Identifying Dark Matter Through the Constraints Imposed by Fourteen Astronomically Based 'Cosmic Constituents'

Abstract

Mankind has not yet explained dark matter, the accelerating expansion of the Universe, the 'knee' and 'ankle' of the cosmic ray energy spectrum graph, the low star formation rates of low surface brightness (LSB) dwarf galaxies, the ignition of hydrogen fusion reactions in the first generation stars or the departing locations of earthbound high-energy cosmic ray protons. A new research hypothesis has been developed by the author based upon finding astronomically based 'cosmic constituents' of the Universe that may be created or influenced by or have a special relationship with possible dark matter candidates. A list of 14 relevant and plausible 'cosmic constituents' of the Universe was developed by the author, which was then used to establish a list of constraints regarding the nature and characteristics of the long-sought dark matter particles. A dark matter candidate was then found that best conformed to the 14 constraints established by the 'cosmic constituents.'