Probing departures from Schwarzschild geometry with the S301 star and kilometre-baseline interferometry
astro-ph.GA, gr-qc
Submitted: 2026-10-05
Updated: 2026-10-05
Sources
- Measuring Distance and Properties of the Milky Way's Central Supermassive Black Hole with Stellar Orbits
- Monitoring stellar orbits around the Massive Black Hole in the Galactic Center
- Detection of the gravitational redshift in the orbit of the star S2 near the Galactic centre massive black hole
- Relativistic redshift of the star S0-2 orbiting the Galactic center supermassive black hole
- Detection of the Schwarzschild precession in the orbit of the star S2 near the Galactic centre massive black hole
- Improved GRAVITY astrometric accuracy from modeling of optical aberrations
- The mass distribution in the Galactic Centre from interferometric astrometry of multiple stellar orbits
- Improving constraints on the extended mass distribution in the Galactic Center with stellar orbits
- What stellar orbit is needed to measure the spin of the Galactic center black hole from astrometric data?
- Orbital precession of stars in the Galactic center
- Bounding the mass of ultralight bosonic Dark Matter particles with the motion of the S2 star around Sgr A*
- Using the motion of S2 to constrain scalar clouds around SgrA*
- Scalar field effects on the orbit of S2 star
- The Galactic Center as a laboratory for theories of gravity and dark matter
- Discovery of a star sensitive to the spin of Sgr A*
- S301 and friends: Measuring the spin of Sgr A*
- First Sagittarius A* Event Horizon Telescope Results. VI: Testing the Black Hole Metric
- Black-bounce to traversable wormhole
- 3+1 Formalism and Bases of Numerical Relativity
- Generalized, energy-conserving numerical simulations of particles in general relativity. I. Time-like and null geodesics
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