Why the dark matter of galaxies is clumps of micro-brown-dwarfs and not Cold Dark Matter
Carl H. Gibson (University of California at San Diego, USA)

TL;DR
The paper argues that galaxy dark matter consists of micro-brown-dwarfs in proto-globular-star-clusters, challenging the cold dark matter paradigm and explaining observed microlensing and void phenomena.
Contribution
It proposes a new baryonic dark matter model based on primordial hydrogen-helium planets and criticizes cold dark matter theory using observational evidence.
Findings
Microlensing observations support baryonic micro-brown-dwarfs as dark matter.
Void sizes correspond to early universe sonic expansion speeds.
Cold dark matter is inconsistent with satellite galaxy observations.
Abstract
Observations of quasar microlensing by Schild 1996 show the baryonic dark matter BDM of galaxies is micro-brown-dwarfs, primordial hydrogen-helium planets formed at the plasma to gas transition 10^13 seconds, in trillion-planet clumps termed proto-globular-star-clusters PGCs. Large photon-viscosity {\nu} of the plasma permits supercluster-mass gravitational fragmentation at 10^12 seconds when the horizon scale L_H = ct is matched by the Schwarz viscous scale L_SV of Gibson 1996. Voids begin expansion at sonic speeds c/ 3^1/2, where c is light speed and t is time, explaining 10^25 meter size regions observed to be devoid of all matter, either BDM or non-baryonic NBDM. Most of the NBDM is weakly-collisional, strongly-diffusive, neutrino-like particles. If cold NBDM (CDM) is assumed, it must soon become warm and diffuse because it is weakly-collisional. It cannot clump and its clumps…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Stellar, planetary, and galactic studies · Astronomy and Astrophysical Research
