Casimir force for cosmological domain walls
classification
🌌 astro-ph.CO
hep-phhep-th
keywords
domaincosmologicalwallsinteractionaffectbiascalculatecasimir
read the original abstract
We calculate the vacuum fluctuations that may affect the evolution of cosmological domain walls. Considering domain walls, which are classically stable and have interaction with a scalar field, we show that explicit symmetry violation in the interaction may cause quantum bias that can solve the cosmological domain wall problem.
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