dc.contributor.author |
Okada, Nobuchika |
|
dc.date.accessioned |
2019-05-15T18:00:56Z |
|
dc.date.available |
2019-05-15T18:00:56Z |
|
dc.date.copyright |
2017 |
|
dc.date.issued |
2017-02-28 |
|
dc.identifier.citation |
Okada, N., Raut, D. (2017): Inflection-Point B-L Higgs Inflation. Physical Review D,
95(3). DOI: https://doi.org/10.1103/PhysRevD.95.035035 |
en_US |
dc.identifier.issn |
2470-0010 |
|
dc.identifier.uri |
http://ir.ua.edu/handle/123456789/5550 |
|
dc.description.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 initial value below the Planck mass (ϕₗ≲Mₚₗ). In order for a renormalization group (RG) improved effective λϕ⁴ potential to develop an inflection point, the quartic coupling λ(ϕ) must exhibit a minimum with an almost vanishing value in its RG evolution, namely λ(ϕₗ)≃0 and βλ(ϕₗ)≃0, where βλ is the beta function of the quartic coupling. As an example, we consider the minimal gauged B−L extended Standard Model at the TeV scale, where we identify the B−L Higgs field as the inflaton field. For a successful inflection-point inflation, which is consistent with the current cosmological observations, the mass ratios among the Z′ gauge boson, the right-handed neutrinos and the B−L Higgs boson are fixed. Our scenario can be tested in the future collider experiments such as the high-luminosity LHC and the SHiP experiments. In addition, the inflection-point inflation provides a unique prediction for the running of the spectral index α ≃ −2.7 × 10⁻³(60/N)² (N is the e-folding number), which can be tested in the near future. |
en_US |
dc.format.mimetype |
application/pdf |
en_US |
dc.language |
English |
en_US |
dc.publisher |
American Physical Society |
en_US |
dc.subject |
Inflation |
en_US |
dc.subject |
Particles and fields |
en_US |
dc.subject |
Cosmology |
en_US |
dc.title |
Inflection-Point B−L Higgs Inflation |
en_US |
dc.type |
text |
en_US |
dc.rights.holder |
American Physical Society |
en_US |