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Fluctuations of the Gravitational Constant in the Inflationary Brans-Dicke Cosmology
Juan Garcia-Bellido, Andrei Linde, Dmitri Linde
According to the Brans--Dicke theory, the value of the gravitational constant G which we measure at present is determined by the value of the Brans--Dicke scalar field ϕat the end…
Comments on Inflationary Cosmology
Andrei Linde
In this talk we discuss three different issues. First of all, there exist several proposals how to solve cosmological problems by adiabatic expansion of the Universe, without any u…
Hybrid Inflation
Andrei Linde
Usually inflation ends either by a slow rolling of the inflaton field, which gradually becomes faster and faster, or by a first-order phase transition. We describe a model where in…
From the Big Bang Theory to the Theory of a Stationary Universe
Andrei Linde, Dmitri Linde, Arthur Mezhlumian
We consider chaotic inflation in the theories with the effective potentials phi^n and e^{αϕ}. In such theories inflationary domains containing sufficiently large and homogeneous sc…
Stationary Universe
Andrei Linde, Arthur Mezhlumian
If the Universe contains at least one inflationary domain with a sufficiently large and homogeneous scalar field, then this domain permanently produces new inflationary domains of…