Chiral nuclear dynamics II: from quarks to nuclei to compact stars

This is the sequel to the first volume to treat in one effective field theory framework the physics of strongly interacting matter under extreme conditions. This is vital for understanding the high temperature phenomena taking place in relativistic heavy ion collisions and in the early Universe, as...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Beteilige Person: Rho, Mannque (VerfasserIn)
Format: Elektronisch E-Book
Sprache:Englisch
Veröffentlicht: Singapore World Scientific Pub. Co. c2008
Ausgabe:2nd ed
Schlagwörter:
Links:http://www.worldscientific.com/worldscibooks/10.1142/6402#t=toc
http://www.worldscientific.com/worldscibooks/10.1142/6402#t=toc
Zusammenfassung:This is the sequel to the first volume to treat in one effective field theory framework the physics of strongly interacting matter under extreme conditions. This is vital for understanding the high temperature phenomena taking place in relativistic heavy ion collisions and in the early Universe, as well as the high-density matter predicted to be present in compact stars. The underlying thesis is that what governs hadronic properties in a heat bath and/or a dense medium is hidden local symmetry which emerges from chiral dynamics of light quark systems and from the duality between QCD in 4D and bulk gravity in 5D as in AdS/QCD. Special attention is paid to hot matter relevant for relativistic heavy ion processes and to dense matter relevant for compact stars that are either stable or on the verge of collapse into black holes
Beschreibung:"Sequel to the previous volume entitled 'Chiral nuclear dynamics' (CND-I for short) that I co-authored with Maciek Nowak and Ismail Zahed ..."--p. vii
Umfang:xix, 352 p. ill
ISBN:9812814744
9789812814746