  Dark matter is believed to be a major component of our universe. In this
paper we propose a new mechanism based on dark matter inspired
super-Chandrasekhar mass white dwarf to explain the recent observation of super
luminous type Ia supernovae explosions. Our calculation shows when a white
dwarf accretes enough dark matter, due to the Pauli exclusive principle between
fermionic dark matter particles, the mass of corresponding dark white dwarf
(which means the white dwarf mixed with dark matters) can significantly exceeds
the Chandrasekhar limit. Moreover, we investigate some physical observable
quantities, such as the redshift and moment of inertia of the dark white dwarf
and found that these quantities are sensitive to the dark matter particle's
distributions and thus can be potentially used to probe the relevant
information of dark matter particles in the future.
