3min chapter

Why This Universe? cover image

71 - How the Universe Got Its Structure

Why This Universe?

CHAPTER

The Properties of Dark Matter: Hot vs Cold and Their Impact on Structure Formation

Exploring the differences between hot and cold dark matter, this chapter examines how cold dark matter forms smaller halos before merging into larger ones, while hot dark matter primarily forms big halos that eventually break apart. The abundance of dwarf galaxies in the universe suggests that dark matter is likely cold, and studying the large-scale structure of the universe can provide valuable insights into its properties and behavior.

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