Inflation in quantum cosmology in higher dimensions

Details Inflation in quantum cosmology in higher dimensions Inflation in quantum cosmology in higher dimensions

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986phrvd..33.2164o&link_type=abstract

Physical Review D (Particles and Fields), Volume 33, Issue 8, 15 April 1986, pp.2164-2174

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Field Theories In Dimensions Other Than Four, Particle-Theory And Field-Theory Models Of The Early Universe

Scientific paper

Quantum cosmology in Kaluza-Klein-type theories is investigated by using the fundamental equation of quantum gravity: the Wheeler-DeWitt equation. The Casimir stress tensor is considered as a prime source of compactification. By imposing the Hartle-Hawking boundary condition, we demonstrate that a fine-tuning of the boundary condition in the quantum regime is necessary, presumably at a moderate level of 10-3, in order to obtain a sufficient inflation of our space.

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