CMB Angular Power Spectrum from Correlated Primordial Fluctuation

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

accepted by PRD, 5 pages, 6 figures

Scientific paper

10.1103/PhysRevD.79.043015

The usual inflationary scenario predicts a Gaussian random primordial density fluctuation, different Fourier modes of which do not correlate with each other. In this paper we propose a correlation between these different modes. A simple case is that these different Fourier modes correlate with each other following a Gaussian function. For such a primordial density fluctuation we calculate the CMB angular power spectrum and find that its amplitude decreases but the decrease is different for different $l$. This feature can be used to constrain the the correlation strength from the real data.

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 Angular Power Spectrum from Correlated Primordial Fluctuation 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 Angular Power Spectrum from Correlated Primordial Fluctuation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and CMB Angular Power Spectrum from Correlated Primordial Fluctuation will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-55245

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