Kavli Affiliate: Xian Chen| Summary: Stellar trajectories around the Galactic Center provide a testing environment for general relativity. The intrinsic rotation of these stars evolves under covariant transport in curved spacetime and classical Newtonian quadrupole torques. We analyze the recently observed S301 S-star to quantify the relativistic precession of its rotational axis. Its 8.7-year period […]
Continue.. Stellar rotation of S301 as a macroscopic gyroscope to test general relativity