The study examines FRB characteristics through Global Complexity–Stability Theory, suggesting new detection methods.
Fast Radio Bursts (FRBs) are millisecond-duration, extragalactic radio pulses with isotropic-equivalent energies of 10³⁹–10⁴³ erg, brightness temperatures T_b > 10³⁵ K, and a wide range of spectral and temporal behaviors including downward frequency drift (“sad trombone” effect) and both repeating and one-off sources. Global Complexity–Stability Theory (GCST) interprets FRBs as localized Rate-Induced Collapse (R-collapse) events: rapid transitions where the complexity growth rate α catastrophically exceeds local recovery capacity γ, forcing explosive release of accumulated structural debt D as coherent broadband radio emission. The core GCST stability condition is During an FRB, G drops below 0.1 on millisecond timescales → coherent radiation with extreme brightness. GCST naturally explains the downward frequency drift as propagation of the R-collapse front into lower-density regions, and predicts that single (catastrophic) FRBs may be accompanied by gravitational-wave bursts detectable by LIGO/Virgo/KAGRA — providing a potential “gold standard” multi-messenger signature.
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Roman Lukin (2026) studied this question.
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