The Equation of State of Neutron Star Matter

Mar 24, 2014, 9:10 AM
40m

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.

Primary author

Dr Hans-Josef Schulze (INFN Sezione di Catania)

Presentation materials