Analysis of colliding nuclear matter in terms of symmetry energy and cross-section using computational method

2015 ◽  
Author(s):  
Arun Sharma ◽  
Sakshi Gautam ◽  
Arun Bharti
Keyword(s):  
Nuclear Matter ◽  
Cross Section ◽  
Symmetry Energy ◽  
Computational Method

Elastic nucleon-nucleon cross section in nuclear matter at finite temperature

1998 ◽  
Vol 57 (2) ◽  
pp. 806-810 ◽  
Author(s):  
A. Schnell ◽  
G. Röpke ◽  
U. Lombardo ◽  
H.-J. Schulze
Keyword(s):  
Nuclear Matter ◽  
Cross Section ◽  
Finite Temperature ◽  
Nucleon Nucleon

scholarly journals Nuclear matter symmetry energy at0.03⩽ρ/ρ0⩽0.2

2012 ◽  
Vol 85 (6) ◽  
Author(s):  
R. Wada ◽  
K. Hagel ◽  
L. Qin ◽  
J. B. Natowitz ◽  
Y. G. Ma ◽  
...  
Keyword(s):  
Nuclear Matter ◽  
Symmetry Energy

The nucleon-nucleon cross section in ground-state and colliding nuclear matter

1996 ◽  
Vol 601 (3-4) ◽  
pp. 505-525 ◽  
Author(s):  
C. Fuchs ◽  
L. Sehn ◽  
H.H. Wolter
Keyword(s):  
Nuclear Matter ◽  
Cross Section ◽  
Ground State ◽  
Nucleon Nucleon

scholarly journals Limiting symmetry energy elements from empirical evidence

2017 ◽  
Vol 26 (05) ◽  
pp. 1750022 ◽  
Author(s):  
B. K. Agrawal ◽  
S. K. Samaddar ◽  
J. N. De ◽  
C. Mondal ◽  
Subhranil De
Keyword(s):  
Nuclear Matter ◽  
Symmetry Energy ◽  
Density Functional ◽  
Effective Interaction ◽  
Finite Range ◽  
Energy Density Functional ◽  
Density Dependent ◽  
Bulk Data ◽  
Energy Coefficient ◽  
Finite Nuclei

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.

K+-nucleus total cross section and polarization of nuclear matter

1995 ◽  
Vol 585 (1-2) ◽  
pp. 337-338 ◽  
Author(s):  
J.C. Caillon ◽  
J. Labarsouque
Keyword(s):  
Total Cross Section ◽  
Nuclear Matter ◽  
Cross Section
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