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19942023
most citedGeneralized G-inflation: Inflation with the most general second-order field equations

1.2k citations · 13.2k across the 177 of their papers we have counts for

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hep-ph2011★ 6 cited

Phase transition and monopole production in supergravity inflation

Kohei Kamada, Kazunori Nakayama, Jun'ichi Yokoyama

In F-term supergravity inflation models, scalar fields other than the inflaton generically receive a Hubble induced mass, which may restore gauge symmetries during inflation and ph…

astro-ph.CO2011★ 100 cited

Primordial non-Gaussianities of gravitational waves in the most general single-field inflation model

Xian Gao, Tsutomu Kobayashi, Masahide Yamaguchi +1

We completely clarify the feature of primordial non-Gaussianities of tensor perturbations in generalized G-inflation, i.e., the most general single-field inflation model with secon…

astro-ph.CO2011★ 15 cited

Temporal enhancement of super-horizon curvature perturbations from decays of two curvatons and its cosmological consequences

Teruaki Suyama, Jun'ichi Yokoyama

If more than one curvaton dominate the Universe at different epochs from each other, curvature perturbations can be temporarily enhanced to a value much larger than the observed on…

hep-th2011★ 1.2k cited

Generalized G-inflation: Inflation with the most general second-order field equations

Tsutomu Kobayashi, Masahide Yamaguchi, Jun'ichi Yokoyama

We study generalized Galileons as a framework to develop the most general single-field inflation models ever, Generalized G-inflation, containing yet further generalization of G-in…

hep-th2011★ 94 cited

Primordial non-Gaussianity from G-inflation

Tsutomu Kobayashi, Masahide Yamaguchi, Jun'ichi Yokoyama

We present a comprehensive study of primordial fluctuations generated from G-inflation, in which the inflaton Lagrangian is of the form with $X=-(\partialϕ)^…

astro-ph.CO2011★ 37 cited

f(R) Gravity and its Cosmological Implications

Hayato Motohashi, Alexei A. Starobinsky, Jun'ichi Yokoyama

We have investigated the evolution of a homogeneous isotropic background of the Universe and inhomogeneous subhorizon matter density perturbations in viable models of presen…