In 1982 Andrei Linde proposed a working model of inflation in which the universe would gracefully exit from
the exponential expansion phase without producing unacceptable inhomogeneities.
Not exact matches
Traditionally, the growth rates of hESC colonies have been manually counted from single cell suspensions as doubling time during the
exponential growth
phase [13] or as an
expansion of the area of a single colony from microscopic images [14].
In 1980 Alexei Starobinsky independently postulated a similar early
phase of
exponential expansion, in this case driven by quantum gravity effects.