Another Look at Gaussian Isocurvature Hot Dark Matter Models For Large- Scale Structure

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

29 pps. compressed postscritp; figures included

Scientific paper

10.1086/177344

We examine Gaussian isocurvature hot dark matter (massive neutrino) models for large-scale structure in which the initial density perturbations are produced in the baryons with a power--law spectrum $P_B(k) = Ak^{n_B}$. We calculate the linearly-evolved power spectrum and cosmic microwave fluctuations. We find that models with only isocurvature perturbations are inconsistent with observations of damped Ly$\alpha$ systems and COBE constraints on the power index. However, models which contain a mixture of adiabatic and isocurvature perturbations can be made consistent with COBE, galaxy surveys and damped Ly$\alpha$ systems.Isocurvature hot dark matter models also produce a bias between baryons and neutrinos even in the linear regime. We find that this ``natural bias'' can increase the baryon fraction in small scale objects like damped Ly$\alpha$ systems, but it has no effect on cluster scales.

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

Another Look at Gaussian Isocurvature Hot Dark Matter Models For Large- Scale Structure 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 Another Look at Gaussian Isocurvature Hot Dark Matter Models For Large- Scale Structure, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Another Look at Gaussian Isocurvature Hot Dark Matter Models For Large- Scale Structure will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-158454

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