Toward an Effective Field Theory for Cold Compressed Baryonic Matter

Abstract

This is an extended version of the note taken by the first author (W.-G.P.) on a lecture given by the second author (M.R.) as a first part of the series on "Hadronic Matter Under Extreme Conditions," the principal theme of the WCU-Hanyang Program. It covers the attempts to go in a framework anchored on effective field theory of QCD from zero density to the nuclear matter density and slightly beyond, with the ultimate goal of arriving at the density relevant to compact stars, including chiral phase transition and quark matter. The focus is on the conceptual aspects rather than detailed "fitting" of the data on the kinds of physics that are being addressed to in radioactive-ion-beam machines in operation as well as in project (such as `KoRIA' in Korea) and will be explored at such forthcoming accelerators as FAIR/GSI. The approach presented here is basically different from the standard ones found in the literature in that the notion of hidden local symmetry -- which underlies the chiral symmetry of the strong interactions -- and its generalization to dual gravity description involving infinite tower of hidden gauge fields are closely relied on.

25 pages, 12 figures, WCU lecture note prepared for the review section of MPLA

References in corpus (7)

• The effective force NL3 revisited
• Cold, dense nuclear matter in a SU(2) parity doublet model
• Super-soft symmetry energy encountering non-Newtonian gravity in neutron stars
• Shell model description of the 14C dating beta decay with Brown-Rho-scaled NN interactions
• Nuclear matter with Brown-Rho-scaled Fermi liquid interactions
• Recent Developments on Kaon Condensation and Its Astrophysical Implications
• Kaon Condensation, Black Holes and Cosmological Natural Selection

Cited by in corpus (8)

• Entropic force, noncommutative gravity and ungravity
• Entropic force approach to noncommutative Schwarzschild black holes signals a failure of current physical ideas
• Entropic force approach in a noncommutative charged black hole and the equivalence principle
• The phase structure of a chiral model with dilatons in hot and dense matter
• Flavor Symmetry and Topology Change in Nuclear Symmetry Energy for Compact Stars
• Cold Dense Baryonic Matter and Compact Stars
• Thermodynamical features of Verlinde's approach for a non-commutative Schwarzschild-anti-deSitter black hole in a broad range of scales
• Black Hole Motion in Entropic Reformulation of General Relativity