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The Universal Dark Matter

2006/09/18 by R. K. Soberman, Robert K. Soberman, Soberman, Robert K. +2
Physics and Astronomy · #Astro and Planetary Science #Astrophysics (astro-ph) #FOS: Physical sciences #Space Science and Extraterrestrial Life #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/0609500

arxiv created 2006/09/18 · openalex publication_date 2006/09/18 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

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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