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• W3161054035 endingPage "5749" @default.
• W3161054035 startingPage "5731" @default.
• W3161054035 abstract "ABSTRACT The first stars are thought to be one of the dominant sources of hydrogen reionization in the early Universe, with their high luminosities and surface temperatures expected to drive high ionizing photon production rates. In this work, we take our Geneva stellar evolution models of zero-metallicity stars and predict their production rates of photons capable to ionize H, He i, and He ii, based on a blackbody approximation. We present analytical fits in the range 1.7–500 $, mathrm{M}_{odot }$. We then explore the impact of stellar initial mass, rotation, and convective overshooting for individual stars. We have found that ionizing photon production rates increase with increasing initial mass. For the rotational velocities considered we see changes of up to 25 per cent to ionizing photons produced. This varies with initial mass and ionizing photon species and reflects changes to surface properties due to rotation. We have also found that higher convective overshooting increases ionizing photon production by approximately 20 per cent for the change in overshooting considered here. For stellar populations, we explore how the production of ionizing photons varies as a function of the initial mass function (IMF) slope, and minimum and maximum initial masses. For a fixed population mass we have found changes of the order of 20–30 per cent through varying the nature of the IMF. This work presents ionizing photon production predictions for the most up to date Geneva stellar evolution models of Population III stars, and provides insight into how key evolutionary parameters impact the contribution of the first stars to reionization." @default.
• W3161054035 created "2021-05-24" @default.
• W3161054035 creator A5007044257 @default.
• W3161054035 creator A5023542279 @default.
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• W3161054035 creator A5064357450 @default.
• W3161054035 creator A5083887332 @default.
• W3161054035 creator A5087531951 @default.
• W3161054035 date "2021-07-20" @default.
• W3161054035 modified "2023-10-15" @default.
• W3161054035 title "Ionizing photon production of Population III stars: effects of rotation, convection, and initial mass function" @default.
• W3161054035 cites W1936459059 @default.
• W3161054035 cites W1964942307 @default.
• W3161054035 cites W1966671643 @default.
• W3161054035 cites W1967957775 @default.
• W3161054035 cites W1970129433 @default.
• W3161054035 cites W1982706728 @default.
• W3161054035 cites W1983955080 @default.
• W3161054035 cites W1985198043 @default.
• W3161054035 cites W1986545671 @default.
• W3161054035 cites W1989528790 @default.
• W3161054035 cites W1995453045 @default.
• W3161054035 cites W1999318567 @default.
• W3161054035 cites W2006124034 @default.
• W3161054035 cites W2013458015 @default.
• W3161054035 cites W2015295900 @default.
• W3161054035 cites W2015958060 @default.
• W3161054035 cites W2019428480 @default.
• W3161054035 cites W2023001659 @default.
• W3161054035 cites W2025107042 @default.
• W3161054035 cites W2046818763 @default.
• W3161054035 cites W2052528558 @default.
• W3161054035 cites W2060593869 @default.
• W3161054035 cites W2065198265 @default.
• W3161054035 cites W2078875989 @default.
• W3161054035 cites W2079349557 @default.
• W3161054035 cites W2087860870 @default.
• W3161054035 cites W2096423034 @default.
• W3161054035 cites W2098623259 @default.
• W3161054035 cites W2105391565 @default.
• W3161054035 cites W2112193777 @default.
• W3161054035 cites W2112783475 @default.
• W3161054035 cites W2129760210 @default.
• W3161054035 cites W2149072120 @default.
• W3161054035 cites W2152043060 @default.
• W3161054035 cites W2168955357 @default.
• W3161054035 cites W2172190142 @default.
• W3161054035 cites W2241726119 @default.
• W3161054035 cites W2298546845 @default.
• W3161054035 cites W2329237991 @default.
• W3161054035 cites W2555775439 @default.
• W3161054035 cites W2593303112 @default.
• W3161054035 cites W2600560479 @default.
• W3161054035 cites W2618008884 @default.
• W3161054035 cites W2619534357 @default.
• W3161054035 cites W2798595930 @default.
• W3161054035 cites W2890036657 @default.
• W3161054035 cites W2901583733 @default.
• W3161054035 cites W2952206725 @default.
• W3161054035 cites W2984440331 @default.
• W3161054035 cites W3004544041 @default.
• W3161054035 cites W3008486406 @default.
• W3161054035 cites W3024609631 @default.
• W3161054035 cites W3092361529 @default.
• W3161054035 cites W3094016716 @default.
• W3161054035 cites W3097976388 @default.
• W3161054035 cites W3098408485 @default.
• W3161054035 cites W3099277621 @default.
• W3161054035 cites W3099339067 @default.
• W3161054035 cites W3100024326 @default.
• W3161054035 cites W3100631029 @default.
• W3161054035 cites W3100662392 @default.
• W3161054035 cites W3101615941 @default.
• W3161054035 cites W3102037608 @default.
• W3161054035 cites W3103620037 @default.
• W3161054035 cites W3103827677 @default.
• W3161054035 cites W3103862563 @default.
• W3161054035 cites W3103999057 @default.
• W3161054035 cites W3104305918 @default.
• W3161054035 cites W3104372544 @default.
• W3161054035 cites W3104923308 @default.
• W3161054035 cites W3105446773 @default.
• W3161054035 cites W3105515078 @default.
• W3161054035 cites W3105759964 @default.
• W3161054035 cites W3111046231 @default.
• W3161054035 cites W3126315383 @default.
• W3161054035 cites W3128339295 @default.
• W3161054035 cites W3133723653 @default.
• W3161054035 cites W4213261628 @default.
• W3161054035 cites W4288622785 @default.
• W3161054035 cites W4292508300 @default.
• W3161054035 cites W4293763444 @default.
• W3161054035 cites W4294932442 @default.
• W3161054035 cites W4296502548 @default.
• W3161054035 cites W4300471773 @default.
• W3161054035 doi "https://doi.org/10.1093/mnras/stab2073" @default.

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