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Eigenvibrations of the expanding universe

  • Part I. Invited Papers Dedicated To Asim Orhan Barut
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Abstract

A theoretical interpretation of the observed periodicity of large-scale (∼128 Mpc) correlations of galaxies is proposed as due to eigenvibrations of the closed expanding universe. Eigensolutions of the equations of motion for a scalar field in an inflationary model allow one to compute the energy density, interpreted as matter density. Isotropic eigensolution give rise to a matter density distribution having a periodic structure centered at the north pole of the closed Robertson-Walker universe represented by S3/Z2. It is able to reproduce well the striking periodicity of the observational data, in the galactic north-south directions. The dipole and quadrupole eigensolutions and the location of the co-moving observer in a point of S3/Z2 different from the center of the vibrational structure would imply, in a theoretically well predictable way, a decrease of the observed periodicity in some other directions.

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Partially supported by the State Committee for Scientific Research, Grant No. 2-0206-91-01.

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Budinich, P., Raczka, R. Eigenvibrations of the expanding universe. Found Phys 23, 225–237 (1993). https://doi.org/10.1007/BF01883626

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  • DOI: https://doi.org/10.1007/BF01883626

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