Nonrelativistic nucleon effective masses in nuclear matter: BHF versus RHF

preprint2016arXivOpen access

Abstract

The density and isospin dependences of the nonrelativistic nucleon effective mass (m∗m^*) are studied, which is a measure of the nonlocality of the single particle (s.p.) potential. We decouple it further into the so called k-mass (mk∗m^*_k, i.e., the nonlocality in space) and E-mass (mE∗m^*_E, i.e., the nonlocality in time). Both masses are determined and compared from the latest versions of the nonrelativistic Brueckner-Hartree Fock (BHF) model and the relativistic Hartree-Fock (RHF) model. The latter are achieved based on the corresponding Schrödinger equivalent s.p. potential in a relativistic framework. We demonstrate the origins of different effective masses and discuss also their neutron-proton splitting in the asymmetric matter in different models. We find that the neutron-proton splittings of both the k-mass and the E-mass have the same asymmetry dependences at considered densities, namely mk,n∗>mk,p∗m^*_{k,n} > m^*_{k,p} and mE,p∗>mE,n∗m^*_{E,p} > m^*_{E,n}. However, the resulting splittings of nucleon effective masses could have different asymmetry dependences in the two models, because they could be dominated either by that of the k-mass (then we have mn∗>mp∗m^*_n > m^*_p in the BHF model) or by that of the E-mass (then we have mp∗>mn∗m^*_p > m^*_n in the RHF model).

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