arXiv · astro-ph/0609500
The Universal Dark Matter
Abstract
Fragile 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.
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Robert K. Soberman, Maurice Dubin. 2006-09-18. The Universal Dark Matter. https://arxiv.org/abs/astro-ph/0609500
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