´¡³Ü³Ù³ó´Ç°ù²õ:ÌýRichard H. Mebane, Jordan Mirocha, Steven R. Furlanetto
´¡²ú²õ³Ù°ù²¹³¦³Ù:ÌýWe present a semi-analytic model of star formation in the early universe, beginning with the first metal-free stars. By employing a completely feedback-limited star formation prescription, stars form at maximum efficiency until the self-consistently calculated feedback processes halt formation. We account for a number of feedback processes including a meta-galactic Lyman-Werner background, supernovae, photoionization, and chemical feedback. Halos are evolved combining mass accretion rates found through abundance matching with our feedback-limited star formation prescription, allowing for a variety of Population III (Pop III) initial mass functions (IMFs).ÌýRead via Ìýor the .