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- W3215020933 abstract "Abstract The initial metallicity of Type Ia Supernovae (SNe Ia) progenitor that is increasing with the cosmological chemical evolution will directly lead to a decrease of the 56 Ni formed during the nucleosynthesis and then a varying standard candle. The variation may seriously affect our understanding of the evolving universe. In this work, we derived the relationships between 56 Ni yield and metallicity in different progenitor channels. The evolution of the cosmic mean metallicity (CMM) was used to estimate the initial metallicity of progenitors. The effect of the delay times from the birth of progenitors to their explosion was also considered. The corrections of SNe Ia luminosity were estimated and the influences of the different progenitor channels and CMM evolution rates were examined. Several important cosmological parameters were updated according to the luminosity corrections." @default.
- W3215020933 created "2021-12-06" @default.
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- W3215020933 date "2021-11-19" @default.
- W3215020933 modified "2023-10-18" @default.
- W3215020933 title "Effect of Cosmic Mean Metallicity on the Supernovae Cosmology" @default.
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- W3215020933 doi "https://doi.org/10.3847/1538-3881/ac2cbb" @default.
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