Early Objects in the Cosmic String Theory with Hot Dark Matter

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dc.creatorMoessner, R.
dc.creatorBrandenberger, R.
dc.date1997-01-27
dc.date.accessioned2026-07-07T02:22:49Z
dc.date.available2026-07-07T02:22:49Z
dc.descriptionWe 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 $z=4$.
dc.description9 pages, includes 1 figure, uses Latex, psfig macro. To appear in Proceedings of the Workshop on `Cosmology at High and Low Redshifts', Hangzhou, China, October 1996
dc.identifierhttps://arxiv.org/abs/astro-ph/9701208
dc.identifierhttp://arxiv.org/abs/astro-ph/9701208
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11015
dc.subjectAstrophysics
dc.titleEarly Objects in the Cosmic String Theory with Hot Dark Matter
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