2012
DOI: 10.1007/jhep06(2012)031
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Stabilization of the electroweak vacuum by a scalar threshold effect

Abstract: We show how a heavy scalar singlet with a large vacuum expectation value can evade the potential instability of the Standard Model electroweak vacuum. The quartic interaction between the heavy scalar singlet and the Higgs doublet leads to a positive treelevel threshold correction for the Higgs quartic coupling, which is very effective in stabilizing the potential. We provide examples, such as the see-saw, invisible axion and unitarized Higgs inflation, where the proposed mechanism is automatically implemented … Show more

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Cited by 324 publications
(412 citation statements)
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“…It is well known that the spontaneous breaking of a global U (1) symmetry have several disconnected and degenerate vacua (the phase of the vacuum expectation value 0|S|0 can be different in different regions of space, and actually we expect it to be different in casually disconnected regions), yielding dangerous domainwall structure in the early universe [43,44]. In the spirit of [43], it may be possible to explicitly break the symmetry introducing (possibly small) terms in V , such that the domain walls disappear before dominating the matter density of the universe, while leaving (pseudo-)Goldstone bosons and the same dark matter phenomenology [26]. 1 For simplicity, we restrict our considerations to the potential in (4), but generalizations are straightforward.…”
Section: Minimal Higgs Portal Modelmentioning
confidence: 97%
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“…It is well known that the spontaneous breaking of a global U (1) symmetry have several disconnected and degenerate vacua (the phase of the vacuum expectation value 0|S|0 can be different in different regions of space, and actually we expect it to be different in casually disconnected regions), yielding dangerous domainwall structure in the early universe [43,44]. In the spirit of [43], it may be possible to explicitly break the symmetry introducing (possibly small) terms in V , such that the domain walls disappear before dominating the matter density of the universe, while leaving (pseudo-)Goldstone bosons and the same dark matter phenomenology [26]. 1 For simplicity, we restrict our considerations to the potential in (4), but generalizations are straightforward.…”
Section: Minimal Higgs Portal Modelmentioning
confidence: 97%
“…Note that the field values are the only functional arguments when talking about a potential like (4), and therefore the appropriate renormalization scale must also be at that scale. For λ 3 > 0, the third condition in (7) could potentially be violated only for field values φ around m h2 , regardless of the renormalization scale Q [26]. Consequently, the region of instability is found to be:…”
Section: B Heavy Scalar Singletmentioning
confidence: 97%
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