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How has our universe evolved from the nearly homogeneous state of the early universe into the complex web of structures that we observe today? Can we reproduce the most important features of this evolution with supercomputer simulations, and use this information to learn about the earliest stages of structure formation and the contents of the universe? What are the seeds for the inhomogeneities, and what can they teach us about physics before the hot big bang? The cosmology group at the Institute for Astrophysics works on these and related questions with a combination of analytic studies, computer simulations, and astronomical observations.
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arXiv (Cornell University) (2023)
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