CMB statistics in noncommutative inflation

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

9 pages, no figures

Scientific paper

10.1007/JHEP02(2011)061

Noncommutative geometry can provide effective description of physics at very short distances taking into account generic effects of quantum gravity. Inflation amplifies tiny quantum fluctuations in the early universe to macroscopic scales and may thus imprint high energy physics signatures in the cosmological perturbations that could be detected in the CMB. It is shown here that this can give rise to parity-violating modulations of the primordial spectrum and odd non-Gaussian signatures. The breaking of rotational invariance of the CMB provides constraints on the scale of noncommutativity that are competitive with the existing noncosmological bounds, and could explain the curious hemispherical asymmetry that has been claimed to be observed in the sky. This introduces also non-Gaussianity with peculiar shape- and scale-dependence, which in principle allows an independent cross-check of the presence of noncommutativity at inflation.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

CMB statistics in noncommutative 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 CMB statistics in noncommutative inflation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and CMB statistics in noncommutative inflation will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-493927

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.