Mazumdar, Anupam ; Panda, Sudhakar ; Perez-Lorenzana, Abdel (2001) Assisted inflation via tachyon condensation Nuclear Physics B, 614 (1-2). pp. 101-116. ISSN 0550-3213
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Official URL: http://www.sciencedirect.com/science/article/pii/S...
Related URL: http://dx.doi.org/10.1016/S0550-3213(01)00410-2
Abstract
In this paper we propose a new mechanism of inflating the Universe with non-BPS D4-branes which decay into stable D3-branes via tachyon condensation. In a single brane scenario the tachyon potential is very steep and unable to support inflation. However, if the universe lives in a stack of branes produced by a set of noninteracting unstable D4̃-branes, then the associated set of tachyons may drive inflation along our 3 spatial dimensions. After tachyon condensation the Universe is imagined to be filled with a set of parallel stable D3-branes. We study the scalar density perturbations and reheating within this setup.
Item Type: | Article |
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Source: | Copyright of this article belongs to Elsevier Science. |
Keywords: | Inspire: Inflation; Tachyon: Condensation; Membrane Model; Effective Action; Density; Perturbation; Numerical Calculations |
ID Code: | 109420 |
Deposited On: | 31 Jan 2018 09:35 |
Last Modified: | 31 Jan 2018 09:35 |
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