Nuclear Phases, Neutron Stars and the Functional Renormalization Group
by
Prof.Wolfram Weise(ECT* Trento, Italy and TU Munich, Germany)
→
Asia/Tokyo
Room 433 in Main Research Building (RIKEN Wako)
Room 433 in Main Research Building
RIKEN Wako
Description
Nuclear Phases, Neutron Stars and the Functional Renormalization Group
Prof. Wolfram Weise
ECT* Trento, Italy and TU Munich, Germany
date: July 14, 2015, 15:30pm-
place: room 433, main research building
Abstract:
The thermodynamics of symmetric and asymmetric nuclear matter up to densities characteristic of neutron star cores is developed starting from a chiral effective Lagrangian in combination with a non-perturbative Functional Renormalization Group approach. Results are presented and discussed with focus on the following topics: nuclear liquid-gas phase transition, chiral order parameter, in-medium pion mass and the equation-of-state for neutron star matter.
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