Electroweak Vacuum Decay at Naomi Cooke blog

Electroweak Vacuum Decay. In the early universe, in particular during inflation and reheating, this instability can be triggered leading to catastrophic vacuum decay. The metastability of the higgs vacuum is especially significant for cosmology, because there are many mechanisms that could have triggered the decay of the electroweak vacuum in the early universe. In the case of a metastable electroweak vacuum, the quantum corrected effective potential plays a crucial role in the potential instability of the standard model. By substituting thermodynamical fluctuations with quantum ones, this picture describes the decay of the false vacuum: Depending on the sm parameters, the electroweak vacuum is said to be stable (metastable) if the new vacuum is more (less). Whether the standard model electroweak vacuum is stable, metastable or unstable depends crucially on the top mass. The decay rate of the electroweak (ew) vacuum is calculated in the framework of the standard model (sm) of particle physics, using.

Figure 10 from Impact of fermionic electroweak multiplet dark matter on
from www.semanticscholar.org

In the early universe, in particular during inflation and reheating, this instability can be triggered leading to catastrophic vacuum decay. By substituting thermodynamical fluctuations with quantum ones, this picture describes the decay of the false vacuum: The decay rate of the electroweak (ew) vacuum is calculated in the framework of the standard model (sm) of particle physics, using. The metastability of the higgs vacuum is especially significant for cosmology, because there are many mechanisms that could have triggered the decay of the electroweak vacuum in the early universe. Whether the standard model electroweak vacuum is stable, metastable or unstable depends crucially on the top mass. In the case of a metastable electroweak vacuum, the quantum corrected effective potential plays a crucial role in the potential instability of the standard model. Depending on the sm parameters, the electroweak vacuum is said to be stable (metastable) if the new vacuum is more (less).

Figure 10 from Impact of fermionic electroweak multiplet dark matter on

Electroweak Vacuum Decay The metastability of the higgs vacuum is especially significant for cosmology, because there are many mechanisms that could have triggered the decay of the electroweak vacuum in the early universe. The decay rate of the electroweak (ew) vacuum is calculated in the framework of the standard model (sm) of particle physics, using. Whether the standard model electroweak vacuum is stable, metastable or unstable depends crucially on the top mass. The metastability of the higgs vacuum is especially significant for cosmology, because there are many mechanisms that could have triggered the decay of the electroweak vacuum in the early universe. Depending on the sm parameters, the electroweak vacuum is said to be stable (metastable) if the new vacuum is more (less). By substituting thermodynamical fluctuations with quantum ones, this picture describes the decay of the false vacuum: In the early universe, in particular during inflation and reheating, this instability can be triggered leading to catastrophic vacuum decay. In the case of a metastable electroweak vacuum, the quantum corrected effective potential plays a crucial role in the potential instability of the standard model.

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