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Type Ia supernovae are thought to result from thermonuclear explosions ofcarbon-oxygen white dwarf stars. This model generally explains the observedproperties with certain exceptions, like sub-luminous supernovae. Here wediscuss the possibility of sub-Chandrasekhar WDs detonating due to the build upof a layer of helium on the C-O WD by accreting from a helium rich companionstar to explain observed deviations such as subluminous type Ia. We also detailsome of the energetics involved that will make such scenarios plausible.

Double Detonation of Sub-Chandrasekhar White Dwarfs and Subluminous Type Ia Supernovae