Initial conditions for the Starobinsky model in a nonminimal-coupling-type theory

Details Initial conditions for the Starobinsky model in a nonminimal-coupling-type theory Initial conditions for the Starobinsky model in a nonminimal-coupling-type theory

Oct 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995phrvd..52.4349c&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 52, Issue 8, 15 October 1995, pp.4349-4360

Mathematics

Probability

4

Origin And Formation Of The Universe, Gravity In More Than Four Dimensions, Kaluza-Klein Theory, Unified Field Theories, Alternative Theories Of Gravity

Scientific paper

We study the classical and quantum Starobinsky model in a Jordan-Brans-Dicke-type theory. At the classical level we describe inflationary attractors. Expressions for the density perturbations and initial amplitudes for gravitational waves are obtained. At the quantum level, the Hartle-Hawking and the tunneling boundary conditions for the wave function of the Universe are determined. These wave functions are used for determining probability distributions for the initial state of the model.

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