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Kiyotomo Ichiki

Researcher at Nagoya University

Publications -  235
Citations -  7674

Kiyotomo Ichiki is an academic researcher from Nagoya University. The author has contributed to research in topics: Cosmic microwave background & Magnetic field. The author has an hindex of 43, co-authored 224 publications receiving 6409 citations. Previous affiliations of Kiyotomo Ichiki include National Taiwan University & National Institutes of Natural Sciences, Japan.

Papers
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The Japanese space gravitational wave antenna DECIGO

Seiji Kawamura, +144 more
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Gravitational Wave Spectrum Induced by Primordial Scalar Perturbations

TL;DR: In this paper, the authors derived the complete spectrum of gravitational waves induced by primordial scalar perturbations ranging over all observable wavelengths and showed that the spectrum is scale invariant on small scales, but has an interesting scale dependence on large and intermediate scales, where scalar-induced gravitational waves do not redshift and are hence enhanced relative to the background density of the Universe.
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The Japanese space gravitational wave antenna?DECIGO

Seiji Kawamura, +131 more
TL;DR: DECi-hertz Interferometer Gravitational wave Observatory (DECIGO) as discussed by the authors is the future Japanese space gravitational wave antenna, which aims at detecting various kinds of gravitational waves between 1 mHz and 100 Hz frequently enough to open a new window of observation for gravitational wave astronomy.
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LiteBIRD: A Satellite for the Studies of B-Mode Polarization and Inflation from Cosmic Background Radiation Detection

Masashi Hazumi, +164 more
TL;DR: LiteBIRD as mentioned in this paper is a candidate satellite for a strategic large mission of JAXA, which aims to map the polarization of the cosmic microwave background radiation over the full sky with unprecedented precision.
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The status of DECIGO

Shuichi Sato, +135 more
TL;DR: DECIGO (DECi-hertz Interferometer Gravitational wave Observatory) is the planned Japanese space gravitational wave antenna, aiming to detect gravitational waves from astrophysically and cosmologically significant sources mainly between 1 Hz and 10 Hz as mentioned in this paper.