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Superdense Matter: Neutrons or Asymptotically Free Quarks?
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1975
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Superdense MatterFree Gauge TheoryNuclear PhysicsPhysicsEngineeringCosmologyNatural SciencesParticle PhysicsQuantum Field TheoryTheoretical High-energy PhysicEarly Big-bang UniverseNeutron-star CoresNon-perturbative QcdHeavy Quark PhysicDark MatterQuantum Chromodynamics
We note the following: The quark model implies that superdense matter (found in neutron-star cores, exploding black holes, and the early big-bang universe) consists of quarks rather than of hadrons. Bjorken scaling implies that the quarks interact weakly. An asymptotically free gauge theory allows realistic calculations taking full account of strong interactions.
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