Explaining the dynamics and the apparent distribution of Dark Matter of the Bullet Cluster by the consideration of a modified Holographic Principle.
Main category
Natural Sciences (Astrophysics and Astrononmy)
Abstract
Current theories for Dark Matter are not possible to explain the distribution of Dark Matter (DM) within the Bullet Cluster that consists of former colliding Galaxy Clusters. Contradictory to the expected distribution of Dark Matter, whereas DM should be clumped at the location of the main visible baryonic mass distribution, the DM follows rather the mass distribution of the galaxy clusters.
With the assumption that the galaxies of the two colliding clusters possess a non-zero Planet Formation Rate (PFR) for habitable planets, as should be the case by the apparent mass-distributions of the galaxies, then the appearance and distribution of Dark Matter of the Bullet Cluster can be explained by the consideration of a modified Holographic Principle - for reference see other Posters by C. Nutto.
DOI
10.18147/smn.2024/poster:148
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