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Radioactivity in strange quark matter
Physical Review C, 1987We develop a mass formula for finite lumps of strange quark matter near flavor equilibrium. Our Fermi-gas model includes surface tension and Coulomb energy but not quantum-chromodynamic radiative corrections. Assuming strange matter is stable in bulk, we investigate the radioactive decays of finite strangelets (clumps of strange matter with baryon ...
, Berger, , Jaffe
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The symmetry energy in nucleon and quark matter
, 2017The symmetry energy characterizes the isospin dependent part of the equation of state of isospin asymmetric strong interaction matter and it plays a critical role in many issues of nuclear physics and astrophysics.
Lie-Wen Chen
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1993
Quantum chromodynamics (QCD) was constructed as a theory of strong interactions, to provide a unique description of the experimental situation in the beginning of the 70’s. However, it was soon realized that one of the properties of QCD, asymptotic freedom1, also has quite striking consequences for the equilibrium thermodynamics of strongly interacting
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Quantum chromodynamics (QCD) was constructed as a theory of strong interactions, to provide a unique description of the experimental situation in the beginning of the 70’s. However, it was soon realized that one of the properties of QCD, asymptotic freedom1, also has quite striking consequences for the equilibrium thermodynamics of strongly interacting
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Quark Matter and Nuclear Collisions
1994I summarize briefly and qualitatively the content of my lectures. They treated on one hand quark deconfinement and its theoretical basis in finite temperature QCD, and on the other hand high energy nuclear collisions as a way to produce a deconfined state of matter in the laboratory.
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1980
We discuss the transition of strongly interacting systems from a hadronic resonance gas to a gas of quasi-free quarks. By limiting the hadron density, we obtain an equation of state which yields a quark phase at small and a hadron phase at large values of the resonance coupling constant.
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We discuss the transition of strongly interacting systems from a hadronic resonance gas to a gas of quasi-free quarks. By limiting the hadron density, we obtain an equation of state which yields a quark phase at small and a hadron phase at large values of the resonance coupling constant.
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Weyl, Dirac and high-fold chiral fermions in topological quantum matter
Nature Reviews Materials, 2021M Zahid Hasan +2 more
exaly