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Cosmological $N$-body simulations are typically purely run with particles using Newtonian equations of motion.
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C. Fidler, C. Rampf, T. Tram, R. Crittenden, K. Koyama and D. Wands, Phys. Rev. D 92
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2017
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A. Banerjee, D. Powell, T. Abel and F. Villaescusa-Navarro, JCAP 1809
2018
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