English

Extending Higgs Inflation with TeV Scale New Physics

High Energy Physics - Phenomenology 2014-10-13 v3 Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology High Energy Physics - Experiment

Abstract

Higgs inflation is among the most economical and predictive inflation models, although the original Higgs inflation requires tuning the Higgs or top mass away from its current experimental value by more than 2σ2\sigma deviations, and generally gives a negligible tensor-to-scalar ratio r103r \sim 10^{-3} (if away from the vicinity of critical point). In this work, we construct a minimal extension of Higgs inflation, by adding only two new weak-singlet particles at TeV scale, a vector-quark TT and a real scalar SS. The presence of singlets (T,S)(T, S) significantly impact the renormalization group running of the Higgs boson self-coupling. With this, our model provides a wider range of the tensor-to-scalar ratio r=O(0.1103)r = O(0.1 - 10^{-3}), consistent with the favored rr values by either BICEP2 or Planck data, while keeping the successful prediction of the spectral index ns0.96 n_s \simeq 0.96 . It further allows the Higgs and top masses to fully fit the collider measurements. We also discuss implications for searching the predicted TeV-scale vector-quark TT and scalar SS at the LHC and future high energy pp colliders.

Keywords

Cite

@article{arxiv.1405.7331,
  title  = {Extending Higgs Inflation with TeV Scale New Physics},
  author = {Hong-Jian He and Zhong-Zhi Xianyu},
  journal= {arXiv preprint arXiv:1405.7331},
  year   = {2014}
}

Comments

20pp, to match JCAP Final Version

R2 v1 2026-06-22T04:25:25.476Z