Finite range momentum and density dependent effective interaction and analysis of nuclear incompressibility

1994 ◽  
Vol 49 (1) ◽  
pp. 541-544 ◽  
Author(s):  
M. M. Majumdar ◽  
S. K. Samaddar ◽  
N. Rudra ◽  
J. N. De
2017 ◽  
Vol 26 (05) ◽  
pp. 1750022 ◽  
Author(s):  
B. K. Agrawal ◽  
S. K. Samaddar ◽  
J. N. De ◽  
C. Mondal ◽  
Subhranil De

In the framework of an equation of state (EoS) constructed from a momentum and density-dependent finite-range two-body effective interaction, the quantitative magnitudes of the different symmetry elements of infinite nuclear matter are explored. The parameters of this interaction are determined from well-accepted characteristic constants associated with homogeneous nuclear matter. The symmetry energy coefficient [Formula: see text], its density slope [Formula: see text], the symmetry incompressibility [Formula: see text] as well as the density-dependent incompressibility [Formula: see text] evaluated with this EoS are seen to be in good harmony with those obtained from other diverse perspectives. The higher order symmetry energy coefficients [Formula: see text], etc., are seen to be not very significant in the domain of densities relevant to finite nuclei, but gradually build up at supra-normal densities. The analysis carried out with a Skyrme-inspired energy density functional (EDF) obtained with the same input values for the empirical bulk data associated with nuclear matter yields nearly the same results.


2005 ◽  
Vol 14 (05) ◽  
pp. 739-749 ◽  
Author(s):  
D. N. BASU

An interesting method of obtaining the equation of state for nuclear matter, from a density dependent M3Y interaction, by minimizing the energy per nucleon is described. The density dependence parameters of the interaction are obtained by reproducing the saturation energy per nucleon and the saturation density of spin and isospin symmetric cold infinite nuclear matter. The nuclear matter equation of state thus obtained is then used to calculate the pressure, energy density, nuclear incompressibility and velocity of sound in nuclear medium. The results obtained are in good agreement with experimental data and provide a unified description of radioactivity, scattering and nuclear matter.


1996 ◽  
Vol 386 (1-4) ◽  
pp. 7-11 ◽  
Author(s):  
G. Bartnitzky ◽  
H. Clement ◽  
P. Czerski ◽  
H. Müther ◽  
F. Nuoffer ◽  
...  

2002 ◽  
Vol 11 (05) ◽  
pp. 369-378
Author(s):  
SERBULENT YILDIRIM ◽  
ABDURRAHMAN TARIKCI

Collisional damping widths of isoscalar giant monopole, isovector giant dipole and isoscalar giant quadrupole excitations for 120 Sn and 208 Pb at zero and finite temperatures are calculated within Thomas-Fermi approximation by employing a recently proposed modified Skyrme force and the results are compared with previous works.


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