Search results for "Masse"

showing 10 items of 219 documents

Neutrino cosmology and Planck

2014

Relic neutrinos play an important role in the evolution of the Universe, modifying some of the cosmological observables. We summarize the main aspects of cosmological neutrinos and describe how the precision of present cosmological data can be used to learn about neutrino properties. In particular, we discuss how cosmology provides information on the absolute scale of neutrino masses, complementary to beta decay and neutrinoless double-beta decay experiments. We explain why the combination of Planck temperature data with measurements of the baryon acoustic oscillation angular scale provides a strong bound on the sum of neutrino masses, 0.23 eV at the 95% confidence level, while the lensing …

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)General Physics and AstronomyFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsCosmologydark matterHigh Energy Physics - Experimentsymbols.namesakeHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)PlanckAbsolute scaleParticle Physics - PhenomenologyPhysicsOscillationneutrino massesHigh Energy Physics::PhenomenologyFísicaObservablePlanck temperatureBaryonHigh Energy Physics - Phenomenology13. Climate action[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]symbolsHigh Energy Physics::ExperimentNeutrinocosmologyAstrophysics - Cosmology and Nongalactic Astrophysics
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How to relax the cosmological neutrino mass bound

2019

We study the impact of non-standard momentum distributions of cosmic neutrinos on the anisotropy spectrum of the cosmic microwave background and the matter power spectrum of the large scale structure. We show that the neutrino distribution has almost no unique observable imprint, as it is almost entirely degenerate with the effective number of neutrino flavours, $N_{\mathrm{eff}}$, and the neutrino mass, $m_{\nu}$. Performing a Markov chain Monte Carlo analysis with current cosmological data, we demonstrate that the neutrino mass bound heavily depends on the assumed momentum distribution of relic neutrinos. The message of this work is simple and has to our knowledge not been pointed out cle…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)cosmological neutrinosPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaCosmic microwave backgroundFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicscosmological parameters from LSS01 natural sciencesCosmologyMomentumsymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)cosmological0103 physical sciencesPhysicsCOSMIC cancer database010308 nuclear & particles physicsMatter power spectrumHigh Energy Physics::Phenomenologycosmological parameters from CMBRAstronomy and AstrophysicsObservableMarkov chain Monte Carloneutrino masses from cosmologyHigh Energy Physics - Phenomenologyparameters from CMBRsymbolsHigh Energy Physics::ExperimentNeutrinoAstrophysics - Cosmology and Nongalactic Astrophysics
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The seesaw path to leptonic CP violation

2016

Future experiments such as SHiP and high-intensity $e^+ e^-$ colliders will have a superb sensitivity to heavy Majorana neutrinos with masses below $M_Z$. We show that the measurement of the mixing to electrons and muons of one such state could imply the discovery of leptonic CP violation in the context of seesaw models. We quantify in the minimal model the CP discovery potential of these future experiments, and demonstrate that a 5$\sigma$ CL discovery of leptonic CP violation would be possible in a very significant fraction of parameter space.

Particle physicsHeavy NeutrinoPhysics and Astronomy (miscellaneous)FOS: Physical sciencesSeesaw Modellcsh:AstrophysicsContext (language use)Parameter space01 natural sciencesMinimal modelHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometrySterile Neutrinolcsh:QB460-4660103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsEngineering (miscellaneous)Particle Physics - PhenomenologyHeavy StatePhysicsMuon010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyLight Neutrino Massehep-phHigh Energy Physics - PhenomenologyMAJORANAlcsh:QC770-798CP violationHigh Energy Physics::ExperimentNeutrino
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Study of Beauty Hadron Decays into Pairs of Charm Hadrons

2014

First observations of the decays Λ[0 over b] → Λ[+ over c]D[− over (s)] are reported using data corresponding to an integrated luminosity of 3  fb[superscript −1] collected at 7 and 8 TeV center-of-mass energies in proton-proton collisions with the LHCb detector. In addition, the most precise measurement of the branching fraction B(B[0 over s] → D[superscript +]D[− over s]) is made and a search is performed for the decays B[0 over (s)] → Λ[+ over c]Λ[− over c]. The results obtained are B(Λ[0 over b] → Λ[+ over c]D[superscript −])/B(Λ[0 over b] → Λ[+ over c]D[− over s]) = 0.042 ± 0.003(stat) ± 0.003(syst), ⎡⎣B(Λ[0 over b] → Λ[+ over c]D[− over s]) over B([¯ over B[superscript 0] → D[superscr…

Particle physicsMesonHadronNuclear TheoryGeneral Physics and AstronomyFOS: Physical sciencesLHCb - Abteilung Hofmann13.30.-aSettore FIS/04 - Fisica Nucleare e SubnucleareHigh Energy Physics - ExperimentNuclear physicsPhysics and Astronomy (all)High Energy Physics - Experiment (hep-ex)precise measurements14.20.Mr[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]TOOLCharm (quantum number)MASSESNuclear ExperimentQCBARYONSPhysicsLuminosity (scattering theory)Branching fractioncenter-of-mass energiesintegrated luminositybaryons; masses; toolParticle physicsBaryonproton proton collisionsLHCbprecise measurements; center-of-mass energies; tellurium compounds; integrated luminosity; hadrons; branching fractions; proton proton collisionshadronsDecays of baryonbranching fractionsBottom baryons (|B|>0)Física nuclearHigh Energy Physics::ExperimentLHCFísica de partículesExperimentstellurium compoundsTellurium compoundsParticle Physics - Experiment
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Neutrino oscillations and Non-Standard Interactions

2017

Current neutrino experiments measure the neutrino mixing parameters with an unprecedented accuracy. The upcoming generation of experiments will be sensitive to subdominant effects that can give information on the unknown neutrino parameters: the Dirac CP-violating phase, the mass ordering and the $\theta_{23}$ octant. Determining the exact values of neutrino mass and mixing parameters is crucial to test neutrino models and flavor symmetries. In the first part of this review, we summarize the current status of neutrino oscillation parameters. We consider the most recent data from solar experiments and the atmospheric data from Super-Kamiokande, IceCube and ANTARES. We implement the data from…

Particle physicsPhysics::Instrumentation and DetectorsMaterials Science (miscellaneous)Physics beyond the Standard ModelAstrophysics::High Energy Astrophysical PhenomenaBiophysicsGeneral Physics and AstronomyFOS: Physical sciencesCHOOZ7. Clean energy01 natural sciencesPartícules (Física nuclear)High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Violació CP (Física nuclear)neutrino physics0103 physical sciencesPhysical and Theoretical Chemistry010306 general physicsNeutrino oscillationMathematical PhysicsPhysicsGauge bosonneutrino oscillationsnon-standard neutrino interactions010308 nuclear & particles physicsneutrino massesElectroweak interactionHigh Energy Physics::Phenomenologylcsh:QC1-999leptonic CP violationHigh Energy Physics - PhenomenologyNeutrino detector13. Climate actionMINOSHigh Energy Physics::ExperimentNeutrinolcsh:Physics
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Patrimonio architettonico diffuso: le masserie delle Madonie come esempio di una "archeologia preindustriale"

2018

Patrimonio masserie archeologia preindustrialeSettore ICAR/10 - Architettura Tecnica
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The decay energy of the pure s-process nuclide ¹²³ Te

2016

Physics letters / B 758, 407 - 411 (2016). doi:10.1016/j.physletb.2016.04.059

Penning-trap mass spectrometryPhysicsNuclear and High Energy Physics010308 nuclear & particles physicsElectron captureAtomic massesIonic bondingAstrophysicsMass spectrometry53001 natural scienceslcsh:QC1-999Atomic massNuclear physicsMassDecay energyTheoryofComputation_ANALYSISOFALGORITHMSANDPROBLEMCOMPLEXITY0103 physical sciencesddc:530NuclidePräzisionsexperimente - Abteilung BlaumAtomic physics010306 general physicss-processlcsh:Physics
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High-Precision Proton-Capture Q Values for 25Al(p,γ)26Si and 30P(p,γ)31Si

2017

The masses of astrophysically relevant nuclei, 25Al and 30P, have recently been measured with the JYFLTRAP double Penning trap at the new IGISOL-4 facility at the University of Jyväskylä. Unparalleled precisions of 63 and 64 eV were achieved for the 25Al and 30P masses, respectively. The proton-capture Q values for 25Al(p, γ)26Si and 30P(p, γ)31S were also determined, and their precisions improved by a factor of 4 and 2, respectively, in comparison with AME12. The impact of the more precise values on the resonant proton-capture rate has also been studied. peerReviewed

Penning-trap mass spectrometryatomic massesnovat
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Mass Measurements for the rp Process

2017

One of the key parameters for the reaction network calculations for the rapid proton capture (rp) process, occurring e.g., in type I X-ray bursts, are the masses of the involved nuclei. Nowadays, masses of even rather exotic nuclei can be measured very precisely employing Penning-trap mass spectrometry. With the JYFLTRAP Penning trap at the IGISOL facility, masses of around 100 neutron-deficient nuclei have been determined with a typical precision of a few keV. Most recently, 25Al, 30P, 31Cl, and 52Co have been measured. Of these, the precision of the mass-excess value of 31Cl was improved from 50 to 3.4 keV, and the mass of 52Co was experimentally determined for the first time. The mass of…

Penning-trap mass spectrometrynovae rp processatomic masses
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Mass Measurements for the rp Process

2017

Penning-trap mass spectrometrynovaePhysicsatomic massesChromatographyta114010308 nuclear & particles physicsrp process0103 physical sciencesrp-process010306 general physics01 natural sciencesProceedings of the 14th International Symposium on Nuclei in the Cosmos (NIC2016)
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