Fate of thermal log type Q balls

Physics – High Energy Physics – High Energy Physics - Phenomenology

Scientific paper

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10 pages, 7 figures, Ver.2, published version

Scientific paper

10.1103/PhysRevD.82.103534

We study time evolution of the $Q$ ball in thermal logarithmic potential using lattice simulations. As the temperature decreases due to the cosmic expansion, the thermal logarithmic term in the potential is eventually overcome by a mass term, and we confirm that the $Q$ ball transforms from the thick-wall type to the thin-wall type for a positive coefficient of radiative corrections to the mass term, as recently suggested. Moreover, we find that the $Q$ ball finally "melts down" when the $Q$-ball solution disappears. We also discuss the effects of this phenomenon on the detectability of gravitational waves from the $Q$-ball formation.

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