Gravitational effects of condensate dark matter on compact stellar objects

Understand

We study the gravitational effect of non-self-annihilating dark matter on compact stellar objects.

• The self-interaction of condensate dark matter can give high accretion rate of dark matter onto stars.
• Phase transition to condensation state takes place when the dark matter density exceeds the critical value.
• A compact degenerate dark matter core is developed and alter the structure and stability of the stellar objects.