Low-momentum relativistic nucleon-nucleon potentials I: Nuclear matter

Abstract

A series of relativistic one-boson-exchange potentials for two-nucleon system, denoted as OBEP$\hat{I}›$, is constructed with a momentum cutoff $\hat{I}›$ ranging from $\infty$ to 2 fm${}^{-1}$. These potentials are developed by simultaneous fitting to nucleon-nucleon ($NN$) scattering phase shifts, low-energy scattering length, effective range, and the binding energy of the deuteron. The momentum-space matrix elements of the low-momentum OBEP$\hat{I}›$ ($\hat{I}›⩽3$ fm${}^{-1}$) demonstrate consistency with the universal behaviors observed in other realistic $NN$ potentials evolved by renormalization group methods. These OBEP$\hat{I}›$s are applied to calculate the equation of state of symmetric nuclear matter (SNM) within either the nonrelativistic (NR) Brueckner-Hartree-Fock (BHF) or relativistic Brueckner-Hartree-Fock (RBHF) frameworks. The results show that the saturation properties of SNM are reproduced qualitatively from the RBHF calculation, but not from the NR-BHF calculation. This study highlights the relativistic mechanism in explaining the saturation properties of nuclear matter. The remaining discrepancy in reproducing empirical saturation properties in the RBHF calculation using the OBEP$\hat{I}›$s signals the necessity of including three-nucleon correlations or genuine three-nucleon forces.