3 research outputs found
Cosmological stabilization of moduli with steep potentials
A scenario which overcomes the well-known cosmological overshoot problem
associated with stabilizing moduli with steep potentials in string theory is
proposed. Our proposal relies on the fact that moduli potentials are very steep
and that generically their kinetic energy quickly becomes dominant. However,
moduli kinetic energy red-shifts faster than other sources when the universe
expands. So, if any additional sources are present, even in very small amounts,
they will inevitably become dominant. We show that in this case cosmic friction
allows the dissipation of the large amount of moduli kinetic energy that is
required for the field to be able to find an extremely shallow minimum. We
present the idea using analytic methods and verify with some numerical
examples.Comment: 15 pages, 5 figure
Maximal Temperature in Flux Compactifications
Thermal corrections have an important effect on moduli stabilization leading
to the existence of a maximal temperature, beyond which the compact dimensions
decompactify. In this note, we discuss generality of our earlier analysis and
apply it to the case of flux compactifications. The maximal temperature is
again found to be controlled by the supersymmetry breaking scale, T_{crit} \sim
\sqrt{m_{3/2} M_P}.Comment: 10 pages, 10 figures. v2:comment and references adde
Creation of a Compact Topologically Nontrivial Inflationary Universe
If inflation can occur only at the energy density V much smaller than the
Planck density, which is the case for many inflationary models based on string
theory, then the probability of quantum creation of a closed or an infinitely
large open inflationary universe is exponentially suppressed for all known
choices of the wave function of the universe. Meanwhile under certain
conditions there is no exponential suppression for creation of topologically
nontrivial compact flat or open inflationary universes. This suggests, contrary
to the standard textbook lore, that compact flat or open universes with
nontrivial topology should be considered a rule rather than an exception.Comment: 9 pages 2 figures, new materials and references adde