Surface tension of strange-quark matter in the early Universe

Journal Article · Fri Sep 15 00:00:00 EDT 1989 · Physical Review (Section) D: Particles and Fields; (USA)

DOI:https://doi.org/10.1103/PhysRevD.40.2128· OSTI ID:5508966

Berger, M S ^[1]

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1. Department of Physics, University of California, Berkeley, California 94720 (US) Theoretical Physics Group, Physics Division, Lawrence Berkeley Laboratory, 1 Cyclotron Road, Berkeley, California 94720

The surface tension of strange-quark matter at finite temperature and pressure is calculated using the MIT bag model and is applied to strange-quark matter created in the QCD phase transition in the early Universe. The surface tension is sufficiently small that any strange-quark matter would have boiled away in the early Universe.

• DOE Contract Number: AC03-76SF00098
• OSTI ID: 5508966
• Journal Information: Physical Review (Section) D: Particles and Fields; (USA), Vol. 40:6; ISSN 0556-2821
• Country of Publication: United States
• Language: English

Related Subjects

71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
QUARK MATTER
SURFACE TENSION
UNIVERSE
BAG MODEL
BOUNDARY CONDITIONS
FERMI GAS
PHASE TRANSFORMATIONS
PRESSURE DEPENDENCE
QUANTUM CHROMODYNAMICS
STRANGENESS
TEMPERATURE DEPENDENCE
COMPOSITE MODELS
EXTENDED PARTICLE MODEL
FIELD THEORIES
FLUIDS
GASES
MATHEMATICAL MODELS
MATTER
PARTICLE MODELS
PARTICLE PROPERTIES
QUANTUM FIELD THEORY
QUARK MODEL
SURFACE PROPERTIES
640106* - Astrophysics & Cosmology- Cosmology