Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aps..apr.y6002g&link_type=abstract
American Physical Society, April Meeting, Jointly Sponsored with the High Energy Astrophysics Division (HEAD) of the American As
Astronomy and Astrophysics
Astrophysics
Scientific paper
The Hot Big Bang plus inflation is the standard model of the early universe. I will present a new cosmological model which uses the observed cosmic dark energy as initial conditions for an inflationary phase which mimics a Hot Big Bang. This inflationary phase (dubbed rejuvenation) will be produced if the effective cosmological constant increases with time. The universe undergoes superexponential expansion until it resumes radiation domination, leaving it identical to a Hot Big Bang in all measurable respects but avoiding an initial singularity. This process can produce adiabatic density perturbations as favored by recent observations of Cosmic Microwave Background anisotropy, although a blue tilt to the primordial power spectrum is predicted.
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