Search results for "mass [leptoquark]"

showing 10 items of 519 documents

Mass Measurements and Implications for the Energy of the High-Spin Isomer inAg94

2008

Nuclides in the vicinity of {sup 94}Ag have been studied with the Penning trap mass spectrometer JYFLTRAP at the Ion-Guide Isotope Separator On-Line. The masses of the two-proton-decay daughter {sup 92}Rh and the beta-decay daughter {sup 94}Pd of the high-spin isomer in {sup 94}Ag have been measured, and the masses of {sup 93}Pd and {sup 94}Ag have been deduced. When combined with the data from the one-proton- or two-proton-decay experiments, the results lead to contradictory mass excess values for the high-spin isomer in {sup 94}Ag, -46 370(170) or -44 970(100) keV, corresponding to excitation energies of 6960(400) or 8360(370) keV, respectively.

PhysicsNuclear physicsMass excessIsotopeAnalytical chemistryGeneral Physics and AstronomyNuclideSpin (physics)Penning trapMass spectrometryBeta decayExcitationPhysical Review Letters
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Mass ofAl23for testing the isobaric multiplet mass equation

2009

The mass excess of the proton-rich nucleus $^{23}\mathrm{Al}$ has been measured with the JYFLTRAP Penning trap setup. As a result of our experiment we obtain a mass excess of 6748.07(34) keV, and by combining the value to existing experimental data we have tested the validity of the isobaric multiplet mass equation $(\mathrm{IMME})$ for the $T=3/2$ quartet in the $A=23$ isobar. The fit to the IMME results in a vanishing cubic term equivalent to zero with high precision [$0.22(42)$ keV].

PhysicsNuclear physicsMass formulaNuclear and High Energy PhysicsMass excessNuclear TheoryZero (complex analysis)IsobarIsobaric processAtomic physicsNuclear ExperimentPenning trapMultipletPhysical Review C
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Searching for the 5H resonance in the t+n+n system

2003

19 pages, 7 figures, 2 tables, 2 appendices.-- PACS nrs.: 27.10.+h; 25.60.Gc.-- Printed version published Jul 28, 2003.

PhysicsNuclear reactionNuclear and High Energy PhysicsComparisons with previous resultsMeasured triton and neutron relative energy spectra energy and angular correlationsHyperspherical harmonic expansion analysisResonance[PACS] Properties of specific nuclei listed by mass ranges: A ≤ 5Nuclear Reactions C(6Hent) (6He2nt) E=240 MeV/nucleonNuclear physicsNuclear magnetic resonanceA ≤ 5 [[PACS] Properties of specific nuclei listed by mass ranges]45H deduced resonance features[PACS] Breakup and momentum distributionsNuclear Physics A
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Mass and low-lying levels ofIn106,108from theCd106,108(p,nγ)reactions

1984

106In has been studied via the reaction 106Cd(p,nγ)106In in the energy range Ep=7-9 MeV. Inbeam γ-ray excitation functions, γ-γ coincidence measurements, and β+-delayed γ-ray excitation functions have been used to identify thirteen levels in 106In. From this new level scheme the energy separation of the high-spin ground state and the low-spin isomer has been determined to be 28.6±0.5 keV. The threshold energy of the strongest low-lying γ-ray transition yields a mass excess for 106In of -80601±15 keV. Spins for some states are suggested by comparing the excitation functions to Hauser-Feshbach calculations. In-beam γ-ray excitation functions for the 108Cd(p,nγ)108In reaction give a mass exces…

PhysicsNuclear reactionNuclear and High Energy PhysicsRange (particle radiation)Mass excessSpinsIsotopeAstrophysics::High Energy Astrophysical PhenomenaAtomic physicsGround stateThreshold energyExcitationPhysical Review C
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Non-standard interactions: Atmospheric versus neutrino factory experiments

2001

We consider the potential of a generic neutrino factory (NUFACT) in probing non-standard neutrino-matter interactions (NSI). We find that the sensitivity to flavour-changing (FC) NSI can be substantially improved with respect to present atmospheric neutrino data, especially at energies higher than approximately 50 GeV, where the effect of the tau mass is small. For example, a 100 GeV NUFACT can probe FC neutrino interactions at the level of few $|\epsilon| < {few} \times 10^{-4}$ at 99 % C.L.

PhysicsParticle physicsAtmospheric neutrinosNuclear and High Energy PhysicsNeutrino mass and mixingNeutrino oscillationsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyNeutrino factoryFOS: Physical sciencesFísicaHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Neutrino FactoryHigh Energy Physics::ExperimentSensitivity (control systems)Atmospheric neutrinoNeutrino
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A non-resonant dark-side solution to the solar neutrino problem

2001

We re-analyse spin-flavour precession solutions to the solar neutrino problem in the light of the recent SNO CC result as well as the 1258--day Super-Kamiokande data and the upper limit on solar anti-neutrinos. In a self-consistent magneto-hydrodynamics approach the resulting scheme has only 3 effective parameters: $\Delta m^2$, $\mu B_\perp$ and the neutrino mixing angle $\theta$. We show how a rates-only analysis for fixed $\mu B_\perp$ slightly favours spin-flavour precession (SFP) solutions over oscillations (OSC). In addition to the resonant solution (RSFP for short), there is a new non-resonant solution (NRSFP) in the ``dark-side''. Both RSFP and NRSFP lead to flat recoil energy spect…

PhysicsParticle physicsNuclear and High Energy PhysicsNeutrino mass and mixingCosmologiaMagnetic momentNeutrino oscillationsSolar neutrinosHigh Energy Physics::PhenomenologyFOS: Physical sciencesSolar neutrino problemSpectral linePartícules (Física nuclear)Magnetic fieldBohr magnetonNeutrino magnetic momentsymbols.namesakeHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)symbolsPrecessionHigh Energy Physics::ExperimentNeutrinoMixing (physics)
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Transfer coefficients for evaporation of a system with a Lennard-Jones long-range spline potential

2007

International audience; Surface transfer coefficients are determined by nonequilibrium molecular dynamics simulations for a Lennard-Jones fluid with a long-range spline potential. In earlier work A. Røsjorde et al., J. Colloid Interface Sci. 240, 355 2001; J. Xu et al., ibid. 299, 452 2006, using a short-range Lennard-Jones spline potential, it was found that the resistivity coefficients to heat and mass transfer agreed rather well with the values predicted by kinetic theory. For the long-range Lennard-Jones spline potential considered in this paper we find significant discrepancies from the values predicted by kinetic theory. In particular the coupling coefficient, and as a consequence the…

PhysicsPhase transitionThermodynamics02 engineering and technologyNonequilibrium molecular dynamics021001 nanoscience & nanotechnology01 natural sciencesTheorem of corresponding states[PHYS.PHYS.PHYS-CHEM-PH] Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph][CHIM.THEO]Chemical Sciences/Theoretical and/or physical chemistry[ PHYS.PHYS.PHYS-CHEM-PH ] Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph]Spline (mathematics)Colloid[CHIM.THEO] Chemical Sciences/Theoretical and/or physical chemistryElectrical resistivity and conductivityMass transfer0103 physical sciences[ CHIM.THEO ] Chemical Sciences/Theoretical and/or physical chemistry[PHYS.PHYS.PHYS-CHEM-PH]Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph]010306 general physics0210 nano-technologyCoupling coefficient of resonatorsComputingMilieux_MISCELLANEOUS
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Binary evolution of PSR J1713+0747

2007

PSR J1713+0747 is a binary millisecond radio pulsar with a long orbital period (Porb ∼ 68 d) and a very low neutron star mass (M NS = 1.3 ± 0.2 M⊙). We simulate the evolution of this binary system with an accurate numerical code, which keeps into account both the evolution of the primary and of the whole binary system. We show that strong ejection of matter from the system is fundamental to obtain a mass at the end of the evolution that is within 1 - σ from the observed one, but propeller effects are almost negligible in such a system, where the accretion rate is always near to the Eddington limit. We show that there are indeed two mechanisms can account for the amount of mass loss from the…

PhysicsPulsars: individual: PSR J1713+0747close; Pulsars: individual: PSR J1713+0747; Relativity; Stars: neutron; X-rays: binaries [Accretion accretion discs; Binaries]X-ray binaryAstrophysicsBinary pulsarStars: neutronRelativityNeutron starsymbols.namesakeX-rays: binariesPulsarMillisecond pulsarBinaries: closeStellar mass lossEddington luminositysymbolsBinary systemAccretion accretion disc
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$a_0-f_0$ mixing in the Khuri-Treiman equations for $\eta\to 3\pi$

2015

A reliable determination of the isospin breaking double quark mass ratio from precise experimental data on $\eta\to 3\pi$ decays should be based on the chiral expansion of the amplitude supplemented with a Khuri-Treiman type dispersive treatment of the final-state interactions. We discuss an extension of this formalism which allows to estimate the effects of the $a_0(980)$ and $f_0(980)$ resonances and their mixing on the $\eta\to 3\pi$ amplitudes. Matrix generalisations of the equations describing elastic $\pi\pi$ rescattering with $I=0,\,2$ are introduced which accomodate both $\pi\pi/K\bar{K}$ and $\eta\pi/K\bar{K}$ coupled-channel rescattering. Isospin violation induced by the physical …

PhysicsQuarkParticle physicsHigh Energy Physics::PhenomenologyDalitz plotResonanceMass ratioFormalism (philosophy of mathematics)High Energy Physics - PhenomenologyAmplitude[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]IsospinPiHigh Energy Physics::ExperimentNuclear Experiment
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Meson decay studies from MAMI A2

2019

Decays of the light mesons π0, η, ω, and η’ provide a unique laboratory to test fundamental aspects of hadron physics. Precision studies of such diverse topics as the light quark mass ratio, π−π scattering lengths, and searches for physics beyond the Standard Model are possible. Additionally, Dalitz decays of light mesons provide a way of measuring the electromagnetic meson transition formfactors in the time-like region. The A2 tagged photon facility at the Mainz Microtron provides a high yield of light mesons produced by photo-induced reactions on protons, which makes the experiment ideal for high precision measurements of meson decays. Presented here are the contributions made by the A2 c…

PhysicsQuarkParticle physicsPhotonMeson010308 nuclear & particles physicsScatteringPhysicsQC1-999Physics beyond the Standard ModelHigh Energy Physics::PhenomenologyNuclear TheoryMass ratio01 natural sciencesHadron physics0103 physical sciencesHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsMicrotronEPJ Web of Conferences
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