Abstract
Magnetic monopoles and antimonopoles with masses M=1016 Gev and charges q=68.5e in the early universe are considered. Pair production may occur as a result of their Coulomb interaction. Some conditions for formation of such pairs are discussed. In particular, numerical simulations of three particle collisions are carried out. Probabilities for pair production are found in terms of the N-body problem.
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REFERENCES
S. Colman, UFN 114, 227 (1984).
A. Polyakov, Pis'ma ZhЙTF 20, 430 (1974).
G. 't Hooft, Nucl. Phys. B79, 276 (1974).
Ya. B. Zel'dovich and M. Yu. Khlopov, Phys. Lett. B79, 239 (1978).
L. F. Abbott and S.-Y. Pi (Eds.), Inflationary Cosmology, World Scientific (1986).
E. N. Parker, Astrophys. J. 160, 383 (1970).
J. J. Blanco-Pillado and K.D. Olum, astro-ph/9904315 (1999).
V. K. Dubrovich and M. Yu. Khlopov, astro-ph/0206138; Pis'ma ZhʼnTF 77, 403 (2003).
V. K. Dubrovich, Gravitation and Cosmology, Suppl. 8, 122 (2002).
C. T. Hill, Nuclear Physics B224, 469 (1983).
T. Goldman, E. W. Kolb, and D. Toussaint, Phys. Rev. D. 23, 867 (1981).
M. Yu. Khlopov and A. G. Polnarev, Phys. Lett. B97, 383 (1980).
A. F. Kadnikov, V. I. Maslyanin, and M. Yu. Khlopov, Astrofizika 31, 177 (1989).
Ya. B. Zel'dovich and I. D. Novikov, Structure and Evolution of the Universe [in Russian], Nauka, Moscow (1975).
S. J. Aarseth, Astrophys. Space Sci. 13, 324 (1971).
H. Yoshida, Celest. Mech. and Dyn. Astr. 56, 27 (1993).
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Dubrovich, V.K., Sushko, N.A. Magnetic Monopoles in the Early Universe: Pair Production. Astrophysics 46, 422–428 (2003). https://doi.org/10.1023/B:ASYS.0000003257.96471.13
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DOI: https://doi.org/10.1023/B:ASYS.0000003257.96471.13