Nonsingular cosmological models: the massive scalar field case

[1]  B. Sathyaprakash,et al.  Phase transitions and gravity , 1984 .

[2]  Andrei Linde,et al.  The inflationary Universe , 1984 .

[3]  D. Page.  A fractal set of perpetually bouncing universe , 1984 .

[4]  T. Padmanabhan,et al.  Quantum cosmology via path integrals , 1983 .

[5]  Alexander Vilenkin,et al.  Creation of Universes from Nothing , 1982 .

[6]  Andrei Linde,et al.  A new inflationary universe scenario: A possible solution of the horizon , 1982 .

[7]  L. Abbott.  Gravitational effects on the SU(5) breaking phase transition for a Coleman-Weinberg potential , 1981 .

[8]  H. Fleming,et al.  Phase transitions in cosmological models: Temperature vs. curvature , 1980 .

[9]  Andrei Linde.  Gauge theories, time-dependence of the gravitational constant and antigravity in the early universe , 1980 .

[10]  A. Zee.  Horizon problem and the broken-symmetric theory of gravity , 1980 .

[11]  G. Senjanovic,et al.  SoftCP-Invariance Violation at High Temperature , 1979 .

[12]  Andrei Linde.  Phase transitions in gauge theories and cosmology , 1979 .

[13]  George F. R. Ellis,et al.  The Large Scale Structure of Space-Time , 2023 .

[14]  D. W. Thomas,et al.  Correlations in the Two-Particle Inclusive Reactions π ± + p → π − + π − + Anything , 1972 .

[15]  C. Callan,et al.  A new improved energy-momentum tensor , 1970 .

[16]  R. Penrose,et al.  The singularities of gravitational collapse and cosmology , 1970, Proceedings of the Royal Society of London. A. Mathematical and Physical Sciences.

[17]  F. Hoyle,et al.  A new theory of gravitation , 1964, Proceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences.