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We study the perturbed equation of state (EOS) parameters of the cosmologicaltachyonic scalar field components and their mutual time-dependent interaction.  It is shown that the discrete temperature-dependent pattern of the EOSemerges from an initial continuum along the evolution of the universe. Thisleads to two major components in form of dark energy and dark matter, and alsosuggests a solution to the cosmological constant problem and the coincidenceproblem.

Evolution of the equation of state parameters of cosmological tachyonic field components through mutual interaction