Ultra-compact twin stars with hybrid equations of state from bosonic dark matter
This study demonstrates that incorporating self-interacting bosonic dark matter into hybrid equations of state with first-order phase transitions to quark matter stabilizes mass-radius configurations, eliminates the instability gap between hadronic and hybrid branches to enable continuous twin star sequences, and gives rise to two distinct classes of ultra-compact objects that can be distinguished by their surface redshifts and dark matter content.