Cosmology from a rolling massive scalar field on the anti-D3 brane of de Sitter vacua

Garousi, Mohammad R. ; Sami, M. ; Tsujikawa, Shinji (2004) Cosmology from a rolling massive scalar field on the anti-D3 brane of de Sitter vacua Physical Review D - Particles, Fields, Gravitation and Cosmology, 70 (4). 043536. ISSN 1550-7998

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We investigate a string-inspired scenario associated with a rolling massive scalar field on D-branes and discuss its cosmological implications. In particular, we discuss cosmological evolution of the massive scalar field on the anti-D3 brane of KKLT vacua. Unlike the case of tachyon field, because of the warp factor of the anti-D3 brane, it is possible to obtain the required level of the amplitude of density perturbations. We study the spectra of scalar and tensor perturbations generated during the rolling scalar inflation and show that our scenario satisfies the observational constraint coming from the cosmic microwave background anisotropies and other observational data. We also implement the negative cosmological constant arising from the stabilization of the modulus fields in the KKLT vacua and find that this leads to a successful reheating in which the energy density of the scalar field effectively scales as a pressureless dust. The present dark energy can be also explained in our scenario provided that the potential energy of the massive rolling scalar does not exactly cancel with the amplitude of the negative cosmological constant at the potential minimum.

Item Type:Article
Source:Copyright of this article belongs to The American Physical Society.
ID Code:70529
Deposited On:18 Nov 2011 13:03
Last Modified:18 Nov 2011 13:03

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