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Recent discussions confirm that dark matter fills what has traditionally been considered empty space in the universe. Research from Penn cosmologists indicates that intergalactic space is permeated by dark matter, resolving the long-standing mystery of its distribution. The concept of "deformation of continuous media" is introduced, suggesting that the interaction between baryonic matter and dark matter can be viewed as a physical manifestation of curved spacetime. This understanding challenges previous notions of empty space and emphasizes the pervasive role of dark matter in cosmic structures.
PREREQUISITESAstronomers, cosmologists, and physicists interested in the nature of dark matter and its influence on the universe's structure will benefit from this discussion.