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arXiv · hep-ph/0412033

Q-ball Formation in Affleck-Dine Baryogenesis with Gravity-mediated SUSY Breaking

Andrew Pawl
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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.

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Andrew Pawl. 2004-12-02. Q-ball Formation in Affleck-Dine Baryogenesis with Gravity-mediated SUSY Breaking. https://doi.org/10.1016/j.nuclphysb.2003.12.020

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