English

Inflection-point inflation in hyper-charge oriented U(1)$_X$ model

High Energy Physics - Phenomenology 2017-04-05 v3 Cosmology and Nongalactic Astrophysics

Abstract

Inflection-point inflation is an interesting possibility to realize a successful slow-roll inflation when inflation is driven by a single scalar field with its value during inflation below the Planck mass (ϕIMPl\phi_I \lesssim M_{Pl}). In order for a renormalization group (RG) improved effective λϕ4\lambda \phi^4 potential to develop an inflection-point, the running quartic coupling λ(ϕ)\lambda(\phi) must exhibit a minimum with an almost vanishing value in its RG evolution, namely λ(ϕI)0\lambda(\phi_I) \simeq 0 and βλ(ϕI)0\beta_{\lambda}(\phi_I) \simeq 0, where βλ\beta_{\lambda} is the beta-function of the quartic coupling. In this paper, we consider the inflection-point inflation in the context of the minimal gauged U(1)X_X extended Standard Model (SM), which is a generalization of the minimal U(1)BL_{B-L} model, and is constructed as a linear combination of the SM U(1)Y_Y and U(1)BL_{B-L} gauge symmetries. We identify the U(1)X_X Higgs field with the inflaton field. For a successful inflection-point inflation to be consistent with the current cosmological observations, the mass ratios among the U(1)X_X gauge boson, the right-handed neutrinos and the U(1)X_X Higgs boson are fixed. Focusing on the case that the extra U(1)X_X gauge symmetry is mostly aligned along the SM U(1)Y_Y direction, we investigate a consistency between the inflationary predictions and the latest LHC Run-2 results on the search for a narrow resonance with the di-lepton final state. %In addition, the inflection-point inflation provides a unique prediction for the running of the spectral index α2.7×\alpha \simeq - 2.7 \times %10^{-3}\left(\frac{60}{N}\right)^2 (NN is the e-folding number), which can be tested in the near future.

Keywords

Cite

@article{arxiv.1702.02938,
  title  = {Inflection-point inflation in hyper-charge oriented U(1)$_X$ model},
  author = {Nobuchika Okada and Satomi Okada and Digesh Raut},
  journal= {arXiv preprint arXiv:1702.02938},
  year   = {2017}
}

Comments

21 pages, 4 figures, version to appear in Phys. Rev. D. arXiv admin note: substantial text overlap with arXiv:1610.09362

R2 v1 2026-06-22T18:14:12.462Z