Late D-term Inflation and the Cosmological Moduli Problem in TeV Scale Strings

Preprint

5 July 1999

preprint
Published by arXiv in arXiv

Abstract

We show that a short period of late D-term inflation can solve the cosmological moduli (radion) problem of (asymmetric) inflation at the TeV scale. Late inflation happens after the large compact dimensions are stabilized which is crucial for obtaining the extremely small Hubble constant and inflaton mass required.

Keywords

COSMOLOGICAL MODULI
MODULI PROBLEM
TERM INFLATION
SMALL HUBBLE
LATE D TERM
TEV SCALE

All Related Versions

Version 1, 1999-07-05, ArXiv
Version 2, 1999-07-28, ArXiv
Published version: Journal of High Energy Physics, 1999 (09), 012.

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