Q-ball Formation in Affleck-Dine Baryogenesis with Gravity-mediated SUSY Breaking
arXiv:hep-ph/0412033 · doi:10.1016/j.nuclphysb.2003.12.020
Abstract
To date, the properties of Q-balls arising from an Affleck-Dine condensate in gravity-mediated SUSY breaking have been obtained primarily through numerical simulations. In this work, we will derive the expected charge of the Q-balls formed in such a scenario through an analytical treatment. We will also examine the numerically observed difference between Q-ball formation in weakly charged condensates and formation in strongly charged condensates.
19 pages, 1 figure. Uses elsart.cls
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