Cosmic phase transitions
Copyright policy )Cosmic phase transitions
AbstractThe sequence of phase transitions during the hot history of the universe is followed within a phenomenological framework. Particular emphasis is put on the QCD confinement transition, which is at reach under earth laboratory conditions. A tepid inflationary scenario on the GUT scale with bubble growth at moderate supercooling is discussed.
deconfinement, Nuclear Theory, cosmic phase transitions, Astrophysics (astro-ph), FOS: Physical sciences, Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.), Astrophysics, universe, Nuclear Theory (nucl-th), inflation, inflationary scenario, Relativistic cosmology
deconfinement, Nuclear Theory, cosmic phase transitions, Astrophysics (astro-ph), FOS: Physical sciences, Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.), Astrophysics, universe, Nuclear Theory (nucl-th), inflation, inflationary scenario, Relativistic cosmology
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