Inflation from Tachyon Condensation, Large N Effects

Details Inflation from Tachyon Condensation, Large N Effects Inflation from Tachyon Condensation, Large N Effects

2003-04-28

arxiv.org/abs/hep-th/0304226v1

Phys.Rev. D69 (2004) 103504

Physics

High Energy Physics

High Energy Physics - Theory

24 pages, 1 figure

Scientific paper

10.1103/PhysRevD.69.103504

Using only general properties of the tachyon potential we show that inflation may be generic when many branes and anti-branes become coincident. Inflation may occur because of: (1) the assistance of the many diagonal tachyon fields; (2) when the tachyons condense in a staggered fashion; or (3) when some of them condense very late. We point out that such inflation is in some sense a stringy implementation of chaotic inflation and may have important applications for ``regularizing'' a lopsided or singular cosmological compact surface.

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