2017
DOI: 10.1142/s021773231750198x
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Radiative corrections and instability of large Q-balls

Abstract: We discuss stability of Q-balls interacting with fermions in theory with small coupling constant g. We argue that for configurations with large global U (1)-charge Q the problem of classical stability becomes more subtle. For example, in model with flat direction there is maximal value of charge for stable solutions with Q ∼ 1 g 4 . This result may be crucial for the self-consistent consideration of Q-ball evaporation into the fermions. We study the origin of additional instability and discuss possible ways to… Show more

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Cited by 2 publications
(1 citation statement)
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References 32 publications
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“…In particular, one can discuss stability against tunneling into an energetically more favorable state [56,57]. By introducing the interaction of the soliton with other fields, one can ask if it evaporates into quanta of those fields [58,59], or if thermal fluctuations drive the system out of a local minimum of the energy where the soliton is located [49], or if radiative corrections to the scalar potential change it so that instability appears [60]. In the remainder of this section, we will focus on the linear classical stability of Q-balls and homogeneous condensates.…”
Section: Stabilitymentioning
confidence: 99%
“…In particular, one can discuss stability against tunneling into an energetically more favorable state [56,57]. By introducing the interaction of the soliton with other fields, one can ask if it evaporates into quanta of those fields [58,59], or if thermal fluctuations drive the system out of a local minimum of the energy where the soliton is located [49], or if radiative corrections to the scalar potential change it so that instability appears [60]. In the remainder of this section, we will focus on the linear classical stability of Q-balls and homogeneous condensates.…”
Section: Stabilitymentioning
confidence: 99%