Hot neutron matter from a Self-Consistent Green's Functions approach

(2) Departament d'Estructura i Constituents de la Mat\`eria; A. Polls (2); A. Rios (1); Astronomy; Department of Physics; Institut de Ci\`encies del Cosmos; I. Vida\~na (2) ((1) National Superconducting Cyclotron Laboratory; Michigan State University; Spain); Universitat de Barcelona

arxiv: 0809.1467 · v1 · submitted 2008-09-09 · ⚛️ nucl-th

Hot neutron matter from a Self-Consistent Green's Functions approach

A. Rios (1) , A. Polls (2) , I. Vida\~na (2) ((1) National Superconducting Cyclotron Laboratory , Department of Physics , Astronomy , Michigan State University , USA , (2) Departament d'Estructura i Constituents de la Mat\`eria

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Institut de Ci\`encies del Cosmos Universitat de Barcelona Spain)

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A systematic study of the microscopic and thermodynamical properties of pure neutron matter at finite temperature within the Self-Consistent Green's Function approach is performed. The model dependence of these results is analyzed by both comparing the results obtained with two different microscopic interactions, the CD-BONN and the Argonne V18 potentials, and by analyzing the results obtained with other approaches, such as the Brueckner--Hartree--Fock approximation, the variational approach and the virial expansion.

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Hot neutron matter from a Self-Consistent Green's Functions approach

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