{ "id": "nucl-th/0202005", "version": "v3", "published": "2002-02-01T12:45:25.000Z", "updated": "2002-07-17T17:07:55.000Z", "title": "Chiral dynamics of nuclear matter at finite temperature", "authors": [ "S. Fritsch", "N. Kaiser", "W. Weise" ], "comment": "10 pages, 4 figures, submitted to Physics Letters B", "journal": "Phys.Lett. B545 (2002) 73-81", "doi": "10.1016/S0370-2693(02)02559-5", "categories": [ "nucl-th" ], "abstract": "We extend a recent three-loop calculation of nuclear matter in the systematic framework of chiral perturbation theory to finite temperatures T. The contributions from one- and two-pion exchange diagrams which cause nuclear binding and saturation at T=0 are included for T>0 in the density and temperature dependent free energy per particle, $\\bar F(rho,T)$. The so-called anomalous 2pi-exchange contribution $\\bar A(rho,T)$ (with no counterpart in the ground state energy density at T=0) is consistently included. The calculated pressure isotherms display the familiar first-order liquid-gas phase transition of isospin symmetric nuclear matter with a critical point at T_c = 25.5 MeV and rho_c = 0.09 fm^{-3}. The too high value of the critical temperature originates from the strong momentum dependence of the underlying single-particle potential U(p,k_{f0}) near the Fermi-surface. We also consider pure neutron matter at T>0 in the same framework and find fair agreement with sophisticated many-body calculations for neutron densities rho_n < 0.2 fm^{-3}.", "revisions": [ { "version": "v3", "updated": "2002-07-17T17:07:55.000Z" } ], "analyses": { "subjects": [ "12.38.Bx", "21.65.+f" ], "keywords": [ "finite temperature", "chiral dynamics", "familiar first-order liquid-gas phase transition", "temperature dependent free energy", "ground state energy density" ], "tags": [ "journal article" ], "note": { "typesetting": "TeX", "pages": 10, "language": "en", "license": "arXiv", "status": "editable", "inspire": 582513 } } }