Incompressibility of Nuclear Matter from the Giant Monopole Resonance

1999 ◽  
Vol 82 (4) ◽  
pp. 691-694 ◽  
Author(s):  
D. H. Youngblood ◽  
H. L. Clark ◽  
Y.-W. Lui
Keyword(s):  
Nuclear Matter ◽  
Giant Monopole Resonance

Nuclear matter incompressibility coefficient and giant monopole resonance

1994 ◽  
Vol 569 (1-2) ◽  
pp. 303-312 ◽  
Author(s):  
S. Shlomo ◽  
D.H. Youngblood
Keyword(s):  
Nuclear Matter ◽  
Giant Monopole Resonance

scholarly journals Nuclear matter compressibility from isoscalar giant monopole resonance

1993 ◽  
Vol 47 (2) ◽  
pp. 529-536 ◽  
Author(s):  
S. Shlomo ◽  
D. H. Youngblood
Keyword(s):  
Nuclear Matter ◽  
Giant Monopole Resonance

NUCLEAR MATTER PROPERTIES FROM COLLECTIVE MODES IN NUCLEI

2006 ◽  
Vol 15 (08) ◽  
pp. 1909-1923
Author(s):  
SHALOM SHLOMO ◽  
V. KIM AU
Keyword(s):  
Nuclear Matter ◽  
Cross Sections ◽  
Heavy Ion ◽  
Current Status ◽  
Transition Strength ◽  
Ion Collisions ◽  
Dipole Resonance ◽  
Giant Monopole Resonance ◽  
Physical Quantities ◽  
Supernova Collapse

Bulk properties of nuclear matter associated with the equation of state, the nuclear matter incompressibility coefficient, Knm, in particular, are very important physical quantities required in the study of properties of nuclei, supernova collapse, neutron stars and heavy-ion collisions. Here we review the current status of Knm and the experimental and theoretical methods used to determine the value of Knm from the excitation cross-sections and the transition strength distributions of compression modes in nuclei, mainly the the isoscalar giant monopole resonance and the isoscalar giant dipole resonance.

Compressibility of nuclear matter from the giant monopole resonance

1999 ◽  
Vol 649 (1-4) ◽  
pp. 49-56 ◽  
Author(s):  
D.H. Youngblood ◽  
H.L. Clark ◽  
Y.-W. Lui
Keyword(s):  
Nuclear Matter ◽  
Giant Monopole Resonance

scholarly journals Softness of Sn isotopes in relativistic semiclassical approximation

2015 ◽  
Vol 30 (20) ◽  
pp. 1550097 ◽  
Author(s):  
S. K. Biswal ◽  
S. K. Singh ◽  
S. K. Patra
Keyword(s):  
Nuclear Matter ◽  
Semiclassical Approximation ◽  
Excitation Energies ◽  
Thomas Fermi ◽  
Giant Monopole Resonance

Within the framework of relativistic Thomas–Fermi (RTF) and relativistic extended Thomas–Fermi (RETF) approximations, we calculate the giant monopole resonance (GMR) excitation energies for Sn and related nuclei. A large number of nonlinear relativistic force parameters are used in these calculations. We find a parameter set is capable to reproduce the experimental monopole energy of Sn isotopes, when its nuclear matter compressibility lies within 210–230 MeV, however, it fails to reproduce the GMR energy of other nuclei. That means, simultaneously a parameter set cannot reproduce the GMR values of Sn and other nuclei.

scholarly journals Giant monopole resonance in Sn and Sm nuclei and the compressibility of nuclear matter

1988 ◽  
Vol 38 (6) ◽  
pp. 2562-2572 ◽  
Author(s):  
M. M. Sharma ◽  
W. T. A. Borghols ◽  
S. Brandenburg ◽  
S. Crona ◽  
A. van der Woude ◽  
...  
Keyword(s):  
Nuclear Matter ◽  
Giant Monopole Resonance

TEMPERATURE DEPENDENCE OF THE EFFECTIVE INTERACTION IN NUCLEAR MATTER

1987 ◽  
Vol 48 (C2) ◽  
pp. C2-301-C2-304
Author(s):  
M. BALDO ◽  
G. GIANSIRACUSA ◽  
U. LOMBARDO
Keyword(s):  
Nuclear Matter ◽  
Temperature Dependence ◽  
Effective Interaction
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