Consequences of Accretion onto Primordial Compact Objects

Details Consequences of Accretion onto Primordial Compact Objects Consequences of Accretion onto Primordial Compact Objects

Apr 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aps..aprb14005m&link_type=abstract

American Physical Society, April Meeting, April 28 - May 1, 2001 Washington, DC Bulletin of the American Physical Society, Vol.

Physics

Scientific paper

Many lines of evidence suggest that nonbaryonic dark matter constitutes roughly 30 percent of the critical closure density, but the composition of this dark matter is unknown. One class of candidates for the dark matter is stellar-mass compact objects formed in the early universe. Specific candidates of this type include black holes formed at the epoch of the QCD phase transition, quark stars, and boson stars. We explore the effects of accretion onto these objects, and show that the resulting radiation may have significant effects on ionization (and hence on the observed CMB power spectrum) and on early structure formation. Observations of radiation from high redshifts can therefore be used to constrain the contribution of primordial compact objects to dark matter.

Affiliated with

Also associated with

No associations

Rating

Consequences of Accretion onto Primordial Compact Objects 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 Consequences of Accretion onto Primordial Compact Objects, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Consequences of Accretion onto Primordial Compact Objects will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1184099