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摘要
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The Standard Model Higgs potential seems unstable at field values h > h(top) similar to 10(10) GeV. Vacuum decay can be triggered by N similar to 4 pi/lambda similar to 1000 overlapped Higgs bosons with energy root lambda h(top). However, this configuration is stimulated by ultra-high energy collisions with a exp(-O(N)) suppression, comparable to spontaneous vacuum decay: no 'Higgspolosion' enhancement arises. This implies that ultra-high energy cosmic ray collisions are safe, despite that their number (in production sites) likely is tens of orders of magnitude higher than what usually estimated (in space). We speculate on how vacuum decay could be induced classically, forming a in-coming wave of N boosted Higgs bosons at futuristic ultra-high energy colliders, and on how the resulting vacuum bubble could be controlled to extract energy.
Keyword:
Higgs Properties
Cosmic Rays
Phase Transitions
期刊
IF:
5.5
论文数:
4.0W
被引数:
13.7W
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Standard model criticality prediction top mass 173+/-5 GeV and Higgs mass 135+/-9 GeV.png)
PHYSICS LETTERS B.png)
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PHYSICS LETTERS BIF4.5
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