The Universal Dark Matter

Simple item page
dc.creatorSoberman, Robert K.
dc.creatorDubin, Maurice
dc.date2006-09-18
dc.date.accessioned2026-07-07T07:23:16Z
dc.date.available2026-07-07T07:23:16Z
dc.descriptionFragile volatile aggregates with extremely low albedo, gravitationally drawn into the solar system are likely from the dark matter dominating the universal mass. Characteristics of this meteoric population permitted avoiding detection through a half-century's search. Measurements from space probes and in the upper atmosphere prove their existence and confirm their elusive properties.
dc.identifierhttps://arxiv.org/abs/astro-ph/0609500
dc.identifierhttp://arxiv.org/abs/astro-ph/0609500
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/115920
dc.subjectAstrophysics
dc.titleThe Universal Dark Matter
dc.typetext

Files

Collections

arXiv