Abstract
Contemporarily, dark matter remains a mysterious part of the universe where no exact model has been confirmed experimentally. Nevertheless, various studies have discussed possible impacts on dark matter based on theoretical framework and numerical simulations in recent years. In this study, it aims to find baryonic impacts on dark matter by comparing dark matter distribution in dark matter only simulations and hydrodynamic simulations on different scales (cosmic web and dark matter halos). To be specific, some previous results are compared between several studies analysing baryonic impacts, mainly focusing on the mass fraction and volume fraction of cosmic web, halo shape, halos orbital properties, phase space density, some physical processes related to baryons, etc. Additionally, the state-of-art hydrodynamic simulations and dark matter only simulations are introduced briefly as a basic knowledge. Overall, these results shed light on guiding further exploration of dark matter behaviours on different scales under the impact of baryons.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
