The properties of symmetric nuclear matter are investigated in the nonlinear relativistic mean field theory of nuclear matter. We consider the constraints imposed by four nuclear ground state properties on the coupling constants and on the equation of state at zero and at finite temperature. We find that the compression constant K(ρ0) as well as the temperature is irrelevant for the stiffness of the equation of state for m*(ρ0)≤0.7. The main point is that the relativistic mean field theory exhibits acausal and unphysical behavior for compressibilities below K(ρ0)=200 MeV. Every set of coupling constants with a negative quartic coupling constant c is unstable against small quantum fluctuations
We have determined the equation of state of nuclear matter according to relativistic non-linear mode...
International audienceWe have determined the equation of state of nuclear matter according to relati...
In order to predict properties of asymmetric nuclear matter, we construct a relativistic mean field ...
The properties of high-density nuclear and neutron matter are studied using a relativistic mean-fiel...
The equation of state (EOS) for highly compressed dense matter is one of the main concerns of nuclea...
The equation of state (EOS) for highly compressed dense matter is one of the main concerns of nuclea...
The equation of state (EOS) for highly compressed dense matter is one of the main concerns of nuclea...
Nuclear matter properties are calculated in the relativistic mean-held theory by using a number of d...
Nuclear matter properties are calculated in the relativistic mean-field theory by using a number of ...
It is shown that the equation of state of nuclear matter can be determined within the mean-field the...
The authors formulate a phenomenological extension of the mean-field theory approach and define a cl...
The relativistic mean-field plus random phase and quasiparticle random phase approximation calculati...
The relativistic mean-field plus random phase and quasiparticle random phase approximation calculati...
The parameters of the sigma-omega-rho model in the relativistic mean-field theory with nonlinear a-m...
We have determined the equation of state of nuclear matter according to relativistic non-linear mode...
We have determined the equation of state of nuclear matter according to relativistic non-linear mode...
International audienceWe have determined the equation of state of nuclear matter according to relati...
In order to predict properties of asymmetric nuclear matter, we construct a relativistic mean field ...
The properties of high-density nuclear and neutron matter are studied using a relativistic mean-fiel...
The equation of state (EOS) for highly compressed dense matter is one of the main concerns of nuclea...
The equation of state (EOS) for highly compressed dense matter is one of the main concerns of nuclea...
The equation of state (EOS) for highly compressed dense matter is one of the main concerns of nuclea...
Nuclear matter properties are calculated in the relativistic mean-held theory by using a number of d...
Nuclear matter properties are calculated in the relativistic mean-field theory by using a number of ...
It is shown that the equation of state of nuclear matter can be determined within the mean-field the...
The authors formulate a phenomenological extension of the mean-field theory approach and define a cl...
The relativistic mean-field plus random phase and quasiparticle random phase approximation calculati...
The relativistic mean-field plus random phase and quasiparticle random phase approximation calculati...
The parameters of the sigma-omega-rho model in the relativistic mean-field theory with nonlinear a-m...
We have determined the equation of state of nuclear matter according to relativistic non-linear mode...
We have determined the equation of state of nuclear matter according to relativistic non-linear mode...
International audienceWe have determined the equation of state of nuclear matter according to relati...
In order to predict properties of asymmetric nuclear matter, we construct a relativistic mean field ...