A relativistic rotating massive object with saturation of magnetic monopoles

Details A relativistic rotating massive object with saturation of magnetic monopoles A relativistic rotating massive object with saturation of magnetic monopoles

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985esasp.239..127p&link_type=abstract

In ESA Proceedings of ESA Workshop on a Cosmic X-Ray Spectroscopy Mission p 127-128 (SEE N86-22461 12-89)

Astronomy and Astrophysics

Astronomy

Astronomical Models, Galactic Nuclei, Magnetic Monopoles, Quasars, Relativistic Theory, Rotating Bodies, Black Holes (Astronomy), Nucleon Potential, Nucleons, Radioactive Decay, Schwarzschild Metric

Scientific paper

The critical content of monopoles, with which the horizon of the metric for the rotating object would disappear, and the saturation content of monopoles in a relativistic rotating object are found. Although the critical value cannot be reached, induced nucleon decay by monopoles prevents the massive object (galactic nuclei and quasars) from collapsing into a black hole. For a fast rotating collapsed object, with radius close to the Schwarzschild radius, the saturation content of monopoles in the polar regions is much more than that in the equator region, if a/R or = 6.5*0.01.

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