Observable Gravity Waves from Supersymmetric Hybrid Inflation II

Details Observable Gravity Waves from Supersymmetric Hybrid Inflation II Observable Gravity Waves from Supersymmetric Hybrid Inflation II

2010-12-01

arxiv.org/abs/1012.0309v1

Phys.Rev.D83:067304,2011

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

4 pages, 4 figures

Scientific paper

10.1103/PhysRevD.83.067304

It is shown that a tensor-to-scalar ratio close to r = 0.03, which can be observed by Planck, is realized in supersymmetric hybrid inflation models with TeV-scale soft supersymmetry breaking terms. This extends our previous analysis, which also found r <~ 0.03 but employed intermediate scale soft terms. Other cosmological observables such as the scalar spectral index are in good agreement with the WMAP data.

Affiliated with

Also associated with

No associations

Rating

Observable Gravity Waves from Supersymmetric Hybrid Inflation II 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 Observable Gravity Waves from Supersymmetric Hybrid Inflation II, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observable Gravity Waves from Supersymmetric Hybrid Inflation II will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-602394