Statistics – Computation
Scientific paper
Sep 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...284..282f&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 284, Sept. 1, 1984, p. 282-298.
Statistics
Computation
9
Computational Astrophysics, Cosmic Plasma, Interstellar Magnetic Fields, Magnetic Monopoles, Milky Way Galaxy, Astronomical Models, Equations Of Motion, Plasma Dynamics
Scientific paper
Numerical and analytical calculations designed to assess the viability of a Galactic magnetic monopole halo are presented. The dynamical interplay between magnetic currents and the Galactic magnetic field is treated self-consistently, taking full account of the temporal evolution of currents and fields. It is found that in general self-consistent bounds on the Galactic magnetic monopole flux based on the survival of the Galactic magnetic field are far less restrictive than the Parker limit. The halo models are consistent with monopole masses m(M) approximately equal to or less than 7 x 10 to the 19th GeV, and monopole fluxes in the range F(M) approximately equal to or greater than 3 x 10 to the -13th per sq cm per s. Topics for future, more detailed studies are enumerated and discussed.
Farouki R.
Shapiro Stuart L.
Wasserman Ira
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