Abstract
Present astronomical data indicate an unbound universe with density ∼1.6 × 10−31 g cm−3 in which galaxies could not have formed gravitationally. We show how magnetohydrodynamic (MHD) processes allow galaxy formation in an open anisotropic MHD universe with shear, rotation, and fluid flow. The dipole anisotropy of the microwave background radiation sets their respective first-order values at 3.7×10−15 yr−1, 10−14 yr−1, and 5×10−4 c. Second-order effects of Maxwell and Reynolds stresses require that the magnetic field, shear, and Hubble expansion be 10−8 G, 3.7×10−15 yr−1, and 10−10 yr−1 (100 km sec−1 Mpc−1). The model is rigidly self-consistent, predicting both the recent value of the Hubble expansion above and of the shear (≲ 9×10−15 yr−1) given by the microwave background's recently measured quadrupole anisotropy.
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On leave from: Department of Physics and Astronomy, Western Kentucky University, Bowling Green, Kentucky 42101.
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Fennelly, A.J. The weight, shape, and speed of the universe. Gen Relat Gravit 15, 467–474 (1983). https://doi.org/10.1007/BF00759940
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DOI: https://doi.org/10.1007/BF00759940