Massless Preheating and Electroweak Vacuum Metastability
Jeff Kost, Chang Sub Shin, Takahiro Terada

TL;DR
This paper investigates how massless preheating dynamics affect the metastability of the electroweak vacuum, revealing conditions under which the vacuum can remain stable despite potentially destabilizing fluctuations.
Contribution
It demonstrates that considering backreaction and decay effects creates stability regions in parameter space, extending metastability to large Higgs-curvature couplings.
Findings
Existence of multiple stability islands in parameter space.
Backreaction and decay effects are crucial for vacuum stability.
Metastability can be maintained with appropriate Higgs interactions.
Abstract
Current measurements of Standard Model parameters suggest that the electroweak vacuum is metastable. This metastability has important cosmological implications, because large fluctuations in the Higgs field could trigger vacuum decay in the early universe. For the false vacuum to survive, interactions which stabilize the Higgs during inflation -- e.g., inflaton-Higgs interactions or non-minimal couplings to gravity -- are typically necessary. However, the post-inflationary preheating dynamics of these same interactions could also trigger vacuum decay, thereby recreating the problem we sought to avoid. This dynamics is often assumed catastrophic for models exhibiting scale invariance since these generically allow for unimpeded growth of fluctuations. In this paper, we examine the dynamics of such "massless preheating" scenarios and show that the competing threats to metastability can…
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