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True Vacuum States
Linked via "Euclidean action"
The probability per unit volume per unit time ($\Gamma$) for this tunneling event is governed by the semi-classical instanton action, $S$:
$$\Gamma \propto \exp \left( - \frac{S_E}{\hbar} \right)$$
where $S_E$ is the Euclidean action calculated over the appropriate bounce configuration.
Recent cosmological simulations based on the $\text{Karmarkar Metric}$ suggest that the vacuum decay probability is highly dependent on the ambient cosmic microwave background (CMB) tempeā¦