Dark Energy Production by Star Formation Processes in the Observable Universe

Victor Borsevici¹ and Ion Borsevici²

¹Universitatea Libera Internationala din Moldova, Emeritus Professor, Russia
²Engineer and researcher, Russia

Abstract

The main content of the presented work is devoted to the study of the dynamics of the growth of dark energy of gravitational radiation due to intense collidings and mergers of dark matter of primordial black holes in the processes of star formation. It is shown that measurements based on the analysis of the cosmic microwave background (CMB) carry information about very early dark energy, while measurements based on the analysis of the brightness of Cepheids and Type Ia supernovae carry information about the dark energy surrounding them, including both its early component and the component associated with current star formation processes. This, in particular, removes the so-called “Hubble tension” problem, based on the unfounded belief in the constancy of dark energy, and also understands the important role played by dark matter in the star formation processes themselves. As it turns out, it is involvement of dark matter in these very important processes that significantly accelerates the formation of early galaxies, as convincingly demonstrated by sensational discoveries of James Webb telescope.

Keywords

Dark Matter, Primordial Black Holes, Dark Energy Production, Star Formation Process, “Hubble Tension” Problem, Early Galaxies

Corresponding Author

Victor Borsevici, Universitatea Libera Internationala din Moldova, Emeritus Professor, Russia.

Citation

Borsevici, V., & Borsevici, I. (2026). Dark Energy Production by Star Formation Processes in the Observable Universe. Int J Astrophys Cosmol Space Explor. 1(1), 01-11.