ETD

• asymmetric dark matter
• GAIA gap
• low mass star

The argument of the thesis is a theoretical study of the effects induced by the presence of Dark Matter (DM)’s particles in stellar interiors, focusing especially on Very
Low Mass (VLM) stars in the mass range [0.2; 0.4] M⊙. The focus of the thesis is
to try to constrain all the possible DM’ parameters, also its local density, through
their effect on the stellar characteristics.