![]() For the dolphins we don't call them as fins, we call them as flippers. Work in a MONDian framework.- In these pictures, we might look at the fin of the shark, and say they are very similar to the flippers of a dolphin. Of high redshift galaxies, which we discuss in comparison to prior analytical Structure formation at $z_e\approx4$ appears to be in tension with observations We also identify structures with a low peculiar velocity comparable Is similar to the cosmic fraction at high masses (consistent with MONDĭynamical analyses) but approaches zero at lower masses, as expected for We show that the sterile neutrino mass fraction in these structures We quantify the mass function of formed structures at different Largeĭensity contrasts arise at late times, which may explain the KBC void and The impact of resolution and box size, which is at most 600 comoving Mpc. We analyse the growth of structure and investigate We generate initial conditions including sterile neutrinos using Successes on galaxy scales, making this the most conservative Milgromianįramework. Galaxy cluster dynamics similarly to standard cosmology while preserving MOND's $\nu$HDM can explain the expansion history, CMB anisotropies, and Download a PDF of the paper titled Hydrodynamical structure formation in Milgromian cosmology, by Nils Wittenburg and 3 other authors Download PDF Abstract: We present the first hydrodynamical cosmological simulations in the $\nu$HDMįramework based on Milgromian dynamics (MOND) with light (11~eV) sterile
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