English

Assisted inflation via tachyon condensation

High Energy Physics - Phenomenology 2009-11-07 v2 Astrophysics General Relativity and Quantum Cosmology High Energy Physics - Theory

Abstract

In this paper we propose a new mechanism of inflating the Universe with non-BPS D4D4 branes which decay into stable D3D3 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 non-interacting unstable D4~\tilde {D4} 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 D3D3 branes. We study the scalar density perturbations and reheating within this setup.

Keywords

Cite

@article{arxiv.hep-ph/0107058,
  title  = {Assisted inflation via tachyon condensation},
  author = {Anupam Mazumdar and Sudhakar Panda and Abdel Pérez-Lorenzana},
  journal= {arXiv preprint arXiv:hep-ph/0107058},
  year   = {2009}
}

Comments

LaTeX file, 10 pages, three figures included. Minor changes, small clarification added in section II. Final version

R2 v1 2026-07-22T13:35:01.374Z