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

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

1999-07-05

arxiv.org/abs/hep-ph/9907223v2

JHEP 9909:012,1999

Physics

High Energy Physics

High Energy Physics - Phenomenology

12 pages in phyzzx.tex, one reference added

Scientific paper

10.1088/1126-6708/1999/09/012

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.

Affiliated with

Also associated with

No associations

Rating

Late D-term Inflation and the Cosmological Moduli Problem in TeV Scale Strings does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Late D-term Inflation and the Cosmological Moduli Problem in TeV Scale Strings, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Late D-term Inflation and the Cosmological Moduli Problem in TeV Scale Strings will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-31054