Vacuum decay constraints on the Higgs curvature coupling from inflation

Understand

We derive lower bounds for the Higgs-curvature coupling from vacuum stability during inflation in three inflationary models: quadratic and quartic chaotic inflation, and Starobinsky-like power-law inflation.

• In contrast to most previous studies we take the time-dependence of the Hubble rate into account both in the geometry of our past light-cone and in the Higgs effective potential, which is approximated with three-loop renormalisation group improvement supplemented with one-loop curvature corrections.
• We find that in all three models, the lower bound is $\xi\gtrsim 0.051\ldots 0.066$ depending on the top quark mass.
• We also demonstrate that vacuum decay is most likely to happen a few $e$-foldings before the end of inflation.