G. Mustafa

The DESI survey examined the motion of galaxies and supernovae, testing the constancy of dark energy. Faint signals point to its evolution, and the Mirage model gave the best but not definitive result. If the energy is indeed growing, the Universe could face a tearing apart of matter.

Recent observations of supernovae, galaxy distribution, and the Big Bang afterglow show that dark energy density is not constant. This challenges the standard cosmological model and promises a revision of the Universe's evolution.

Analysis of galaxy maps, quasar light, and supernovae shows that the simple model of constant dark energy is losing to a version with a smoothly changing force. This needs verification, but it's intriguing.