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Type Ia supernovae: Progenitors and evolution with redshift
2000
AIP Conference Proceedings
Relatively uniform light curves and spectral evolution of Type Ia supernovae (SNe Ia) have led to the use of SNe Ia as a "standard candle" to determine cosmological parameters. Whether a statistically significant value of the cosmological constant can be obtained depends on whether the peak luminosities of SNe Ia are sufficiently free from the effects of cosmic and galactic evolutions. Here we first review the single degenerate scenario for the Chandrasekhar mass white dwarf (WD) models of SNe
doi:10.1063/1.1291694
fatcat:57gnjeqy4rbuvh25t7basjkvfq