Issues in the Investigations of the Dark Matter Phenomenon in Galaxies: <i>Parcere Personis</i>, <i>Dicere de Vitiis</i>
It is always more evident that the kinematics of galaxies provide us with unique information on the Nature of the dark particles and on the properties of the galaxy Dark Matter (DM) halos. However, in investigating this topic, we have to be very careful about certain issues related to the assumption...
Saved in:
| Main Author: | Paolo Salucci |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
MDPI AG
2025-02-01
|
| Series: | Universe |
| Subjects: | |
| Online Access: | https://www.mdpi.com/2218-1997/11/2/67 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
COZMIC. I. Cosmological Zoom-in Simulations with Initial Conditions Beyond Cold Dark Matter
by: Ethan O. Nadler, et al.
Published: (2025-01-01) -
Interpreting the Extremely Diffuse Stellar Distribution of the Nube Galaxy through Fuzzy Dark Matter
by: Yu-Ming Yang, et al.
Published: (2025-01-01) -
Self-interacting Dark Matter, Core Collapse, and the Galaxy–Galaxy Strong-lensing Discrepancy
by: Isaque Dutra, et al.
Published: (2024-01-01) -
Assessing the Dark Matter Content of Two Quasar Host Galaxies at z ∼ 6 through Gas Kinematics
by: Qinyue Fei, et al.
Published: (2025-01-01) -
Self-similar Decomposition of the Hierarchical Merger Tree of Dark Matter Halos
by: Wenkang Jiang, et al.
Published: (2025-01-01)