Dolgov, A.D (1997) The Problem of Vacuum Energy and Cosmology. In: De Vega, H. and Sanchez, N., eds., Fourth Paris Cosmology Colloquium: Phase Transitions in Cosmology EuroConference: Within the International School of Astrophysics “Daniel Chalonge”, World Scientific Publishing Company, Singapore, 161-195.

has been cited by the following article:

• TITLE: Using “Particle Density” of “Graviton Gas”, to Obtain Value of Cosmological Constant

  AUTHORS: Andrew Beckwith

  KEYWORDS: Graviton Gas, Partition Function, Modified HUP, Symmetry Breaking Potential

  JOURNAL NAME: Journal of High Energy Physics, Gravitation and Cosmology, Vol.9 No.1, January 17, 2023

  ABSTRACT: We use the work of de Vega, Sanchez, and Comes (1997), to approximate the “particle density” of a “graviton gas”. This “particle density” derivation is compared with Dolgov’s (1997) expression of the Vacuum energy in terms of a phase transition. The idea is to have a quartic potential, and then to utilize the Bogomol’nyi inequality to refine what the phase transition states. We utilize Ng, Infinite quantum information procedures to link our work with initial entropy and other issues and close with a variation in the HUP: at the start of the expansion of the universe.