Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Saturation properties and incompressibility of nuclear matter: A consistent determination from nuclear masses

Journal Article · · Physical Review, C
 [1]; ;  [2]
  1. Physics Department, Ravenshaw College, Cuttack (India)
  2. Institute of Physics, Bhubaneswar-751005 (India)
Starting with a two-body effective nucleon-nucleon interaction, it is shown that the infinite nuclear matter model of atomic nuclei is more appropriate than the conventional Bethe-Weizsacker-like mass formulas to extract saturation properties of nuclear matter from nuclear masses. In particular, the saturation density thus obtained agrees with that of electron scattering data and the Hartree-Fock calculations. For the first time using nuclear mass formula, the radius constant {ital r}{sub 0}=1.138 fm and binding energy per nucleon {ital a}{sub {ital v}}={minus}16.11 MeV, corresponding to the infinite nuclear matter, are consistently obtained from the same source. An important off-shoot of this study is the determination of nuclear matter incompressibility {ital K}{sub {infinity}} to be 288{plus_minus}28 MeV using the same source of nuclear masses as input.
OSTI ID:
90546
Journal Information:
Physical Review, C, Journal Name: Physical Review, C Journal Issue: 2 Vol. 52; ISSN 0556-2813; ISSN PRVCAN
Country of Publication:
United States
Language:
English

Similar Records

The Symmetry Energy Term in Nuclear Incompressibility from Giant Monopole Resonances: A Short Status Report
Journal Article · Thu May 07 00:00:00 EDT 2009 · AIP Conference Proceedings · OSTI ID:21304898

Finite range momentum and density dependent effective interaction and analysis of nuclear incompressibility
Journal Article · Fri Dec 31 23:00:00 EST 1993 · Physical Review, C (Nuclear Physics); (United States) · OSTI ID:5339583

Incompressibility of nuclear matter, and Coulomb and volume-symmetry coefficients of nucleus incompressibility in the relativistic mean field theory
Journal Article · Wed May 01 00:00:00 EDT 1996 · Physical Review, C · OSTI ID:283995