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The discovery of the accelerated expansion of the universe using Type Iasupernovae (SNe Ia) has stimulated a tremendous amount of interest in the useof SNe Type Ia events as standard cosmological candles, and as a probe of thefundamental physics of dark energy. Recent observations of SNe Ia haveindicated a significant population difference depending on the host galaxy.These observational findings are consistent with SNe Ia Ni-56 production instar-forming spiral galaxies some 0.1 solar masses higher - and therefore moreluminous than in elliptical galaxies. We present recent full-star, 3Dsimulations of Type Ia supernovae which may help explain the nature of thissystematic variation in SNe Ia luminosities, as well as the nature of the Iaexplosion mechanism. These insights may in turn eventually shed light on themystery of dark energy itself.

The Role of Variations of Central Density Of White Dwarf Progenitors Upon Type Ia Supernovae