Phase transitions in cosmological models - Temperature vs. curvature

Details Phase transitions in cosmological models - Temperature vs. curvature Phase transitions in cosmological models - Temperature vs. curvature

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ncimb..58..208f&link_type=abstract

Nuovo Cimento B, Serie 11, vol. 58B, Aug. 11, 1980, p. 208-214.

Physics

1

Astronomical Models, Cosmology, Field Theory (Physics), Phase Transformations, Temperature Effects, Curvature, Euler-Lagrange Equation, High Temperature Environments, Space-Time Functions, Universe

Scientific paper

Restoration of symmetry in field theories describing the early Universe
is considered when the effects of curvature are taken into account. A
model is exhibited in which these effects compensate high-temperature
ones so as to prevent symmetry restoration.

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