Speaker
Dr
Hans-Josef Schulze
(INFN Sezione di Catania)
Description
The main features of the EOS of neutron star matter are reviewed,
comprising nucleonic, hyperonic, and quark matter contributions.
The focus in on the Brueckner-Hartree-Fock theoretical method,
but also other approaches will be regarded.
Author
Dr
Hans-Josef Schulze
(INFN Sezione di Catania)
