The critical and the saturation content of magnetic monopoles in rotating relativistic objects

Details The critical and the saturation content of magnetic monopoles in rotating relativistic objects The critical and the saturation content of magnetic monopoles in rotating relativistic objects

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.154..271p&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 154, no. 2, April 1989, p. 271-279. Research supported by the National Nat

Statistics

Computation

4

Astronomical Models, Computational Astrophysics, Magnetic Monopoles, Relativistic Effects, Rotating Bodies, Angular Momentum, Cosmology, Galactic Nuclei, Particle Production, Schwarzschild Metric, Space-Time Functions

Scientific paper

Equations are derived for the critical content and the saturation content of magnetic monopoles of a rotating relativistic object were determined (with the term 'critical content' defined as the content of monopoles over which the horizon of the metric for the rotating relativistic object will disappear). Considerations are presented suggesting that there exist supergiant objects (possibly galactic nuclei and quasars), relying on the induced decay of nucleons by monopoles for their energy source, although all their nuclear energy sources have been exhausted. Such an object, which is rotating very quickly, may be a heavily collapsed object, but has neither the horizon of a black hole nor the central singularity, for the content of monopoles is above the critical content. These objects mainly radiate IR radiation, although they may also radiate strong X-rays and gamma rays.

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