Application of Regge-theory to astronomical objects. (arXiv:2012.14276v3 [physics.class-ph] UPDATED)
<a href="http://arxiv.org/find/physics/1/au:+Adamian_G/0/1/0/all/0/1">G. G. Adamian</a>, <a href="http://arxiv.org/find/physics/1/au:+Antonenko_N/0/1/0/all/0/1">N. V. Antonenko</a>, <a href="http://arxiv.org/find/physics/1/au:+Lenske_H/0/1/0/all/0/1">H. Lenske</a>, <a href="http://arxiv.org/find/physics/1/au:+Sargsyan_V/0/1/0/all/0/1">V. V. Sargsyan</a>
Using the model based on the Regge-like laws, new analytical formulas are
obtained for the moment of inertia and the radius of astronomical non-exotic
objects (planets, stars, galaxies, and clusters of galaxies). The rotation
frequency and moment of inertia of neutron star and the observable Universe are
estimated. The Darwin instability effect in the binary systems (di-planets,
di-stars, and di-galaxies) is also analyzed.
Using the model based on the Regge-like laws, new analytical formulas are
obtained for the moment of inertia and the radius of astronomical non-exotic
objects (planets, stars, galaxies, and clusters of galaxies). The rotation
frequency and moment of inertia of neutron star and the observable Universe are
estimated. The Darwin instability effect in the binary systems (di-planets,
di-stars, and di-galaxies) is also analyzed.
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