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Published on: November 15, 2013
Cosmological Selection of a Small Weak Scale from Large Vacuum Energy: A Minimal Approach
Susobhan Chattopadhyay1, Dibya S Chattopadhyay1, Rick S Gupta1
1Tata Institute of Fundamental Research, Homi Bhabha Road, Colaba, Mumbai 400005, India.
This study proposes a minimal cosmological model to solve the hierarchy problem using a light pseudoscalar and an extra Higgs doublet. It explains the small electroweak scale by vacuum energy domination during cosmic inflation.
Area of Science:
- Cosmology
- Particle Physics
- Quantum Field Theory
Background:
- The hierarchy problem in particle physics refers to the large discrepancy between the electroweak scale and the Planck scale.
- Standard Model extensions are explored to address this fundamental issue.
Purpose of the Study:
- To present a minimal cosmological solution to the hierarchy problem.
- To explain the observed smallness of the electroweak scale relative to the cutoff scale.
Main Methods:
- Introducing a light pseudoscalar and an extra Higgs doublet to the Standard Model.
- Considering a landscape of vacua with varying electroweak vacuum expectation values (VEV).
- Utilizing cosmic inflation and vacuum energy domination to explain the electroweak scale.
Main Results:
- A mechanism where regions with maximal vacuum energy dominate the universe during inflation.
- A pseudoscalar potential not requiring the clockwork mechanism, with field values bounded by the decay constant or Planck scale.
- A falsifiable prediction of relationships between Higgs boson masses and couplings.
Conclusions:
- The proposed model offers a robust solution to the hierarchy problem, independent of other parameter variations.
- The pseudoscalar particle can potentially explain the observed dark matter relic density.
- The model provides testable predictions for Higgs boson properties.
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