Dublin Core The Dublin Core metadata element set is common to all Omeka records, including items, files, and collections. For more information see, http://dublincore.org/documents/dces/. Title A name given to the resource Articles Article Faculty Publications -Articles Dublin Core The Dublin Core metadata element set is common to all Omeka records, including items, files, and collections. For more information see, http://dublincore.org/documents/dces/. Title A name given to the resource Evolution of primordial dark matter planets in the early Universe Subject The topic of the resource Dark matter; DM planets; Early Universe Description An account of the resource In a recent paper we had discussed possibility of DM at high redshifts forming primordial planets composed entirely of DM to be one of the reasons for not detecting DM (as the flux of ambient DM particles would be consequently reduced). In this paper we discuss the evolution of these DM objects as the Universe expands. As Universe expands there will be accretion of DM, helium and hydrogen layers (discussed in detail) on these objects. As they accumulate more and more mass, the layers get heated up leading to nuclear reactions which burn H and He when a critical thickness is reached. In the case of heavier masses of these DM objects, matter can be ejected explosively. It is found that the time scale of ejection is smaller than those from other compact objects like neutron stars (that lead to x-ray bursts). These flashes of energy could be a possible observational signature for these dense DM objects. 2021 COSPAR Creator An entity primarily responsible for making the resource Kiren O.V.; Arun K.; Sivaram C. Source A related resource from which the described resource is derived Advances in Space Research, Vol-68, No. 4, pp. 2050-2056. Publisher An entity responsible for making the resource available Elsevier Ltd Date A point or period of time associated with an event in the lifecycle of the resource 2021-01-01 Identifier An unambiguous reference to the resource within a given context <a href="https://doi.org/10.1016/j.asr.2021.04.016" target="_blank" rel="noreferrer noopener">https://doi.org/10.1016/j.asr.2021.04.016</a> <br /><br /><a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85105337124&amp;doi=10.1016%2Fj.asr.2021.04.016&amp;partnerID=40&amp;md5=1b52e3e202d726827bd8085144a8945e" target="_blank" rel="noreferrer noopener">https://www.scopus.com/inward/record.uri?eid=2-s2.0-85105337124&amp;doi=10.1016%2fj.asr.2021.04.016&amp;partnerID=40&amp;md5=1b52e3e202d726827bd8085144a8945e</a> Rights Information about rights held in and over the resource All Open Access; Green Open Access Relation A related resource ISSN: 2731177; CODEN: ASRSD Format The file format, physical medium, or dimensions of the resource Online Language A language of the resource English Type The nature or genre of the resource Article Coverage The spatial or temporal topic of the resource, the spatial applicability of the resource, or the jurisdiction under which the resource is relevant Kiren O.V., Department of Physics and Electronics, CHRIST (Deemed to be University), Bengaluru, 560029, India; Arun K., Department of Physics and Electronics, CHRIST (Deemed to be University), Bengaluru, 560029, India, Christ Junior College, Bangalore, 560 029, India; Sivaram C., Indian Institute of Astrophysics, Bangalore, 560 034, India