Berndt Müller
Published 2005-08-29, updated 2005-11-14Version 3
This is a review of the latest developments in the theory of superdense nuclear matter, formed in relativistic heavy ion collisions or in the core of collapsed stars, as they were reported and discussed at the Quark Matter 2005 conference in Budapest (Hungary).
Comments: Final version containing multiple modifications in response to comments received on the draft version
Quark Matter '99 --- Theoretical Summary: What Next?
Axial-Vector and Tensor Spin Polarization and Chiral Restoration in Quark Matter
Color Ferromagnetism in Quark Matter
