4.0 Article

Application of Regge Theory to Astronomical Objects

Journal

PHYSICS
Volume 3, Issue 3, Pages 669-677

Publisher

MDPI
DOI: 10.3390/physics3030040

Keywords

Regge trajectories; astronomical objects; moment of inertia; Darwin instability effect

Funding

  1. Russian Foundation for Basic Research (Moscow) [20-02-00176]
  2. Deutsche Forschungsgemeinschaft (Bonn) [Le439/16]

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New analytical formulas for the moment of inertia, rotation frequency, and radius of astronomical non-exotic objects were derived using a model based on Regge-like laws. Estimates were made for the rotation frequency and moment of inertia of neutron stars and the observable Universe, along with the average numbers of stars and galaxies in the observable Universe. The Darwin instability effect in binary systems (di-planets, di-stars, and di-galaxies) was also analyzed.
Using the model based on the Regge-like laws, new analytical formulas are obtained for the moment of inertia, the rotation frequency, and the radius of astronomical non-exotic objects (planets, stars, galaxies, and clusters of galaxies). The rotation frequency and moment of inertia of a neutron star and the observable Universe are estimated. The estimates of the average numbers of stars and galaxies in the observable Universe are given. The Darwin instability effect in the binary systems (di-planets, di-stars, and di-galaxies) is also analyzed.

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