Some remarks on the problem of very early universe

The roles of singularities in a perpetually oscillating universe are discussed. The work focuses on the arbitrary character of interpretations available to earliest epochs of the universe. The universe would have started at a singularity and is expanding with a total mass equal to a black hole that acts as a stable particle. After maximum expansion the universe will recollapse until the mass density attains a quantum value. At that point the presence of asymptotic freedom of gravitational interactions will result in further contractions and mass loss. It will eventually end in a de Sitter phase with Planck dimensions and have an entropy value that is the same as at all other times that stage is reached.