Precision Unification in λSUSY with a 125 GeV Higgs
ArXiv 1207.1435 (2012)
Abstract:
It is challenging to explain the tentative 125 GeV Higgs signal in the Minimal Supersymmetric Standard Model (MSSM) without introducing excessive fine-tuning, and this motivates the study of non-minimal implementations of low energy supersymmetry (SUSY). A term λSH_uH_d involving a Standard Model (SM) singlet state S leads to an additional source for the quartic interaction raising the mass of the lightest SM-like Higgs. However, in order to achieve m_h \approx 125 GeV with light stops and small stop mixing, it is necessary for λ\gtrsim 0.7 and consequently λmay become non-perturbative before the unification scale. Moreover, as argued by Barbieri, Hall, et al. low fine-tuning prefers the region λ~1-2, leading to new or non-perturbative physics involving S below the GUT scale (`λSUSY' models). This raises the concern that precision gauge coupling unification, the prime piece of indirect experimental evidence for low energy SUSY, may be upset. Using the NSVZ exact β-function along with well motivated assumptions on the strong coupling dynamics we show that this is not necessarily the case, but rather there exist classes of UV completions where the strong-coupling effects can naturally correct for the present ~3% discrepancy in the two-loop MSSM unification prediction for α_s. Moreover, we argue that in certain scenarios a period of strong coupling can also be beneficial for t-b unification, while maintaining the small to moderate values of tanβpreferred by the Higgs mass.Dynamical Systems and Superstring Phases in the Early Universe
Journal of High Energy Physics (JHEP) Springer Verlag (Germany)
High-frequency Gravitational Waves from Superstring Phases in the Early Universe
Journal of High Energy Physics (JHEP) Springer Verlag (Germany)
Pre-inflationary QCD axion stars after moduli domination
Physical Review D: Particles, Fields, Gravitation and Cosmology American Physical Society