In medium T matrix for neutron matter
P. Bozek, P. Czerski
Abstract
We calculate the equation of state of pure neutron matter, comparing the G-matrix calculation with the in-medium T-matrix result. At low densities, we obtain similar energies per nucleon, however some differences appear at higher densities. We use the self-consistent spectral functions from the T-matrix approach to calculate the 1S0 superfluid gap including self-energy effects. We find a reduction of the superfluid gap by 30%.
Create a lesson
Related papers
Pionization experiments in light nuclei
Slawomir Wycech, Guillaume Hupin, Jaume Carbonell
Deep Learning for Longitudinal Asymmetry in Heavy-Ion Collisions at RHIC Energies
Anup Kumar Sikdar, Sanchari Thakur, Pingal Dasgupta et al.
Non-uniqueness of the amplitude reconstruction in the inverse scattering problem and a refinement of Hoehler's resonance clustering
A. Švarc
Modeling fragmentation of 20Ne nuclei at the LHC
Aleksandr Svetlichnyi, Savva Savenkov, Igor Pshenichnov
Parametrization of unitary matrices, parametrizing the symmetric S matrix and the NN S matrix above the inelastic threshold
N. A. Khokhlov
Thermofractal Dynamics in the Multisource Thermal Model: A Unified Approach to Multiparticle Production
Airton Deppman, Trambak Bhattacharyya, Maciej Rybczyński et al.