Search results for "Radius"

showing 10 items of 708 documents

Constraints on cosmological models from strong gravitational lensing systems

2012

Strong lensing has developed into an important astrophysical tool for probing both cosmology and galaxies (their structure, formation, and evolution). Using the gravitational lensing theory and cluster mass distribution model, we try to collect a relatively complete observational data concerning the Hubble constant independent ratio between two angular diameter distances $D_{ds}/D_s$ from various large systematic gravitational lens surveys and lensing by galaxy clusters combined with X-ray observations, and check the possibility to use it in the future as complementary to other cosmological probes. On one hand, strongly gravitationally lensed quasar-galaxy systems create such a new opportun…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Strong gravitational lensingFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsCosmologyRedshiftEinstein radiussymbols.namesakeGravitational lenssymbolsDark energyGalaxy clusterAstrophysics - Cosmology and Nongalactic AstrophysicsHubble's lawJournal of Cosmology and Astroparticle Physics
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form factor at order of chiral perturbation theory

2001

Abstract This paper describes the calculation of the electromagnetic form factor of the K 0 meson at order p 6 of chiral perturbation theory which is the next-to-leading order correction to the well-known p 4 result achieved by Gasser and Leutwyler. On the one hand, at order p 6 the chiral expansion contains 1- and 2-loop diagrams which are discussed in detail. Especially, a numerical procedure for calculating the irreducible 2-loop graphs of the sunset topology is presented. On the other hand, the chiral Lagrangian L (6) produces a direct coupling of the K 0 current with the electromagnetic field tensor. Due to this coupling one of the unknown parameters of L (6) occurs in the contribution…

PhysicsCouplingNuclear and High Energy PhysicsChiral perturbation theoryMesonCharge radiusHigh Energy Physics::LatticeForm factor (quantum field theory)Order (group theory)Direct couplingMathematical physicsElectromagnetic tensorNuclear Physics B
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Halo-like structure in 7He nucleus

2020

Abstract A study of the neutron structure of the ground state of 7He has been performed by means of registration and analysis of the decay channels of the residual nuclei following absorption of stopped pions. In particular, the reaction 9Be ( π − , d )X have been investigated where X denotes any system with five neutrons and two protons – the constituencies of a 7He nucleus. It was shown that the structure of 7He is determined by correlations of two neutrons in the states 6He (0+), 6He (2+) and one neutron in the shell p3/2. The 4He+3n structure is not manifested in the ground state of 7He. The obtained results are consistent with the known data on considerable mixture of configurations “6…

PhysicsDiffractionHistoryRadiusComputer Science ApplicationsEducationPionmedicine.anatomical_structureTheoryofComputation_ANALYSISOFALGORITHMSANDPROBLEMCOMPLEXITYExcited statemedicineNeutronHaloAtomic physicsGround stateNucleusJournal of Physics: Conference Series
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Rotational band in 12C based on the Hoyle state

2014

t. α + 12C inelastic differential cross-sections were measured at the energies 65 and 110 MeV. A new broad state at 13.75 MeV was observed. Its spin-parity has been determined as 4+ and the diffraction radius of the corresponding L = 4 transition is ~ 0.8 fm larger than that of the excitation of the 4+, 14.8 MeV level. The 13.75 MeV state was considered to be the third member of the rotational band based on the Hoyle state. peerReviewed

PhysicsDiffractionHoyle stateta114PhysicsQC1-999State (functional analysis)RadiusAtomic physicsNuclear ExperimentExcitationEPJ Web of Conferences
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The Near-Infrared Surface Brightness Distribution of NGC4696

2006

We present H-band observations of the elliptical galaxy NGC4696, the brightest member of the Centaurus cluster of galaxies. We have measured its light profile, using a two-dimensional fitting algorithm, out to a radius of 180 arcsec (37 h^{-1}_{70} kpc). The profile is well described by a de Vaucouleurs law, with an effective radius of 35.3 +/- 1.0 h^{-1}_{70} kpc. There is no need for the extra free parameter allowed by a Sersic law. Allowing for a variation of 0.3% in the sky level, the profile obtained is compatible with data from 2MASS. The profile shows no sign of either a truncation or an extended halo.

PhysicsEffective radiusmedia_common.quotation_subjectAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsRadiusAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsSpace and Planetary ScienceSkyElliptical galaxyHaloSurface brightnessGalaxy clusterAstrophysics::Galaxy Astrophysicsmedia_commonFree parameter
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Puzzling out the proton radius puzzle

2014

The discrepancy between the proton charge radius extracted from the muonic hydrogen Lamb shift measurement and the best present value obtained from the elastic scattering experiments, remains unexplained and represents a burning problem of today’s nuclear physics: after more than 50 years of research the radius of a basic constituent of matter is still not understood. This paper presents a summary of the best existing proton radius measurements, followed by an overview of the possible explanations for the observed inconsistency between the hydrogen and the muonic-hydrogen data. In the last part the upcoming experiments, dedicated to remeasuring the proton radius, are described.

PhysicsElastic scatteringHydrogenProtonPhysicsQC1-999chemistry.chemical_elementRadiusLamb shiftNuclear physicschemistryCharge radiusPhysics::Atomic PhysicsAtomic physicsNuclear ExperimentExotic atomAIP Conference Proceedings
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The elastic scattering of 25MeV α-particles and neutron shell effects in the A = 50 TO A = 93 mass region

1982

Abstract Experimental elastic scattering angular distributions of 25 MeV α-particles scattered from 28 nuclei ranging from 50Cr to 93Nb have been measured and then analysed in terms of a regular optical model with standard Woods-Saxon geometries for both the real and imaginary potentials. The experimental distributions are well fitted over the whole angular range from 5° to 175° c.m. by the predictions, provided that a smaller than normal diffuseness is used for the imaginary potentials. The usual families of potentials with volume integrals differing by approximately 100 MeV · fm3 are found. The family with volume integral ranging from 540 to 420 MeV· fm3 over the nuclei studied has been c…

PhysicsElastic scatteringNuclear reactionNuclear and High Energy PhysicsPairingNuclear TheoryShell (structure)NeutronRadiusAtomic physicsNuclear ExperimentAbsorption (electromagnetic radiation)Volume integralNuclear Physics A
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Two-photon exchange corrections in elastic electron-proton scattering

2015

We apply a subtracted dispersion relation (DR) formalism with the aim to improve predictions for the two-photon exchange (TPE) corrections to elastic electron-proton scattering observables at small momentum transfers. We study the formalism on the elastic TPE contribution in comparison with existing data for unpolarized cross sections. We extend the general formalism of TPE to elastic scattering with massive lepton and perform a numerical estimate of the muon-proton scattering at low momentum transfer in view of the upcoming muon-proton scattering experiment (MUSE). We study the influence of the double-virtual Compton scattering (VVCS) subtraction function on the unpolarized lepton-proton s…

PhysicsElastic scatteringPhotonNuclear TheoryProtonScatteringMomentum transferCompton scatteringFOS: Physical sciencesElectronNuclear Theory (nucl-th)Nuclear physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Charge radiusNuclear ExperimentProceedings of 53rd International Winter Meeting on Nuclear Physics — PoS(Bormio2015)
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ISR Experiment at A1-Collaboration

2019

The discrepancy between the proton charge radius extracted from the muonic hydrogen Lamb shift measurement and the best present value obtained from the elastic scattering experiments, remains unexplained and represents a burning problem of today’s nuclear physics. In a pursuit of reconciling the puzzle an experiment is underway at MAMI, which exploits the radiative tail of the elastic peak to study the properties of electromagnetic processes and to extract the proton charge form factor $ \left( {\mathop G\nolimits_E^p } \right) $ at extremely small Q2. This paper reports on the latest results of the first such measurement performed at the three-spectrometer facility of the A1-Collaboration,…

PhysicsElastic scatteringProton010308 nuclear & particles physicsPhysicsQC1-999Form factor (quantum field theory)Charge (physics)01 natural sciencesLamb shiftNuclear physicsCharge radius0103 physical sciencesRadiative transfer010306 general physicsExotic atomEPJ Web of Conferences
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Comparison of woods-saxon and double-folding potentials forα-particle scattering from54Fe at 24.5 MeV

1988

Inelastic-scattering data are presented forα-particles of 24.5 MeV from54Fe over the range 15° to 175° in the centre-of-mass system. The real part of the optical potential is calculated microscopically using the M3Y effective interaction of Bertschet al. and the DDM3Y density-dependent interaction. Elastic scattering has been analysed by using as real part of the optical potential M3Y, DDM3Y and Woods-Saxon forms (WS), taking in all three cases as imaginary part a WS potential. To fit the data the double-folding potential needs to be normalized by a factor of ⋍1.6 for the M3Y interaction and of ⋍1.13 for the DDM3Y interaction. By the study of the invariant-point ambiguity it has been observ…

PhysicsElastic scatteringRange (particle radiation)Scattering theoryRadiusInelastic scatteringWell-definedInvariant (mathematics)Atomic physicsInelastic neutron scatteringIl Nuovo Cimento A
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