Search results for "Number"

showing 10 items of 3939 documents

Observation of a Narrow Meson State Decaying toDs+π0at a Mass of2.32  GeV/c2

2003

We have observed a narrow state near 2.32 GeV/c(2) in the inclusive D(+)(s)pi(0) invariant mass distribution from e(+)e(-) annihilation data at energies near 10.6 GeV. The observed width is consistent with the experimental resolution. The small intrinsic width and the quantum numbers of the final state indicate that the decay violates isospin conservation. The state has natural spin-parity and the low mass suggests a J(P)=0(+) assignment. The data sample corresponds to an integrated luminosity of 91 fb(-1) recorded by the BABAR detector at the SLAC PEP-II asymmetric-energy e(+)e(-) storage ring.

PhysicsParticle physicsAnnihilationMeson010308 nuclear & particles physicsElectron–positron annihilationGeneral Physics and AstronomyQuantum number7. Clean energy01 natural sciencesLuminosityNuclear physicsParticle decayIsospin0103 physical sciencesHigh Energy Physics::ExperimentInvariant mass010306 general physicsPhysical Review Letters
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P̅P annihilation at rest: annihilation dynamics and meson spectroscopy

1990

Proton-antiproton annihilations provide an excellent tool to study the dynamics of quarks and gluons in the confinement region. Annihilations at rest into two mesons show selection rules which can be related to symmetries between SU(3) invariant amplitudes. In the annihilation process not only conventional (q\(\bar{\text{q}}\)) mesons are produced but also states which do not fit into the meson nonets. It is shown how knowledge of the atomic state of the pp system at annihilation can be used to restrict the possible quantum numbers of meson resonances.

PhysicsParticle physicsAnnihilationMesonHigh Energy Physics::LatticeNuclear TheoryHigh Energy Physics::PhenomenologyInvariant (physics)Quantum numberAmplitudeQuark–gluon plasmaHomogeneous spaceHigh Energy Physics::ExperimentNuclear ExperimentSpectroscopy
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Determination of Strong-Phase Parameters in D→KS,L0π+π−

2020

We report the most precise measurements to date of the strong-phase parameters between D^{0} and D[over ¯]^{0} decays to K_{S,L}^{0}π^{+}π^{-} using a sample of 2.93  fb^{-1} of e^{+}e^{-} annihilation data collected at a center-of-mass energy of 3.773 GeV with the BESIII detector at the BEPCII collider. Our results provide the key inputs for a binned model-independent determination of the Cabibbo-Kobayashi-Maskawa angle γ/ϕ_{3} with B decays. Using our results, the decay model sensitivity to the γ/ϕ_{3} measurement is expected to be between 0.7° and 1.2°, approximately a factor of three smaller than that achievable with previous measurements, based on the studies of the simulated data. The…

PhysicsParticle physicsAnnihilationPhase (waves)General Physics and Astronomy01 natural scienceslaw.inventionlaw0103 physical sciencesCP violationCharm (quantum number)Sensitivity (control systems)010306 general physicsColliderMixing (physics)Energy (signal processing)Physical Review Letters
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Dark Matter and the Seesaw Scale

2018

We discuss the possibility to find an upper bound on the seesaw scale using the cosmological bound on the cold dark matter relic density. We investigate a simple relation between the origin of neutrino masses and the properties of a dark matter candidate in a simple theory where the new symmetry breaking scale defines the seesaw scale. Imposing the cosmological bounds, we find an upper bound of order multi-TeV on the lepton number violation scale. We investigate the predictions for direct and indirect detection dark matter experiments, and the possible signatures at the Large Hadron Collider.

PhysicsParticle physicsCold dark matter010308 nuclear & particles physicsDark matterHigh Energy Physics::PhenomenologyFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesLepton numberUpper and lower boundsPartícules (Física nuclear)High Energy Physics - ExperimentHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometryWeakly interacting massive particles0103 physical sciencesGran col·lisionador d'hadrons (França i Suïssa)High Energy Physics::ExperimentSymmetry breakingNeutrino010306 general physics
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Lepton number asymmetries and the lower bound on the reheating temperature

2017

We show that the reheating temperature of a matter-domination era in the early universe can be pushed down to the neutrino decoupling temperature at around $2 \ {\rm MeV}$ if the reheating takes place through non-hadronic decays of the dominant matter and neutrino-antineutrino asymmetries are still large enough, $|L| \gtrsim \mathcal{O}(10^{-2})$ (depending on the neutrino flavor) at the end of reheating.

PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFOS: Physical sciencesAstronomy and AstrophysicsNeutrino decouplingAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesLepton numberUpper and lower boundsUniverseGeneral Relativity and Quantum Cosmology0103 physical sciencesHigh Energy Physics::ExperimentNeutrino010303 astronomy & astrophysicsmedia_commonAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Spontaneous Breaking of Lepton Number and Cosmological Domain Wall Problem

2019

We show that if global lepton number symmetry is spontaneously broken in a post inflation epoch, then it can lead to the formation of cosmological domain walls. This happens in the well-known "Majoron paradigm" for neutrino mass generation. We propose some realistic examples which allow spontaneous lepton number breaking to be safe from such domain walls.

PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Mass generationHigh Energy Physics::PhenomenologyGeneral Physics and AstronomyFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesLepton numberSymmetry (physics)High Energy Physics - PhenomenologyDomain wall (string theory)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesDomain (ring theory)High Energy Physics::ExperimentNeutrino010306 general physicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Resurrection of large lepton number asymmetries from neutrino flavor oscillations

2016

We numerically solve the evolution equations of neutrino three-flavor density matrices, and show that, even if neutrino oscillations mix neutrino flavors, large lepton number asymmetries are still allowed in certain limits by Big Bang Nucleosynthesis (BBN).

PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics::Instrumentation and Detectors010308 nuclear & particles physicsHigh Energy Physics::LatticeAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFOS: Physical sciences01 natural sciencesLepton numberNuclear physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Big Bang nucleosynthesis0103 physical sciencesMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillationFlavorAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review D
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X-ray photons from late-decaying majoron dark matter

2008

An attractive way to generate neutrino masses as required to account for current neutrino oscillation data involves the spontaneous breaking of lepton number. The resulting majoron may pick up a mass due to gravity. If its mass lies in the kilovolt scale, the majoron can play the role of late-decaying Dark Matter (LDDM), decaying mainly to neutrinos. In general the majoron has also a sub-dominant decay to two photons leading to a mono-energetic emission line which can be used as a test of the LDDM scenario. We compare expected photon emission rates with observations in order to obtain model independent restrictions on the relevant parameters. We also illustrate the resulting sensitivities w…

PhysicsParticle physicsDark matterAstrophysics (astro-ph)High Energy Physics::PhenomenologyCosmic background radiationFOS: Physical sciencesFísicaAstronomy and AstrophysicsAstrophysicsLepton numberHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometryHiggs bosonHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationMajoron
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Impact parameter dependent JIMWLK evolution meets HERA data

2019

We calculate the small-$x$ evolution of protons with finite size by solving numerically the JIMWLK evolution equation. The initial condition is constrained by the HERA measurements of charm reduced cross section and of exclusive vector meson production. We compute the energy dependence of diffractive cross sections in order to access the energy evolution of the event-by-event fluctuating proton density profile. The fundamental problems arising from the regime sensitive to non-perturbatively large dipoles are also discussed.

PhysicsParticle physicsFOS: Physical sciencesHERAhiukkasfysiikkaHigh Energy Physics - PhenomenologyCross section (physics)DipoleHigh Energy Physics - Phenomenology (hep-ph)Initial value problemCharm (quantum number)Vector mesonImpact parameterEnergy (signal processing)Proceedings of International Conference on Hard and Electromagnetic Probes of High-Energy Nuclear Collisions — PoS(HardProbes2018)
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Neutrino masses and GUT baryogenesis

2004

We reconsider the GUT-baryogenesis mechanism for generating the baryon asymmetry of the Universe. The baryon asymmetry is produced by the out of equilibrium decay of coloured Higgs bosons at the GUT scale, conserving B-L. If neutrinos are Majorana particles, lepton number violating interactions erase the lepton number excess, but part of the baryon asymmetry may be preserved, provided those interactions are not in thermal equilibrium when the sphaleron processes become effective, at $T \sim 10^{12}~ GeV$. We analyse whether this mechanism for baryogenesis is feasible in a variety of GUT models of fermion masses proposed in the literature, based on horizontal symmetries.

PhysicsParticle physicsHigh Energy Physics::PhenomenologyFOS: Physical sciencesFermionLepton numberSphaleronBaryogenesisNuclear physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Baryon asymmetryHiggs bosonHigh Energy Physics::ExperimentNeutrinoParticle Physics - PhenomenologyBosonProceedings of International Workshop on Astroparticle and High Energy Physics — PoS(AHEP2003)
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