The Binary Black Hole System in OJ287 and Its Connection to the Cosmological Thermosynthesis Theory

The quasar OJ287, located at approximately 5 billion light-years (redshift z ≈ 0.056), is a
unique cosmic laboratory for studying the dynamics of binary supermassive black holes
(SMBHs), with masses of 18.4 × 10ff M⊙ and 150 × 10ff M⊙, orbiting with a period of 12
years. Its luminous flares (L > 10¹² L⊙) and twisted jet ( 10 kpc, precession angle 15°) reflect
gravitational and superfluid interactions, as evidenced by recent observations (2025). This
work links OJ287 to the Cosmological Thermosynthesis Theory (CTT), a cyclic framework
unifying dark matter