Structure formation from power law (and extended) inflation

Details Structure formation from power law (and extended) inflation Structure formation from power law (and extended) inflation

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phlb..279..244l&link_type=abstract

Physics Letters B, Volume 279, Issue 3-4, p. 244-249.

Physics

43

Scientific paper

In models of inflation where the expansion rate is slower than exponential, scale invariance is broken and the primeval density spectrum is no longer flat. We consider power law inflation models (of which extended inflation provides a specific example) where the scale factor increases like a power p of the time. They give a spectrum which increases like a power 2/(p - 1) of the scale. A power p ~ 5 in a cold dark matter universe can explain recent observations of the galaxy angular correlation function without violating published limits on the microwave anisotropy. The formation of nonlinear structure occurs more recently than in standard CDM. One can calculate the inflationary energy scale, which is much lower than the energy scale of structure forming topological defects.

Affiliated with

Also associated with

No associations

Rating

Structure formation from power law (and extended) inflation 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 Structure formation from power law (and extended) inflation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Structure formation from power law (and extended) inflation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1739891