activity
20082021
most citedSingle-field inflation, anomalous enhancement of superhorizon fluctuations, and non-Gaussianity in primordial black hole formation

131 citations · 260 across the 3 of their papers we have counts for

collaborators

10 papers

astro-ph.CO2021

Unified approach to secondary effects on the CMB B-mode polarization

Toshiya Namikawa, Atsushi Naruko, Ryo Saito +2

We develop a systematic and unified approach to estimate all possible secondary (i.e. non-primordial) nonlinear effects to the cosmic microwave background (CMB) polarization, named…

gr-qc2020

Dynamical Analysis of Screening in Scalar-Tensor Theory

Tomohiro Nakamura, Taishi Ikeda, Ryo Saito +2

We investigate linear and non-linear dynamics of spherically symmetric perturbations on a static configuration in scalar-tensor theories focusing on the chameleon screening mechani…

astro-ph.CO2020

Local gravity test of unified models of inflation and dark energy in gravity

Mai Yashiki, Nobuyuki Sakai, Ryo Saito

We consider gravity theories which unify inflation and dark energy models. First, from the final Planck data of the cosmic microwave background, we obtain a condition,…

hep-th201917 cited

Is Trans-Planckian Censorship a Swampland Conjecture?

Ryo Saito, Satoshi Shirai, Masahito Yamazaki

During an accelerated expansion of the Universe, quantum fluctuations of sub-Planckian size can be stretched outside the horizon and be regarded effectively classical. Recently, it…

hep-th2018

Phenomenological Consequences of the Refined Swampland Conjecture

Hajime Fukuda, Ryo Saito, Satoshi Shirai +1

We discuss phenomenological consequences of the recently-introduced refinements of the de Sitter swampland conjecture. The conjecture constraints the first and the second derivativ…

hep-th2018

Heavy Particle Signatures in Cosmological Correlation Functions with Tensor Modes

Ryo Saito, Takahiro Kubota

We explore the possibility to make use of cosmological data to look for signatures of unknown heavy particles whose masses are on the order of the Hubble parameter during the time…