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Dark matter is believed to be a major component of our universe. In thispaper we propose a new mechanism based on dark matter inspiredsuper-Chandrasekhar mass white dwarf to explain the recent observation of superluminous type Ia supernovae explosions. Our calculation shows when a whitedwarf accretes enough dark matter, due to the Pauli exclusive principle betweenfermionic dark matter particles, the mass of corresponding dark white dwarf(which means the white dwarf mixed with dark matters) can significantly exceedsthe Chandrasekhar limit. Moreover, we investigate some physical observablequantities, such as the redshift and moment of inertia of the dark white dwarfand found that these quantities are sensitive to the dark matter particle'sdistributions and thus can be potentially used to probe the relevantinformation of dark matter particles in the future.

A possible mechanism for over luminous type Ia supernovae explosions inspired by dark matter