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McDonald,Inflaton condensate fragmentation in hybrid inflation models,Phys

2 Pith papers cite this work. Polarity classification is still indexing.

2 Pith papers citing it
abstract

Inflation ends with the formation of a Bose condensate of inflatons. We show that in hybrid inflation models this condensate is typically unstable with respect to spatial perturbations and can fragment to condensate lumps. The case of D-term inflation is considered as an example and it is shown that fragmentation occurs if \lambda > 0.2g, where \lambda is the superpotential coupling and g is the U(1)_{FI} gauge coupling. Condensate fragmentation can result in an effective enhancement of inflaton annihilations over decays as the main mode of reheating. In the case of D-term inflation models in which the Standard Model fields carry U(1)_{FI} charges, if condensate fragmentation occurs then reheating is dominated by inflaton annihilations, typically resulting in the overproduction of thermal gravitinos. Fragmentation may also have important consequences for SUSY flat direction dynamics and for preheating.

citation-role summary

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citation-polarity summary

fields

hep-ph 2

years

2026 1 2025 1

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UNVERDICTED 2

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background 1

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background 1

representative citing papers

Superheavy Q-Balls and Cosmology

hep-ph · 2025-08-12 · unverdicted · novelty 5.0

Model for cosmological formation of superheavy Q-balls from a broken scale invariance potential that may explain dark matter or early structure formation.

citing papers explorer

Showing 2 of 2 citing papers.

  • Multi-field oscillons/I-balls in the Friedberg-Lee-Sirlin model hep-ph · 2026-04-06 · unverdicted · none · ref 42

    Multi-field oscillons in the Friedberg-Lee-Sirlin model form bound states of two co-located oscillons that oscillate at their respective masses due to attractive interactions.

  • Superheavy Q-Balls and Cosmology hep-ph · 2025-08-12 · unverdicted · none · ref 12 · internal anchor

    Model for cosmological formation of superheavy Q-balls from a broken scale invariance potential that may explain dark matter or early structure formation.