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THE CONDENSED MATTER PHYSICS OF QCD

2000/11/30 by Krishna Rajagopal, Frank Wilczek · 17 citations
Earth and Planetary Sciences · Physics and Astronomy · #Asymptotic freedom #Chiral symmetry #Coupling (piping) #Dense matter #Hadron #High-Energy Particle Collisions Research #High-pressure geophysics and materials #Neutron star #Particle physics #Phase (matter) #Phase diagram #Physics #QCD matter #Quantum Chromodynamics and Particle Interactions #Quantum chromodynamics #Quantum mechanics #Strange matter #Theoretical physics #astro-ph #cond-mat #hep-ph #hep-th #nucl-th

paper · pdf · doi:10.1142/9789812810458_0043

91 pages. latex with sprocl.sty. 6 eps figures. To appear as Chapter 35 in the Festschrift in honor of B. L. Ioffe, "At the Frontier of Particle Physics / Handbook of QCD", M. Shifman, ed., (World Scientific). v2: References corrected

arxiv created 2000/12/13 · openalex publication_date 2001/04/01 · arxiv updated 2016/11/23 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Important progress in understanding the behavior of hadronic matter at high density has been achieved recently, by adapting the techniques of condensed matter theory. At asymptotic densities, the combination of asymptotic freedom and BCS theory make a rigorous analysis possible. New phases of matter with remarkable properties are predicted. They provide a theoretical laboratory within which chiral symmetry breaking and confinement can be studied at weak coupling. They may also play a role in the description of neutron star interiors. We discuss the phase diagram of QCD as a function of temperature and density, and close with a look at possible astrophysical signatures.

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