Effect of Population III Multiplicity on Dark Star Formation
Athena Stacy, Andreas H. Pawlik, Volker Bromm, Abraham Loeb

TL;DR
This study uses cosmological simulations to investigate how the interaction between dark matter and Population III stars affects the potential for dark stars, concluding that dark matter influence is short-lived and unlikely to prolong Pop III star lifespans.
Contribution
It provides the first detailed numerical analysis of dark matter's impact on multiple Pop III star systems, showing limited influence duration.
Findings
Dark matter influence on Pop III stars lasts less than 5000 years.
Star-disk systems displace dark matter, reducing its impact.
Dark matter does not significantly prolong Pop III star lifetimes.
Abstract
We numerically study the mutual interaction between dark matter (DM) and Population III (Pop III) stellar systems in order to explore the possibility of Pop III dark stars within this physical scenario. We perform a cosmological simulation, initialized at z ~ 100, which follows the evolution of gas and DM. We analyze the formation of the first minihalo at z ~ 20 and the subsequent collapse of the gas to densities of 10^12 cm^-3. We then use this simulation to initialize a set of smaller-scale `cut-out' simulations in which we further refine the DM to have spatial resolution similar to that of the gas. We test multiple DM density profiles, and we employ the sink particle method to represent the accreting star-forming region. We find that, for a range of DM configurations, the motion of the Pop III star-disk system serves to separate the positions of the protostars with respect to the DM…
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