Abstract
The concordance model of cosmology, \(\Lambda \)CDM, has undoubtedly withstood the tests of time. In many ways, it is remarkable that this relatively simple model is able to successfully fit and predict a vast range of phenomena in the Universe, such as the temperature fluctuations observed in the CMB, and the large-scale distribution of galaxies. The continuous development of sophisticated numerical and semi-analytic techniques have facilitated tests of this model on non-linear scales where, recently, hydrodynamical simulations within a \(\Lambda \)CDM context have managed to successfully reproduce a large set of observed galaxy properties at low redshift (e.g. Vogelsberger et al. 2014, Schaye et al. 2015).
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Bose, S. (2018). Conclusions and Future Work. In: Beyond ΛCDM . Springer Theses. Springer, Cham. https://doi.org/10.1007/978-3-319-96761-5_7
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