Search results for "Nuclear physic"

showing 10 items of 5307 documents

Search for a Charged Higgs Boson Produced in the Vector-Boson Fusion Mode with DecayH±→W±ZusingppCollisions ats=8  TeVwith the ATLAS Experiment

2015

A search for a charged Higgs boson, H-+/-, decaying to a W-+/- boson and a Z boson is presented. The search is based on 20.3 fb(-1) of proton-proton collision data at a center-of-mass energy of 8 TeV recorded with the ATLAS detector at the LHC. The H-+/- boson is assumed to be produced via vector-boson fusion and the decays W-+/- -> q (q') over bar and Z -> e(+)e(-)/mu(+)mu(-) are considered. The search is performed in a range of charged Higgs boson masses from 200 to 1000 GeV. No evidence for the production of an H+ boson is observed. Upper limits of 31-1020 fb at 95% C.L. are placed on the cross section for vector-boson fusion production of an H-+/- boson times its branching fraction to W…

Condensed Matter::Quantum GasesPhysicsParticle physicsLarge Hadron ColliderBranching fractionHigh Energy Physics::PhenomenologyATLAS experimentGeneral Physics and AstronomyElementary particle7. Clean energyVector bosonNuclear physicsHiggs bosonHigh Energy Physics::ExperimentBosonDimensionless quantityPhysical Review Letters
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Electron-cooled accumulation of 4 × 109positrons for production and storage of antihydrogen atoms

2016

Four billion positrons (e+) are accumulated in a Penning–Ioffe trap apparatus at 1.2 K and <6 × 10−17 Torr. This is the largest number of positrons ever held in a Penning trap. The e+ are cooled by collisions with trapped electrons (e−) in this first demonstration of using e− for efficient loading of e+ into a Penning trap. The combined low temperature and vacuum pressure provide an environment suitable for antihydrogen () production, and long antimatter storage times, sufficient for high-precision tests of antimatter gravity and of CPT.

Condensed Matter::Quantum GasesPhysicsPhysics::General PhysicsAntiparticleAnnihilationPlasmaElectronCondensed Matter PhysicsPenning trap01 natural sciencesAtomic and Molecular Physics and Optics010305 fluids & plasmasNuclear physicsTorrAntimatter0103 physical sciencesPhysics::Atomic and Molecular ClustersPhysics::Atomic PhysicsAtomic physics010306 general physicsAntihydrogenJournal of Physics B: Atomic, Molecular and Optical Physics
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Search for a multi-Higgs-boson cascade inW+W−bb¯events with the ATLAS detector inppcollisions ats=8  TeV

2014

A search is presented for new particles in an extension to the Standard Model that includes a heavy Higgs boson (H-0), an intermediate charged Higgs-boson pair (H-+/-), and a light Higgs boson (h(0)). The analysis searches for events involving the production of a single heavy neutral Higgs boson which decays to the charged Higgs boson and a W boson, where the charged Higgs boson subsequently decays into a W boson and the lightest neutral Higgs boson decaying to a bottom-antibottom-quark pair. Such a cascade results in a W-boson pair and a bottom-antibottom-quark pair in the final state. Events with exactly one lepton, missing transverse momentum, and at least four jets are selected from a d…

Condensed Matter::Quantum GasesQuarkPhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderBranching fractionHigh Energy Physics::PhenomenologySupersymmetry7. Clean energyCharged particleNuclear physicsPair productionHiggs bosonHigh Energy Physics::ExperimentLeptonPhysical Review D
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Mass Measurements of Proton-rich Nuclei with JYFLTRAP

2011

The Penning trap setup JYFLTRAP, connected to the IGISOL facility, has been extensively used for atomic mass measurements of exotic nuclei. On the proton rich side of the chart of nuclei mass measurements have mostly contributed to fundamental physics and nuclear astrophysics studies with about 100 atomic masses measured. peerReviewed

Condensed Matter::Quantum Gasesnuclear spectroscopyydinrakennenuclear physicsaccelerator-based physicsNuclear Theorynuclear structurePhysics::Atomic and Molecular ClustersydinspektroskopiaPhysics::Atomic PhysicsNuclear Experimentydinfysiikkakiihdytinpohjainen fysiikka
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Chiral approach to antikaon s- and p-wave interactions in dense nuclear matter

2006

The properties of the antikaons in nuclear matter are investigated from a chiral unitary approach which incorporates the s- and p-waves of the ${\bar K}N$ interaction. To obtain the in-medium meson-baryon amplitudes we include, in a self-consistent way, Pauli blocking effects, meson self-energies corrected by nuclear short-range correlations and baryon binding potentials. We pay special attention to investigating the validity of the on-shell factorization, showing that it cannot be applied in the evaluation of the in-medium corrections to the p-wave amplitudes. In nuclear matter at saturation energy, the $\Lambda$ and $\Sigma$ develop an attractive potential of about -30 MeV, while the $\Si…

Constitució de la matèriaNuclear TheoryNuclear TheoryFOS: Physical sciencesFísicaNuclear Theory (nucl-th)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Collisions (Nuclear physics)Col·lisions (Física nuclear)AntikaonsConstitution of matterNuclear ExperimentPropietats de la matèriaProperties of matter
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Unitarity constraint for threshold coherent pion photoproduction on the deuteron

1997

The contribution of the two-step process {gamma}d{r_arrow}pn{r_arrow}{pi}{sup 0}d to the imaginary part of the amplitude for coherent pion production on the deuteron is calculated at threshold exploiting unitarity constraints. The result shows that this absorptive process is not negligible and has to be considered in an extraction of the elementary neutron production amplitude from the {gamma}d{r_arrow}{pi}{sup 0}d cross section at threshold. {copyright} {ital 1997} {ital The American Physical Society}

Constraint (information theory)Nuclear physicsPhysicsNuclear and High Energy PhysicsParticle physicsPionAmplitudeDeuteriumUnitarityNeutronProduction (computer science)Few-body systemsPhysical Review C
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Mixed MHD convection and Tritium transport in fusion-relevant configurations

2005

Mixed MHD flow and Tritium transport were computed for a slender poloidal duct, representative of a DEMO HCLL blanket element. 2-D flow and temperature fields were computed in the duct's cross section under the assumption of parallel, fully developed flow, while Tritium concentration C was found by solving a fully 3-D problem with simplifying assumptions at the duct's ends. The spatial distribution of C depended on the intensity and direction of the forced flow. Significant peak factors were obtained if the net flow rate was so low that re-circulation occurred; C maxima were attained near the walls for upward flow, in the core region for downward flow.

ConvectionPhysicsMechanical EngineeringHCLL blanketMechanicsBlanketFusion powerMagnetohydrodynamicVolumetric flow ratePhysics::Fluid DynamicsNuclear physicsNuclear Energy and EngineeringCombined forced and natural convectionFlow conditioningGeneral Materials ScienceDuct (flow)Mixed convectionMagnetohydrodynamicsSettore ING-IND/19 - Impianti NucleariCivil and Structural Engineering
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Characteristics of the diffuse astrophysical electron and Tau neutrino flux with six years of IceCube high energy cascade data

2020

We report on the first measurement of the astrophysical neutrino flux using particle showers (cascades) in IceCube data from 2010-2015. Assuming standard oscillations, the astrophysical neutrinos in this dedicated cascade sample are dominated (∼90%) by electron and tau flavors. The flux, observed in the sensitive energy range from 16 TeV to 2.6 PeV, is consistent with a single power-law model as expected from Fermi-type acceleration of high energy particles at astrophysical sources. We find the flux spectral index to be γ=2.53±0.07 and a flux normalization for each neutrino flavor of φastro=1.66-0.27+0.25 at E0=100 TeV, in agreement with IceCube's complementary muon neutrino results and wit…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Physics and AstronomyElectronpower spectrumflux [electron]energy [particle]01 natural sciencesIceCubeNuclear physics5/3Tau neutrinomuon0103 physical scienceslow [energy]Muon neutrinoddc:530010303 astronomy & astrophysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSPECTRUMSpectral indexMuon010308 nuclear & particles physicsHigh Energy Physics::Phenomenologyflavor [neutrino]RAYSflux [neutrino]accelerationshowersoscillationPhysics and Astronomy13. Climate actionEnergy cascadePhysique des particules élémentairesastro-ph.COhigh [energy]cascade [energy]High Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaFermi Gamma-ray Space TelescopeAstrophysics - Cosmology and Nongalactic Astrophysics
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A search for light dark matter in XENON10 data

2011

We report results of a search for light (3.5x10^{-42} cm^2, for a dark matter particle mass m_{\chi}=8 GeV. We find that our data strongly constrain recent elastic dark matter interpretations of excess low-energy events observed by CoGeNT and CRESST-II, as well as the DAMA annual modulation signal.

Cosmology and Nongalactic Astrophysics (astro-ph.CO)LightDark matterGeneral Physics and AstronomyFOS: Physical sciencesElectronsElementary particleElectron01 natural sciencesParticle detectorHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesHumansScattering Radiation010306 general physicsLight dark matterNuclear PhysicsPhysicsPhotons010308 nuclear & particles physicsScatteringFermionBaryonHigh Energy Physics - PhenomenologyData Interpretation StatisticalCosmic RadiationAstrophysics - Cosmology and Nongalactic Astrophysics
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Dark matter results from 225 live days of XENON100 data

2012

We report on a search for particle dark matter with the XENON100 experiment, operated at the Laboratori Nazionali del Gran Sasso (LNGS) for 13 months during 2011 and 2012. XENON100 features an ultra-low electromagnetic background of (5.3 \pm 0.6) \times 10^-3 events (kg day keVee)^-1 in the energy region of interest. A blind analysis of 224.6 live days \times 34 kg exposure has yielded no evidence for dark matter interactions. The two candidate events observed in the pre-defined nuclear recoil energy range of 6.6-30.5 keVnr are consistent with the background expectation of (1.0 \pm 0.2) events. A Profile Likelihood analysis using a 6.6-43.3 keVnr energy range sets the most stringent limit o…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Physics - Instrumentation and DetectorsLarge Underground Xenon experimentDark matterFOS: Physical sciencesGeneral Physics and AstronomyWIMP Argon Programme01 natural sciences7. Clean energyParticle detectorHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)WIMP0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsLiquid XenonPhysicsRange (particle radiation)010308 nuclear & particles physicsDARK MATTERInstrumentation and Detectors (physics.ins-det)High Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]DAMA/NaITPCPandaXDirect search for Dark MatterAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review Letters
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