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20172026
most citedGeneralized multi-Galileons, covariantized new terms, and the no-go theorem for non-singular cosmologies

59 citations · 156 across the 12 of their papers we have counts for

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6 papers · 1 filter

gr-qc2024★ 9 cited

Parity violation in primordial tensor non-Gaussianities from matter bounce cosmology

Shingo Akama, Mian Zhu

It has been shown that primordial tensor non-Gaussianities from a cubic Weyl action with a non-dynamical coupling are suppressed by the so-called slow-roll parameter in a conventio…

gr-qc2023★ 1 cited

Imprints of primordial gravitational waves with non-Bunch-Davies initial states on CMB bispectra

Shingo Akama, Hiroaki W. H. Tahara

It has been shown that both scalar and tensor modes with non-Bunch-Davies initial states can enhance the amplitudes of the primordial bispectra compared to those with the Bunch-Dav…

gr-qc2022★ 11 cited

Primordial non-Gaussianity from Galilean Genesis without strong coupling problem

Shingo Akama, Shin'ichi Hirano

Galilean Genesis is generically plagued with a strong coupling problem, but this can be avoided depending on the hierarchy between a classical energy scale of genesis and a strong…

gr-qc2020★ 24 cited

Primordial tensor non-Gaussianities from general single-field inflation with non-Bunch-Davies initial states

Shingo Akama, Shin'ichi Hirano, Tsutomu Kobayashi

It has been found that the primordial non-Gaussianity of the curvature perturbation in the case of non-Bunch-Davies initial states can be enhanced compared with those in the case o…

gr-qc2019★ 24 cited

Primordial non-Gaussianities of scalar and tensor perturbations in general bounce cosmology: Evading the no-go theorem

Shingo Akama, Shin'ichi Hirano, Tsutomu Kobayashi

It has been pointed out that matter bounce cosmology driven by a k-essence field cannot satisfy simultaneously the observational bounds on the tensor-to-scalar ratio and non-Gaussi…

gr-qc2018★ 25 cited

General theory of cosmological perturbations in open and closed universes from the Horndeski action

Shingo Akama, Tsutomu Kobayashi

Our Universe is nearly spatially flat, but this does not mean that it is exactly spatially flat. In this paper we derive general quadratic actions for cosmological perturbations in…