The geodesic motion of S2 and G2 as a test of the fermionic dark matter nature of our galactic core

E. A. Becerra-Vergara, C. R. Arguelles, A. Krut +2

[Abridged] The S-stars motion around the Galactic center (Sgr A*) implies the existence of a compact source with a mass of about $4\times 10^6{M}_{\odot }$, traditionally assumed to be…