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GROUND STATE PROPERTIES OF O{sup 16}, Ca{sup 40} AND Ca{sup 48} IN A RELATIVISTIC HARTREE THEORY OF NUCLEAR MATTER [electronic resource].

Published:
Berkeley, Calif. : Lawrence Berkeley National Laboratory. Nuclear Science Division, 1980.
Oak Ridge, Tenn. : Distributed by the Office of Scientific and Technical Information, U.S. Dept. of Energy.
Physical Description:
18 pages : digital, PDF file
Additional Creators:
Lawrence Berkeley National Laboratory, Lawrence Berkeley National Laboratory. Nuclear Science Division, and United States. Department of Energy. Office of Scientific and Technical Information
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Summary:
A relativistic field theory model of nuclear matter is solved in a Hartree approximation for finite nuclei. We show that the theory predicts small shell effects for the charge density distributions in magic nuclei and is in agreement with recent electron scattering data. The effects of the small component of the relativistic wave function are investigated as well as the role of the isospin dependent force generated by the rho field.
Report Numbers:
E 1.99:lbl-11894
lbl-11894
Subject(s):
Note:
Published through SciTech Connect.
12/01/1980.
"lbl-11894"
Nuclear Physics A FT
Boguta, J.
Funding Information:
DE-AC02-05CH11231
View MARC record | catkey: 14669357