Turbulence Gradients Driving Temporally Compressed Wolf Rayet Cluster Evolution

The clustered deaths of massive stars remain poorly linked to both galactic structure and planetary biospheric risk. We present a model in which an external hypernova or gamma-ray burst compresses a magnetized molecular cloud, creating a turbulence gradient that suppresses fragmentation and forces the formation of solitary Wolf-Rayet (WR) stars with aligned spins and synchronized lifetimes. These stars collapse within a narrow temporal window to produce high-fluence, unmodulated GRBs, consistent with isolated ∆¹⁴C anomalies and paleoclimatic disturbances on Earth. Because the WR progenitors inherit angular momentum aligned with the galactic magnetic field, their hypernovae launch fast, coherent relativistic jets that both reinforce spiral arm magnetism and extend plasma coupling over hundreds of light-years. This framework links star formation physics, GRB clustering, and galactic magnetic order into a predictive paradigm of astrophysical hazard.