Enhancement of weak interactions in phase transitions in condensed matter and early Universe
V. V. Flambaum
APS Open Sci. 1, 000213 (2026) - Published 12 November, 2026
Parity-violating weak interactions produce extremely small energy differences between left- and right-handed chiral systems. We show that these microscopic effects may be amplified during collective phenomena such as phase transitions. The enhancement factor is proportional to the critical number of atoms, , in the nucleus of the new phase. Measurement of the ratio of produced left- and right-handed chiral structures may provide a way to determine . Experiments in which spin-chiral structures are formed in during a phase transition in crossed electric and magnetic fields indicate an effective amplification corresponding to . We emphasize, however, that such large values cannot be inferred from homogeneous capillary nucleation alone, since the same parameters imply a very large nucleation barrier; in real crystals heterogeneous nucleation, defects, strain, and domain-growth dynamics may be essential. We also discuss, more cautiously, whether analogous collective enhancement could operate in first-order cosmological phase transitions beyond the standard model. The standard-model electroweak transition for the observed Higgs mass is a crossover and therefore has no critical bubble nucleus.



