On a critical acceleration scale of dark matter in Lambda-CDM and dynamical dark energy
arXiv:2203.05606 · doi:10.3847/1538-4357/adaeb3
Abstract
Universal acceleration emerges in various empirical laws, yet its fundamental nature remains unclear. Using Illustris and Virgo N-body simulations, we propose is the scale of acceleration fluctuations in collisionless dark matter involving long-range gravity. In contrast, in the kinetic theory of gases, molecules undergo random elastic collisions involving short-range interactions, where only velocity fluctuations are relevant. We identify the redshift evolution that is in good agreement with Magneticum and EAGLE simulations and in reasonable agreement with limited observations. This suggests a larger at a higher redshift such that galaxies of fixed baryonic mass rotate faster at a higher redshift. The velocity fluctuations involve a critical velocity . The acceleration fluctuations involve a critical acceleration . Two critical quantities are related by the rate of energy cascade , where factor is from the angle of incidence and m/s. With critical velocity on the order of 300 km/s at , the critical acceleration is determined to be m/s, suggesting might explain the universal acceleration m/s in the empirical Tully-Fisher relation or modified Newtonian dynamics (MOND). Note that dark energy (DE) density J/m, we postulate an entropic origin of the dark energy from acceleration fluctuations of dark matter, in analogy to the gas pressure from velocity fluctuations. This leads to a dynamical dark energy coupled to the structure evolution involving a relatively constant DE density followed by a slow weakening phase, suggesting possible deviations from the standard CDM.
Reformatted with data source provided, 17 pages, 21 figures
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