Early Objects in the Cosmic String Theory with Hot Dark Matter
classification
🌌 astro-ph
keywords
cosmicdarkmatterobjectsredshiftstringaccretionadaptation
read the original abstract
We study the accretion of hot dark matter onto moving cosmic string loops, using an adaptation of the Zeldovich approximation to HDM. We show that a large number of nonlinear objects of mass greater than $10^{12}M_\odot$, which could be the hosts of high redshift quasars, are formed by a redshift of $z=4$.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.