TY - JOUR
T1 - Inflation in universes with a massive scalar field
AU - Piran, Tsvi
AU - Williams, Ruth M.
PY - 1985/11/28
Y1 - 1985/11/28
N2 - We discuss the evolution of toy universes coupled to a massive scalar field. Under most initial conditions such a universe enters an inflationary phase from which it emerges naturally. When the universe is anisotropic or inhomogeneous, the anisotropy or inhomogeneity freezes during the inflationary phase.
AB - We discuss the evolution of toy universes coupled to a massive scalar field. Under most initial conditions such a universe enters an inflationary phase from which it emerges naturally. When the universe is anisotropic or inhomogeneous, the anisotropy or inhomogeneity freezes during the inflationary phase.
UR - http://www.scopus.com/inward/record.url?scp=0039169246&partnerID=8YFLogxK
U2 - 10.1016/0370-2693(85)90291-6
DO - 10.1016/0370-2693(85)90291-6
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AN - SCOPUS:0039169246
SN - 0370-2693
VL - 163
SP - 331
EP - 335
JO - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
JF - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
IS - 5-6
ER -