Initial conditions of a stringy universe

Details Initial conditions of a stringy universe Initial conditions of a stringy universe

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988phrvd..38.2951g&link_type=abstract

Physical Review D (Particles and Fields), Volume 38, Issue 10, 15 November 1988, pp.2951-2957

Physics

3

Origin And Formation Of The Universe

Scientific paper

The ground-state functional corresponding to a closed bosonic string is derived by using the path-integral approach for the simple compact topology of a finite cylinder. This functional integral satisfies the ``no boundary'' Hartle-Hawking prescription and, therefore, we consider it as a candidate to describe the quantum state of the very early Universe. In light of this result and some thermodynamical considerations, the initial conditions of a stringy universe and its low-energy limit are discussed.

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