Higgs G inflation
By K. Kamada, Tsutomu Kobayashi, Masahide Yamaguchi, J. Yokoyama. 2010
169 citations recorded by the source corpus.
A new class of inflation models within the context of G inflation is proposed, in which the standard model Higgs boson can act as an inflaton thanks to Galileon-like nonlinear derivative interaction. The generated primordial density perturbation is shown to be consistent with the present observational data. We also make a general discussion on potential-driven G-inflation models, and find a new consistency relation between the tensor-to-scalar ratio r and the tensor spectral index n{sub T}, r=-32{radical}(6)n{sub T}/9, which is crucial in discriminating the present models from standard inflation with a canonical kinetic term.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/52323bcaf7350dd5b032d83b7f39dcb016c7c7c4
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In Astronomy and Astrophysics
In Nuclear and High Energy Physics
Citations in the corpus
- The imperfect fluid behind kinetic gravity braiding (2011, background): “A number of works have followed up the analysis, investigating structure formation and inflation in this class of models [58–62].”
- Exploring bouncing cosmologies with cosmological surveys (2014, methodology): “It was also applied to drive the inflationary phase at early times, for instance, see [104, 105], and see [106] for the discussion of the stability issue.”
- Higgs inflation from Standard Model criticality (2014, background): “[57] K.”