Cosmology with dark energy decaying through its chemical-potential contribution

  • J Besprosvany
  • Published 2008


The consideration of dark energy’s quanta, required also by thermodynamics, introduces its chemical potential into the cosmological equations. Isolating its main contribution, we obtain solutions with dark energy decaying to matter or radiation. When dominant, their energy densities tend asymptotically to a constant ratio, explaining today’s dark energy… (More)


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