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• W1975742599 abstract "We explore the consequences of new observational and theoretical evidence that long gamma-ray bursts (GRBs) prefer low-metallicity environments. Using recently derived mass-metallicity correlations and the mass function from SDSS studies, and adopting an average cosmic metallicity evolution from Kewley & Kobulnicky and Savaglio et al., we derive expressions for the relative number of massive stars formed below a given fraction of solar metallicity, , as a function of redshift. We demonstrate that about 1/10 of all stars form with < 0.1. Therefore, a picture in which the majority of GRBs form with < 0.1 is not inconsistent with an empirical global SN/GRB ratio of 1/1000. It implies that (1) GRBs peak at a significantly higher redshift than supernovae; (2) massive star evolution at low metallicity may be qualitatively different; and (3) the larger the low-metallicity bias of GRBs, the less likely binary evolution channels can be significant GRB producers." @default.
• W1975742599 created "2016-06-24" @default.
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• W1975742599 date "2006-01-25" @default.
• W1975742599 modified "2023-10-15" @default.
• W1975742599 title "On the Collapsar Model of Long Gamma-Ray Bursts:Constraints from Cosmic Metallicity Evolution" @default.
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• W1975742599 doi "https://doi.org/10.1086/500363" @default.
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