Search results for "Basso continuo"

showing 5 items of 5 documents

1.6 GHz VLBI observations of SN 1979C: almost-free expansion

2009

We report on 1.6 GHz Very-Long-Baseline-Interferometry (VLBI) observations of supernova SN 1979C made on 18 November 2002. We derive a model-dependent supernova size. We also present a reanalysis of VLBI observations made by us on June 1999 and by other authors on February 2005. We conclude that, contrary to our earlier claim of strong deceleration in the expansion, SN 1979C has been undergoing almost-free expansion ($m = 0.91\pm0.09$; $R \propto t^m$) for over 25 years.

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Continuum (measurement)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsSupernovaSpace and Planetary ScienceVery-long-baseline interferometryFree expansionBasso continuoAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic AstrophysicsAstronomy & Astrophysics
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The iron K-shell features of MXB 1728-34 from a simultaneous Chandra-RXTE observation

2005

We report on a simultaneous Chandra and RossiXTE observation of the low-mass X-ray binary atoll bursting source MXB 1728-34 performed on 2002 March 3-5. We fit the 1.2-35 keV continuum spectrum with a blackbody plus a Comptonized component. Large residuals at 6-10 keV can be fitted by a broad (FWHM ~ 2 keV) Gaussian emission line or, alternatively, by two absorption edges associated with lowly ionized iron and Fe XXV/XXVI at ~7.1 keV and ~9 keV, respectively. In this interpretation, we find no evidence of broad, or narrow, emission lines between 6 and 7 keV. We test our alternative modelling of the iron K shell region by reanalysing a previous BeppoSAX observation of MXB 1728-34, finding a …

PhysicsAstrophysics::High Energy Astrophysical Phenomenaindividual : MXB 1728-34; stars : neutron; X-rays : stars; X-rays : binaries; X-rays : general [accretion accretion disks; stars]Astrophysics (astro-ph)X-ray binaryElectron shellAstronomyFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysicsaccretion accretion diskstars : neutronNeutron starAbsorption edgeSpace and Planetary ScienceIonizationX-rays : starBlack-body radiationEmission spectrumBasso continuoX-rays : binariestars : individual : MXB 1728-34X-rays : general
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Cross-sections for (e, 3e) collisions on helium: the DS6C wavefunction

2006

A dynamically screened product of six pairwise Coulomb functions (DS6C) is used as an analytic approximation to describe the four-body Coulomb continuum state produced by electron-impact full fragmentation of helium. Good agreement is obtained with experimental data close to threshold, where four-body effects are expected to be important. Even for the high impact energy of 640 eV, four-body effects still play a role in deciding the shape of multi-differential cross-sections.

PhysicsContinuum (measurement)chemistry.chemical_elementCondensed Matter PhysicsAtomic and Molecular Physics and OpticschemistryFragmentation (mass spectrometry)CoulombImpact energyAtomic physicsBasso continuoWave functionHeliumElectron ionizationJournal of Physics B: Atomic, Molecular and Optical Physics
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The effect of dynamical screening on helium (e, 3e) differential cross-sections

2005

A simplified derivation of dynamic screening in the case of three Coulomb-interacting particles in the continuum is given and applied to describe the shapes of multi-differential cross-sections for the (e, 3e) process on the helium atom in which the incident fast electron is treated in first-order Born approximation. A very good agreement with experimental multi-differential cross-sections is obtained for two slow ejected electrons (specifically both electrons have 5 eV) but the strategy appears to be breaking down at intermediate emission energies.

PhysicsDynamic screeningHelium atomchemistry.chemical_elementElectronCondensed Matter PhysicsAtomic and Molecular Physics and Opticschemistry.chemical_compoundchemistryBasso continuoAtomic physicsBorn approximationElectron ionizationHeliumJournal of Physics B: Atomic, Molecular and Optical Physics
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D mesic nuclei

2010

The energies and widths of several D-0 meson bound states for different nuclei are obtained using a D-meson selfenergy in the nuclear medium, which is evaluated in a selfconsistent manner using techniques of unitarized coupled-channel theory. The kernel of the meson-baryon interaction is based on a model that treats heavy pseudoscalar and heavy vector mesons on equal footing, as required by heavy quark symmetry. We find D-0 bound states in all studied nuclei, from C-12 up to Pb-208. The inclusion of vector mesons is the keystone for obtaining an attractive D-nucleus interaction that leads to the existence of D-0-nucleus bound states, as compared to previous studies based on SU(4) flavor sym…

QuarkNuclear reactionNuclear and High Energy PhysicsParticle physicsCharmNuclear TheoryMesonHigh Energy Physics::LatticeNuclear TheoryFOS: Physical sciencesHEAVY-ION COLLISIONS01 natural sciences7. Clean energyBOUND-STATESHigh Energy Physics - ExperimentNuclear Theory (nucl-th)Nuclear physicsENERGYHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)ANTIPROTON ANNIHILATION0103 physical sciencesBound stateHeavy quark effective theorySCATTERINGNuclear Experiment (nucl-ex)Basso continuoNuclear Experiment010306 general physicsNuclear ExperimentSUPPRESSIONPhysicsPIONIC ATOMS010308 nuclear & particles physicsScatteringHigh Energy Physics::PhenomenologyFísicaCHIRAL DYNAMICSHeavy quark symmetryETAPseudoscalarHigh Energy Physics - PhenomenologyMesic nucleiPhysics Letters B
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