Heavy-ion interactions in relativistic mean-field models

1996 ◽  
Vol 602 (3-4) ◽  
pp. 502-512 ◽  
Author(s):  
M. Rashdan
Keyword(s):  
Mean Field ◽  
Heavy Ion ◽  
Relativistic Mean Field ◽  
Ion Interactions ◽  
Mean Field Models

scholarly journals Parameter counting in relativistic mean-field models

2000 ◽  
Vol 671 (1-4) ◽  
pp. 447-460 ◽  
Author(s):  
R.J. Furnstahl ◽  
Brian D. Serot
Keyword(s):  
Mean Field ◽  
Relativistic Mean Field ◽  
Mean Field Models

DENSITY AND ISOSPIN DEPENDENCIES IN RELATIVISTIC MEAN FIELD MODELS

2004 ◽  
Author(s):  
M. SERRA ◽  
T. OTSUKA ◽  
Y. AKAISHI ◽  
S. HIROSE ◽  
P. RING
Keyword(s):  
Mean Field ◽  
Relativistic Mean Field ◽  
Mean Field Models

scholarly journals Consistent relativistic mean-field models constrained by GW170817

2019 ◽  
Vol 99 (4) ◽  
Author(s):  
Odilon Lourenço ◽  
Mariana Dutra ◽  
César H. Lenzi ◽  
César V. Flores ◽  
Débora P. Menezes
Keyword(s):  
Mean Field ◽  
Relativistic Mean Field ◽  
Mean Field Models

Covariant Equation of State for Two Colliding Nuclear Matters in the Relativistic Meson Field Theory

1997 ◽  
Vol 06 (01) ◽  
pp. 151-159 ◽  
Author(s):  
M. Rashdan
Keyword(s):  
Field Theory ◽  
Equation Of State ◽  
Nonlinear Models ◽  
Mean Field Theory ◽  
Mean Field ◽  
Heavy Ion ◽  
Ion Scattering ◽  
Relativistic Mean Field ◽  
Heavy Ion Scattering ◽  
Covariant Equation

The relativistic mean field theory (linear and nonlinear) models are extended to the case of two colliding nuclear matters, relevant to heavy ion scattering and reactions. The effect of vacuum corrections is taken into account through the relativistic Hartree approximation. The Fermi sea is assumed to consist of two colliding Lorentz elongated spheres. A relativistic covariant Pauli correction is considered for the overlap case. This relativistic Pauli correction is found to be very important due to its dependence on the effective nucleon mass which strongly depends on the model equation of state. It is found that by increasing the velocity the energy per baryon increases and saturates at higher densities. The increase in the energy per baryon at low density (the region of no overlap) is much larger than that at high density (the region of large overlap), due to Pauli correction effects. The saturation density of the nonlinear model is shifted to larger values than that of the linear model. Vacuum corrections effects are found to reduce largely te overlap region.

scholarly journals Relativistic mean-field models and nuclear matter constraints

2013 ◽  
Author(s):  
M. Dutra ◽  
O. Lourenço ◽  
B. V. Carlson ◽  
A. Delfino ◽  
D. P. Menezes ◽  
...  
Keyword(s):  
Nuclear Matter ◽  
Mean Field ◽  
Relativistic Mean Field ◽  
Mean Field Models

Dynamical Instabilities in Relativistic Mean-Field Models and Inner Edge of the Compact Star Crust

2010 ◽  
Author(s):  
Alexandre Santos ◽  
Lucília Brito ◽  
Constança Provide^ncia ◽  
J. A. Caballero ◽  
C. E. Alonso ◽  
...  
Keyword(s):  
Compact Star ◽  
Mean Field ◽  
Relativistic Mean Field ◽  
Mean Field Models ◽  
Dynamical Instabilities
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