A theoretical analysis of the formation of Bose–Einstein condensates in astrophysical and cosmological settings, taking into account the effects of curved spacetime, has been carried out. Condensation conditions in extreme gravitational fields are derived, and the role of these phenomena in neutron stars, the formation of primordial black holes, and dark matter halos is explored. It is shown that the critical condensation temperature depends nontrivially on spacetime curvature: corrections of order O(GM/(rc^2)) become significant near compact objects. In particular, if dark matter consists of axions with a mass ~10^(-22) eV, it naturally forms a cosmic condensate with a coherence length of order 10^(-3) parsecs, which resolves the core-cusp problem in galaxies. These results indicate that macroscopic quantum coherence is more widespread in the universe than previously thought and has fundamental importance for structure formation and the behavior of matter under extreme conditions.
In a special quantum state — a Bose–Einstein condensate — atoms stop being 'individualists' and merge into a single quantum wave, like droplets of mercury gathering into a single ball. On Earth, this is only achieved at temperatures billionths of a degree above absolute zero. But physicists have figured out: in space, extreme gravity and the curvature of spacetime can create similar conditions without any cold, because curvature shifts the threshold at which particles 'freeze' into a common rhythm.
Calculations show that inside neutron stars and near black holes, matter naturally falls into this clumped state. And if dark matter consists of ultra-light particles — axions — then it forms giant quantum blobs throughout the Universe. This solves a long-standing puzzle: according to standard theories, dark matter should pile up at the centers of galaxies, but observations reveal a smoother distribution. Its quantum nature keeps it from clumping together.
🎯 The lowest temperature ever created by humans was achieved precisely during the formation of a Bose–Einstein condensate.