS.PHYS-GEN-PH ] Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]Axions; Dark matter; High-field magnets; Neutrino mass; Spectroscopy; Vacuum birefringence; Physics and Astronomy (all)[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Detectors and Experimental Techniques010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Axionphysics.ins-detSpectroscopyactivity reportExotic atomPhysicsVacuum birefringence010308 nuclear & particles physicsInstrumentation and Detectors (physics.ins-det)Polarization (waves)magnet: technology[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]3. Good healthMagnetic fieldHigh-field magnetsAntimatterMagnetAstrophysics - Instrumentation and Methods for Astrophysicsastro-ph.IM
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Production, isolation and characterization of radiochemically pure 163Ho samples for the ECHo-project

2018

Abstract Several experiments on the study of the electron neutrino mass are based on high-statistics measurements of the energy spectrum following electron capture of the radionuclide 163Ho. They rely on the availability of large, radiochemically pure samples of 163Ho. Here, we describe the production, separation, characterization, and sample production within the Electron Capture in Holmium-163 (ECHo) project. 163Ho has been produced by thermal neutron activation of enriched, prepurified 162Er targets in the high flux reactor of the Institut Laue-Langevin, Grenoble, France, in irradiations lasting up to 54 days. Irradiated targets were chemically processed by means of extraction chromatogr…

ChromatographyChemistryEcho (computing)lanthanide separationneutron activation[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]010403 inorganic & nuclear chemistryIsolation (microbiology)7. Clean energy01 natural sciencesNeutrino mass determination0104 chemical sciencesCharacterization (materials science)163Ho0103 physical sciencesextraction chromatographyPhysical and Theoretical Chemistry010306 general physicsNeutron activationRadiochimica Acta
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Decoherence in supernova neutrino transformations suppressed by deleptonization

2007

16 pages, 12 figures.-- PACS nrs.: 14.60.Pq; 97.60.Bw.-- ISI Article Identifier: 000251987300100.-- ArXiv pre-print available at: http://arxiv.org/abs/0706.2498

HistoryParticle physicsNuclear and High Energy PhysicsQuantum decoherence[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Physics::Instrumentation and Detectorsmedia_common.quotation_subjectHigh Energy Physics::LatticeAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences[PACS] Supernovae[PACS] Neutrino mass and mixingAstrophysicsAsymmetryMeasure (mathematics)01 natural sciences7. Clean energyEarly UniverseStandard ModelEducationLuminosity[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesInvariant massddc:530High Energy Physics010306 general physicsMixing (physics)media_commonPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsAstrophysics (astro-ph)High Energy Physics::PhenomenologyFísicaWeinberg angleFunction (mathematics)Atomic and Molecular Physics and OpticsComputer Science Applications3. Good healthSupernovaHigh Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]PhenomenologyHigh Energy Physics::ExperimentNeutrino
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Supersymmetric SO(10)-inspired GUTs with sliding scales

2013

We construct lists of supersymmetric models with extended gauge groups at intermediate steps, all of which are inspired by SO(10) unification. We consider three different kinds of setups: (i) the model has exactly one additional intermediate scale with a left-right (LR) symmetric group; (ii) SO(10) is broken to the LR group via an intermediate Pati-Salam scale; and (iii) the LR group is broken into SU(3)(c) X SU(2)(L) X U(1)(R) X U(1)(B-L), before breaking to the standard model (SM) group. We use sets of conditions, which we call the "sliding mechanism," which yield unification with the extended gauge group(s) allowed at arbitrary intermediate energy scales. All models thus can have new gau…

Left-right symmetryNeutrino massModelsUnificationHigh Energy Physics::PhenomenologyGrand unified theoryNumberFísicaHiggs-bosonR-ParityBreakingLeptons
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Neutrino transition magnetic moments within the non-standard neutrino-nucleus interactions

2015

Tensorial non-standard neutrino interactions are studied through a combined analysis of nuclear structure calculations and a sensitivity $\chi^2$-type of neutrino events expected to be measured at the COHERENT experiment, recently planned to operate at the Spallation Neutron Source (Oak Ridge). Potential sizeable predictions on transition neutrino magnetic moments and other electromagnetic parameters, such as neutrino milli-charges, are also addressed. The non-standard neutrino-nucleus processes, explored from nuclear physics perspectives within the context of quasi-particle random phase approximation, are exploited in order to estimate the expected number of events originating from vector …

Neutrino magnetic moment and interactionsParticle physicsNuclear and High Energy PhysicsReactor neutrinosPhysics::Instrumentation and DetectorsPhysics beyond the Standard ModelAstrophysics::High Energy Astrophysical PhenomenaSpallation neutron source neutrinosFOS: Physical sciencesContext (language use)Nuclear physicsHigh Energy Physics - Phenomenology (hep-ph)Quasi-particle random phase approximationNon-standard electroweak interactionsNeutrino oscillationPhysicsHigh Energy Physics::PhenomenologyNuclear structureSolar neutrino problemlcsh:QC1-999Lepton flavour violationHigh Energy Physics - PhenomenologyNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinolcsh:Physics
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Theory of Neutrinos: A White Paper

2005

During 2004, four divisions of the American Physical Society commissioned a study of neutrino physics to take stock of where the field is at the moment and where it is going in the near and far future. Several working groups looked at various aspects of this vast field. The summary was published as a main report entitled ``The Neutrino Matrix'' accompanied by short 50 page versions of the report of each working group. Theoretical research in this field has been quite extensive and touches many areas and the short 50 page report provided only a brief summary and overview of few of the important points. The theory discussion group felt that it may be of value to the community to publish the e…

Neutrino mass physics; Matter-antimatter asymmetry of the UniverseParticle physicsSupersymmetric Standard ModelPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaElectric-dipole momentsPhysics beyond the Standard ModelFOS: Physical sciencesGeneral Physics and AstronomyTheoretical researchHigh Energy Physics - Phenomenology (hep-ph)White paperSee-saw mechanismneutriniPublicationParticle Physics - PhenomenologyPhysicsLepton-flavor violationDiscussion groupbusiness.industryHigh Energy Physics::PhenomenologyFísicaMatter-antimatter asymmetry of the UniverseDouble beta decaySettore FIS/02 - Fisica Teorica Modelli e Metodi MatematiciEpistemologyElectroweak symmetry-breakingHigh Energy Physics - PhenomenologyLarge extra dimensionsNeutrino mass physicsHeavy Majorana neutrinosHigh Energy Physics::ExperimentRight-handed neutrinoNeutrinoAnomalous magnetic momentWorking groupbusiness
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