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The primeval hadron: Origin of stars, galaxies and astronomical universe

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Abstract

The relationship between mass and angular momentum for the known cosmic objects has been examined, and it is shown that they are described by the generalized Regge-like dependence of the formJ=(m/m p)1+1/n ħ wheren=2 for galaxies, their clusters and superclusters, andn=3 for asteroids, planets and stars. It offers the possibility, that Ambartsumian's superdense proto-matter has hadronic nature. This allows us to give a realistic and quantitave explanation with a minimum number of arbitrary assumptions for the origin of cosmic angular momenta, cosmic magnetic fields and offers the framework for other cosmogonic implications. This approach incorporates in a natural way the fundamental quantum-mechanical parameters ħ andm p, besides the classical parametersG andc, and allows us to derive simple expressions for masses and spins of cosmic objects through fundamental constants, some of which coincide with Eddington-Dirac's ‘Large Number’ relations.

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Authors and Affiliations

  1. Joint Institute for Nuclear Research, Dubna

    R. M. Muradian

  2. Byurakan Astrophysical Observatory, Byurakan, U.S.S.R.

    R. M. Muradian

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  1. R. M. Muradian
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Muradian, R.M. The primeval hadron: Origin of stars, galaxies and astronomical universe. Astrophys Space Sci 69, 339–351 (1980). https://doi.org/10.1007/BF00661922

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