Evaporation of strange matter in the early Universe
- 15 September 1985
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 32 (6) , 1273-1279
- https://doi.org/10.1103/physrevd.32.1273
Abstract
Strange matter, a stable form of quark matter containing a large fraction of strange quarks, may have been copiously produced when the Universe had a temperature of ∼100 MeV. We study the evaporation of lumps of strange matter as the Universe cooled to 1 MeV. Only lumps with baryon number larger than ∼ could survive. This places a severe restriction on scenarios for strange-matter production.
Keywords
This publication has 14 references indexed in Scilit:
- Nuclearites—a novel form of cosmic radiationNature, 1984
- Cosmic separation of phasesPhysical Review D, 1984
- Non-Abelian gauge theories of Fermi systems: Quantum-chromodynamic theory of highly condensed matterPhysical Review D, 1978
- Quark star phenomenologyPhysical Review D, 1978
- (Non)-Abelian gauge field theories of the Fermi gas. Neutron-quark starsPhysics Letters B, 1978
- Fermions and gauge vector mesons at finite temperature and density. III. The ground-state energy of a relativistic quark gasPhysical Review D, 1977
- Fermions and gauge vector mesons at finite temperature and density. II. The ground-state energy of a relativistic electron gasPhysical Review D, 1977
- Fermions and gauge vector mesons at finite temperature and density. I. Formal techniquesPhysical Review D, 1977
- Superdense Matter: Neutrons or Asymptotically Free Quarks?Physical Review Letters, 1975
- Hydrostatic Equilibrium of Hypothetical Quark StarsProgress of Theoretical Physics, 1970