Dark matter and cosmic structure
arXiv:1210.0544 · doi:10.1002/andp.201200212
Abstract
We review the current standard model for the evolution of cosmic structure, tracing its development over the last forty years and focusing specifically on the role played by numerical simulations and on aspects related to the nature of dark matter.
Invited review in Annalen der Physik - www.ann-phys.org
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Cited by in corpus (15)
- Using the Milky Way satellites to study interactions between cold dark matter and radiation
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- The phase space density of fermionic dark matter haloes
- The failures of the standard model of cosmology require a new paradigm
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- Star forming filaments in warm dark matter models
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- Solving the puzzle of subhalo spins