arXiv · nucl-th/9902019
Superfluid nuclear matter calculations
Abstract
We present a method to calculate nuclear matter properties in the superfluid phase. The method is based on the use of self-consistent off-shell nucleon propagators in the T-matrix equation. Such a complete treatment of the spectral function, is required below and around $T_c$ due to a pseudogap formation in the spectral function. In the superfluid phase we introduce the anomalous self-energy in the fermion propagators and in the T-matrix equation, consistently with the strong coupling BCS equations. The equations for the nucleon spectral function include both a contribution of condensed and scattering pairs. The method is illustrated by numerical calculations. Above $T_c$ pseudogap formation is visible in the spectral function and below $T_c$ a superfluid gap also appears.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
P. Bozek. 1999-06-16. Superfluid nuclear matter calculations. https://doi.org/10.1016/s0375-9474(99)00325-5
Cite the original work for its findings. Save a collection to share your selection of sources.