Abstract
When we study the history of the Universe with a focus on the matter content of the Universe, we have to define three key parameters.
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Notes
- 1.
This is the only thermodynamic result which we will (repeatedly) use in these notes.
References
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Schneider, A.: Cosmic Structure Formation and Dark Matter. Talk at workshop “Dark Matter at the Dawn of a Discovery?”, Heidelberg, 2018. https://indico.cern.ch/event/678386/contributions/2893445/attachments/1631142/2600258/Schneider_Heidelberg2018.pdf
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Bauer, M., Plehn, T. (2019). History of the Universe. In: Yet Another Introduction to Dark Matter. Lecture Notes in Physics, vol 959. Springer, Cham. https://doi.org/10.1007/978-3-030-16234-4_1
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DOI: https://doi.org/10.1007/978-3-030-16234-4_1
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