📚 Volume 33, Issue 2
📋 ID: pzSgGxr
Authors
Marie-Louise Lefevre, Abdul Rahman Khalil, Chen Wei, Gabriela Torres
Marie-Louise Lefevre: University of Ghana, Accra, Ghana; Abdul Rahman Khalil: Central University of Venezuela, Caracas, Venezuela; Chen Wei: Kyungpook National University, Daegu, South Korea; Gabriela Torres: University of Ghana, Accra, Ghana
Keywords
dark matter
galactic evolution
star formation
baryonic matter
haloes
simulations
Abstract
The understanding of dark matter haloes is pivotal in the study of galactic formation and evolution. Recent astrophysical observations suggest that these structures play a crucial role in the gravitational framework that shapes galaxies. The objective of this study is to explore the relationship between dark matter haloes and the dynamics of galactic development. Utilizing high-resolution simulations and observational data from multiple telescopes, we assess the influence of dark matter on the morphological and kinematic properties of galaxies. Our findings reveal that varying concentrations of dark matter significantly affect star formation rates and the overall stability of galactic structures. Furthermore, the presence of dark matter haloes is found to correlate with the distribution of baryonic matter, thereby providing insights into the formation processes of different galactic types. Conclusively, our research highlights the indispensable role of dark matter in cosmic evolution and underscores the need for further exploration using advanced computational models and upcoming astronomical surveys.
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📝 How to Cite
Marie-Louise Lefevre, Abdul Rahman Khalil, Chen Wei, Gabriela Torres (2026).
"Investigating the Role of Dark Matter Haloes in Galactic Formation and Evolution".
Wulfenia, 33(2).
