The Axion Quark Nugget Dark Matter Model: Size Distribution and Survival
  Pattern
  We consider the formation and evolution of Axion Quark Nugget dark matter
particles in the early universe. The goal of this work is to estimate the mass
distribution of these objects and assess their ability to form and survive to
the present day. We argue that this model allows a broad range of parameter
space in which the AQN may account for the observed dark matter mass density,
naturally explains a similarity between the "dark" and "visible" components,
i.e. $\Omega_{\rm dark}\sim \Omega_{\rm visible}$, and also offer an
explanation for a number of other long standing puzzles such as "Primordial
Lithium Puzzle" and "the Solar Corona Mystery" among many other cosmological
puzzles.
