1995/10/26 by Richhild Moessner, R. Moessner, R. Brandenberger +1 · 1 citation
Physics and Astronomy · #Accretion (finance) #Astronomy #Astrophysics #COSMIC cancer database #Cold dark matter #Cosmic string #Cosmology #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Dark energy #Dark matter #Galaxies: Formation, Evolution, Phenomena #Galaxy #Hot dark matter #Physics #Quasar #Redshift #Scalar field dark matter #String (physics) #String theory #Structure formation #Theoretical physics #astro-ph
paper · pdf · doi:10.1093/mnras/280.3.797
published as Mon.Not.Roy.Astron.Soc.280:797,1996 · 21 pages, 1 figure, uses phyzzx and epsf macros
arxiv created 1995/10/26 · openalex publication_date 1996/06/01 · arxiv updated 2015/06/24 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Using a modification of the Zel'dovich approximation adapted to hot dark matter (HDM), the accretion of such matter on to moving cosmic string loops is studied. It is shown that a large number of 1012-M⊙ non-linear objects will be produced by a redshift of z = 4. These objects could be the hosts of high-redshift quasars.