Application of relativistic mean field and effective field theory densities to scattering observables for Ca isotopes
Abstract
In the framework of relativistic mean field (RMF) theory, we have calculated the density distribution of protons and neutrons for {sup 40,42,44,48}Ca with NL3 and G2 parameter sets. The microscopic protonnucleus optical potentials for p+{sup 40,42,44,48}Ca systems are evaluated from the Dirac nucleonnucleon scattering amplitude and the density of the target nucleus using relativisticLoveFraney and McNeilRayWallace parametrizations. We have estimated the scattering observables, such as the elastic differential scattering cross section, analyzing power and the spin observables with the relativistic impulse approximation (RIA). The results have been compared with the experimental data for a few selective cases and we find that the use of density as well as the scattering matrix parametrizations are crucial for the theoretical prediction.
 Authors:
 Institute of Physics, Sachivalaya Marg, Bhubaneswar751 005 (India)
 (India)
 Department of Physics, ITER, Siksha O Anusandhan University, Bhubaneswar751 030 (India)
 School of Physics, Sambalpur University, Jyotivihar, Burla 768 019 (India)
 Publication Date:
 OSTI Identifier:
 21499273
 Resource Type:
 Journal Article
 Resource Relation:
 Journal Name: Physical Review. C, Nuclear Physics; Journal Volume: 82; Journal Issue: 6; Other Information: DOI: 10.1103/PhysRevC.82.064602; (c) 2010 American Institute of Physics
 Country of Publication:
 United States
 Language:
 English
 Subject:
 73 NUCLEAR PHYSICS AND RADIATION PHYSICS; AMPLITUDES; CALCIUM 40; CALCIUM 42; CALCIUM 44; COMPUTERIZED SIMULATION; CROSS SECTIONS; DENSITY; DISTRIBUTION; FIELD THEORIES; FORECASTING; IMPULSE APPROXIMATION; MEANFIELD THEORY; NEUTRONS; NUCLEONNUCLEON INTERACTIONS; POLARIZATIONASYMMETRY RATIO; PROTONNUCLEON INTERACTIONS; PROTONS; RELATIVISTIC RANGE; SCATTERING; SPIN; ALKALINE EARTH ISOTOPES; ANGULAR MOMENTUM; APPROXIMATIONS; BARYONBARYON INTERACTIONS; BARYONS; CALCIUM ISOTOPES; CALCULATION METHODS; DIMENSIONLESS NUMBERS; ELEMENTARY PARTICLES; ENERGY RANGE; EVENEVEN NUCLEI; FERMIONS; HADRONHADRON INTERACTIONS; HADRONS; INTERACTIONS; INTERMEDIATE MASS NUCLEI; ISOTOPES; LIGHT NUCLEI; NUCLEI; NUCLEONS; PARTICLE INTERACTIONS; PARTICLE PROPERTIES; PHYSICAL PROPERTIES; SIMULATION; STABLE ISOTOPES
Citation Formats
Bhuyan, M., School of Physics, Sambalpur University, Jyotivihar, Burla 768 019, Panda, R. N., Routray, T. R., and Patra, S. K.. Application of relativistic mean field and effective field theory densities to scattering observables for Ca isotopes. United States: N. p., 2010.
Web. doi:10.1103/PHYSREVC.82.064602.
Bhuyan, M., School of Physics, Sambalpur University, Jyotivihar, Burla 768 019, Panda, R. N., Routray, T. R., & Patra, S. K.. Application of relativistic mean field and effective field theory densities to scattering observables for Ca isotopes. United States. doi:10.1103/PHYSREVC.82.064602.
Bhuyan, M., School of Physics, Sambalpur University, Jyotivihar, Burla 768 019, Panda, R. N., Routray, T. R., and Patra, S. K.. Wed .
"Application of relativistic mean field and effective field theory densities to scattering observables for Ca isotopes". United States.
doi:10.1103/PHYSREVC.82.064602.
@article{osti_21499273,
title = {Application of relativistic mean field and effective field theory densities to scattering observables for Ca isotopes},
author = {Bhuyan, M. and School of Physics, Sambalpur University, Jyotivihar, Burla 768 019 and Panda, R. N. and Routray, T. R. and Patra, S. K.},
abstractNote = {In the framework of relativistic mean field (RMF) theory, we have calculated the density distribution of protons and neutrons for {sup 40,42,44,48}Ca with NL3 and G2 parameter sets. The microscopic protonnucleus optical potentials for p+{sup 40,42,44,48}Ca systems are evaluated from the Dirac nucleonnucleon scattering amplitude and the density of the target nucleus using relativisticLoveFraney and McNeilRayWallace parametrizations. We have estimated the scattering observables, such as the elastic differential scattering cross section, analyzing power and the spin observables with the relativistic impulse approximation (RIA). The results have been compared with the experimental data for a few selective cases and we find that the use of density as well as the scattering matrix parametrizations are crucial for the theoretical prediction.},
doi = {10.1103/PHYSREVC.82.064602},
journal = {Physical Review. C, Nuclear Physics},
number = 6,
volume = 82,
place = {United States},
year = {Wed Dec 15 00:00:00 EST 2010},
month = {Wed Dec 15 00:00:00 EST 2010}
}

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