Search results for "masses"

showing 10 items of 98 documents

Search for heavy neutral lepton production in K+ decays

2018

A search for heavy neutral lepton production in $K^+$ decays using a data sample collected with a minimum bias trigger by the NA62 experiment at CERN in 2015 is reported. Upper limits at the $10^{-7}$ to $10^{-6}$ level are established on the elements of the extended neutrino mixing matrix $|U_{\ell 4}|^2$ ($\ell=e,\mu$) for heavy neutral lepton mass in the range $170-448~{\rm MeV}/c^2$. This improves on the results from previous production searches in $K^+$ decays, setting more stringent limits and extending the mass range.

Nuclear and High Energy PhysicsleptonPontecorvo–Maki–Nakagawa–Sakata matrixheavy neutral leptons neutrino mixingFOS: Physical sciencesk mesonNA62 experiment01 natural sciencesneutrino mixingSettore FIS/04 - Fisica Nucleare e SubnuclearedecayHigh Energy Physics - ExperimentNuclear physicsneutrinoHigh Energy Physics - Experiment (hep-ex)Minimum biasEconomicaBounds; neutrinos; masses; testsTheoryofComputation_ANALYSISOFALGORITHMSANDPROBLEMCOMPLEXITY0103 physical sciencesheavy neutral leptonslepton k meson decay neutrino010306 general physicsNuclear ExperimentPhysicsRange (particle radiation)Large Hadron Collider010308 nuclear & particles physicshep-exHigh Energy Physics::PhenomenologyAmbientalelcsh:QC1-999High Energy Physics::Experimentlcsh:PhysicsParticle Physics - ExperimentLepton
researchProduct

Gamma Vel cluster membership and IMF

2016

Understanding the properties of young open clusters, such as the Initial Mass Function (IMF), star formation history and dynamic evolution, is crucial to obtain reliable theoretical predictions of the mechanisms involved in the star formation process. We want to obtain a list, as complete as possible, of confirmed members of the young open cluster Gamma Velorum, with the aim of deriving general cluster properties such as the IMF. We used all available spectroscopic membership indicators within the Gaia-ESO public archive together with literature photometry and X-ray data and, for each method, we derived the most complete list of candidate cluster members. Then, we considered photometry, gra…

Open star clustersobservational astronomyPre main sequence starsRadial velocityAstrophysics and AstronomyHertzsprung Russell diagramPhysicsexoplanet astronomyStellar massesPre-main sequence starsNatural Sciencesstellar astronomySpectroscopy
researchProduct

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
researchProduct

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
researchProduct

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
researchProduct

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
researchProduct

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
researchProduct

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
researchProduct

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
researchProduct

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)
researchProduct