Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7483
Title: Primordial planets predominantly of dark Matter
Authors: Sivaram, C
Arun, K
Kiren, O. V
Keywords: Dark matter;Primordial planets;DM planets
Issue Date: May-2019
Publisher: Springer
Citation: Earth, Moon, and Planets, Vol.122, No.3-4, pp.115-119
Abstract: Cosmic structure formation is thought to occur as a bottom-up scenario, i.e. the lightest objects would have formed first. It has been suggested that the earliest structures to form could have been primordial planets. Here we propose the possibility of formation of primordial planets at high redshifts composed predominantly of dark matter (DM) particles, with planetary masses ranging from Neptune mass to asteroid mass. Most of these primordial DM planets could be free floating without being attached to a host star and a substantial fraction could be present in the halo contributing to the DM. Here we suggest that the flux of DM particles could be significantly reduced as substantial number of DM particles are now trapped in such objects, perhaps accounting for the negative results seen so far in the ongoing DM detection experiments.
Description: Restricted Access
The original publication is available at springerlink.com
URI: http://hdl.handle.net/2248/7483
ISSN: 1573-0794
???metadata.dc.rights???: © Springer
???metadata.dc.relation.uri???: https://doi.org/10.1007/s11038-019-09525-4
Appears in Collections:IIAP Publications

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