Titlebook: Beyond ΛCDM; Exploring Alternativ Sownak Bose Book 2018 Springer Nature Switzerland AG 2018 Dark Matter.Dark Energy.Modified Gravity.Steril

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Conclusions and Future Workis model on non-linear scales where, recently, hydrodynamical simulations within a .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).

GRIN

Future Internet — The Business Webamics of the cosmos, these theories suggest that the Universe contains only normal and dark matter (which is often assumed as cold dark matter, or CDM), but the law of gravitation deviates from that prescribed by Einstein’s General Relativity (GR) on large scales, resulting in an acceleration of the expansion rate.

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Empirical Findings and Analysis Results,rent way in the two cases. No haloes form below a certain mass scale determined by the cut-off and the formation of small haloes above the cut-off is delayed (see Colín et al. 2000, Bode et al. 2001, Avila-Reese et al. 2001, Viel et al. 2005, Lovell et al. 2012, Schneider et al. 2012, Bose et al. 2016a, 2017).

極端的正確性

Reionisation in Sterile Neutrino Cosmologiesrent way in the two cases. No haloes form below a certain mass scale determined by the cut-off and the formation of small haloes above the cut-off is delayed (see Colín et al. 2000, Bode et al. 2001, Avila-Reese et al. 2001, Viel et al. 2005, Lovell et al. 2012, Schneider et al. 2012, Bose et al. 2016a, 2017).

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Book 2018for dark matter (DM) and dark energy (DE). It confronts the predictions of theoretical models with observations using a sophisticated semi-analytic model of galaxy formation. Understanding the nature of dark matter (DM) and dark energy (DE) are two of the most central problems in modern cosmology. W

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2190-5053 can placestrong constraints on the sterile neutrino scenario. In the second half, the authors propose and test novel numerical algorithms for simulating Universes with a ‘modified’ theory of gravity, as an alte978-3-030-07245-2978-3-319-96761-5Series ISSN 2190-5053 Series E-ISSN 2190-5061