Search results for "Magnitude"

showing 10 items of 501 documents

Eta bound states in nuclei

2002

The energies and widths of bound states of the $\eta$ meson in different nuclei are obtained using the results for its selfenergy in a nuclear medium, which is evaluated in a selfconsistent manner using techniques of unitarized chiral perturbation theory. We find bound states in all studied nuclei (from $^{12}{C}$ on) and the half widths obtained are larger than the separation of the levels, what makes the experimental observation of peaks unlikely. We have paid a special attention to the region of nuclei where only the $1s$ state appears and the binding energies are of the order of magnitude of the half width, which would magnify the chances that some broad peak could be observed. This is …

PhysicsNuclear and High Energy PhysicsChiral perturbation theoryMesonNuclear TheoryBinding energyNuclear TheoryFísicaState (functional analysis)Bound stateProduction (computer science)Continuum (set theory)Atomic physicsNuclear ExperimentOrder of magnitude
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Sensitivity of electromagnetic spectra to equation of state and initial energy density in the Pb+Pb collisions at SPS

1998

We study Pb+Pb collisions at 158 A GeV/c using a hydrodynamical approach. We test different equations of state (EoSs) and different initial conditions and show that there are more than one initial state for each EoS which reproduce the observed hadronic spectra. We also find that different equations of state favour different freeze-out temperature. Simultaneously we calculate the thermal dilepton and photon spectra for each EoS and initial state. We compare the dilepton mass spectrum to data measured by the CERES collaboration and find that the differences in spectra obtained using different EoSs and initial states are not resolvable within the current experimental resolution. However, at i…

PhysicsNuclear and High Energy PhysicsEquation of stateNuclear TheoryHadronNuclear TheoryFOS: Physical sciencesSpectral lineNuclear Theory (nucl-th)Nuclear physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)ThermalMass spectrumRapidityNuclear ExperimentOrder of magnitudeLepton
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Non-analog β decay of 74Rb

2001

The magnitude of the Coulomb mixing parameter δ 1 has been experimentally deduced, for the first time, for the β decay of 74 Rb. The estimated magnitude is derived from the feeding of the non-analog first excited 0 + state in 74 Kr. The inferred upper limit of 0.07% is small compared to theoretical predictions. The half-life was measured to be 64.90(9) ms.  2001 Published by Elsevier Science B.V.

PhysicsNuclear and High Energy PhysicsExcited stateMagnitude (astronomy)CoulombAtomic physicsBeta decayMixing (physics)Physics Letters B
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Effects of orbital occupancies and spin–orbit partners II: decays of 76Ge, 82Se and 136Xe to first excited states

2011

Abstract The neutrinoless double beta ( 0 ν β β ) decays of 76Ge, 82Se and 136Xe to the first excited 0 + states ( 0 1 + ) in 76Se, 82Kr and 136Ba are studied in calculations using different sizes of the single-particle model spaces and different occupancies of the individual orbits. This is a continuation of a similar study [J. Suhonen, O. Civitarese, Effects of orbital occupancies and spin–orbit partners on 0 ν β β -decay rates, Nucl. Phys. A 847 (2010) 207–232] of the 0 ν β β decays of 76Ge, 82Se, 128Te, 130Te and 136Xe to the ground states of 76Se, 82Kr, 128Xe, 130Xe and 136Ba. The nuclear matrix elements and half-lives of the decays to the 0 1 + states are calculated by the use of the …

PhysicsNuclear and High Energy PhysicsExcited stateOrbit (dynamics)Nuclear forceBeta (velocity)Atomic physicsSpin (physics)Order of magnitudeNuclear Physics A
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Electro-produced slow positrons

1989

During the last 6 years it has been demonstrated that electro-produced intense beams of slow positrons are possible. High energy electrons from an accelerator generate bremsstrahlung in a thick conversion target of high element number Z. The photons produce electronpositron pairs and a small fraction of the positrons may be moderated to thermal energies. A review is given of the existing slow positron beam lines using this technique. At accelerator energies of 100 MeV total conversion efficiencies of several slow positrons per 106 primary electrons have been obtained, resulting in average intensities of several 109 slow positrons per second or more than 105 slow positrons in pulses having a…

PhysicsNuclear and High Energy PhysicsHigh energyPhotonBremsstrahlungElectronCondensed Matter PhysicsAtomic and Molecular Physics and OpticsIntensity (physics)Nuclear physicsPositronThermalPhysics::Accelerator PhysicsPhysical and Theoretical ChemistryAtomic physicsOrder of magnitudeHyperfine Interactions
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Presence of a soft excess between 0.6 keV and 0.9 keV in the energy spectrum of Cir X-1

2004

Abstract We report on the results of a new BeppoSAX (0.12–200 keV) observation of the peculiar X–ray binary source Circinus X–1 (Cir X–1) near the apastron. We produced a color-color diagram and selected seven different zones. We fitted the spectra obtained from each zone using a model consisting of a blackbody component, at a temperature of ∼0.5 keV, and a Comptonized component, with a seed-photon temperature of ∼1 keV, electron temperature of ∼2.7 keV and optical depth of ∼11. A soft excess between 0.6 keV and 0.9 keV is present in four out of the seven extracted spectra. To fit the soft excess we tried several continuum emission models, and we find good results only adding a further blac…

PhysicsNuclear and High Energy PhysicsHydrogenAstrophysics::High Energy Astrophysical PhenomenaBinary numberchemistry.chemical_elementAstrophysicsAtomic and Molecular Physics and OpticsSpectral linechemistryEnergy spectrumElectron temperatureCircinusBlack-body radiationOrder of magnitude
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Enhanced solar anti-neutrino flux in random magnetic fields

2004

We discuss the impact of the recent KamLAND constraint on the solar anti-neutrino flux on the analysis of solar neutrino data in the presence of Majorana neutrino transition magnetic moments and solar magnetic fields. We consider different stationary solar magnetic field models, both regular and random, highlighting the strong enhancement in the anti-neutrino production rates that characterize turbulent solar magnetic field models. Moreover, we show that for such magnetic fields inside the Sun, one can constrain the intrinsic neutrino magnetic moment down to the level of mu_nu lessthan few times 10^-12 x mu_B irrespective of details of the underlying turbulence model. This limit is more str…

PhysicsNuclear and High Energy PhysicsMagnetic momentMagnetismSolar neutrinoAstrophysics (astro-ph)FOS: Physical sciencesFísicaAstrophysicsMagnetic fieldNuclear physicsMAJORANAHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Physics::Space PhysicsNeutrinoOrder of magnitudeRandomness
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Determination of the η-transition form factor in the γp→pη→pγe+e− reaction

2011

The Dalitz decay η→γe+e− has been measured using the combined Crystal Ball and TAPS photon detector setup at the electron accelerator MAMI-C. Compared to the most recent transition form-factor measurement in the e+e− channel, statistics have been improved by one order of magnitude. The e+e− invariant mass distribution shows a deviation from the QED prediction for a point-like particle, which can be described by a form-factor. Using the usual monopole transition form-factor parameterization, F(m2)=(1−m2/Λ2)−1, a value of Λ−2=(1.92±0.35(stat)±0.13(syst)) GeV−2 has been determined. This value is in good agreement with a recent measurement of the η Dalitz decay in the μ+μ− channel and with rece…

PhysicsNuclear and High Energy PhysicsMass distribution010308 nuclear & particles physicsPoint particleBranching fractionForm factor (quantum field theory)Particle accelerator01 natural scienceslaw.inventionNuclear physicslaw0103 physical sciencesHigh Energy Physics::ExperimentInvariant massNuclear Experiment010306 general physicsOrder of magnitudeCrystal BallPhysics Letters B
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C(,pn) photon asymmetry for Eγ=180–340 MeV

1999

The photon asymmetry (Σ) of the 12C(,pn) reaction has been measured using linearly polarised tagged photons at the Mainz microtron MAMI for Eγ=180–340 MeV. The data have been analysed in separate missing energy (Em) regions corresponding to the ejection of nucleons from (1p)2 and (1p)(1s) shells. The measured Σ values for both Em regions are smaller in magnitude than corresponding 2H data, but the (1p)2 results have a similar Eγ dependence. Calculations of direct two-nucleon emission overestimate the magnitude of Σ at all photon energies.

PhysicsNuclear and High Energy PhysicsMissing energyPhotonmedia_common.quotation_subjectNuclear TheoryAsymmetryNuclear physicsMagnitude (astronomy)Atomic physicsNuclear ExperimentNucleonMicrotronmedia_commonPhysics Letters B
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Inclusive pion double charge exchange on 16O at 0.6-1.1 GeV

2003

The inclusive pion double charge exchange (DCX) on oxygen nuclei has been measured in the region where additional pion production is kinematically forbidden. The experiment was performed at ITEP PS at incident pi- kinetic energies T_0= 0.59, 0.75 and 1.1 GeV. The integrated forward differential cross section was found to decrease with energy slowly. At 1.1 GeV it exceeds the theoretical prediction within the conventional sequential single charge exchange mechanism with a neutral pion in the intermediate state (Glauber elastic rescattering) by about half an order of magnitude. The sequential mechanism with two pions in the intermediate state (Glauber inelastic rescatterings), which was propo…

PhysicsNuclear and High Energy PhysicsNuclear TheoryFísicaKinetic energyNuclear physicsCross section (physics)PionIntermediate stateHigh Energy Physics::ExperimentNuclear ExperimentGlauberOrder of magnitudeOxygen-16Charge exchange
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