Cosmological evolution of a brane Universe in a type 0 string background

Details Cosmological evolution of a brane Universe in a type 0 string background Cosmological evolution of a brane Universe in a type 0 string background

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aipc..607..337p&link_type=abstract

STRING THEORY; 10th Tohwa University International Symposium on String Theory. AIP Conference Proceedings, Volume 607, pp. 337-

Mathematics

Logic

Particle-Theory And Field-Theory Models Of The Early Universe, Extended Classical Solutions, Cosmic Strings, Domain Walls, Texture

Scientific paper

We study the cosmological evolution of a D3-brane Universe in a type 0 string background. We follow the brane universe along the radial coordinate of the background and we calculate the energy density which is induced on the brane because of its motion in the bulk. For constant values of tachyon and dilaton an inflationary phase is appearing. For non constant values of tachyon and dilaton and for a particular range of values of the scale factor of the brane-universe, the effective energy density is dominated by a term proportional to 1/(log α)4 indicating a slowly varying inflationary phase. .

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