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CosmoPlMeeting2006 -
CosmoPlMeeting2006Program
COSMO-PL SPRING MEETING 2006
A Big-Rip (phantom) scenario and an exotic future of the Universe.
abstract:
The recent supernovae data together with large scale structure and CMBR
observations favours the dark energy with the matter equation of state
$p< - \varrho$ which was dubbed phantom. This matter forces the universe
to inflate much faster than the cosmological constant and its
gravitational effect is first felt on larger scales which leads to the
total distraction of the bound objects in the universe from the largest to
the smallest - a Big-Rip singularity.
In my talk I will review cosmological models with a Big-Rip
singularity, the support, motivation, and their relation to superstring
and M-theory cosmology. Apart from classical scenarios, I will also discuss
quantum cosmological scenarios with phantom. I will also show other more
exotic scenarios of the future evolution of the universe and their
possible observational detection/support.