activity
20172020
most citedGauge Independence of Induced Gravitational Waves

127 citations · 231 across the 3 of their papers we have counts for

collaborators

13 papers

astro-ph.CO202093 cited

NANOGrav results and LIGO-Virgo primordial black holes in axion-like curvaton model

Keisuke Inomata, Masahiro Kawasaki, Kyohei Mukaida +1

We discuss a possible connection between the recent NANOGrav results and the primordial black holes (PBHs) for the LIGO-Virgo events. In particular, we focus on the axion-like curv…

gr-qc2020

Analytic solutions of scalar perturbations induced by scalar perturbations

Keisuke Inomata

We study scalar perturbations induced by scalar perturbations through the non-linear interaction appearing at second order in perturbations. We derive analytic solutions of the ind…

astro-ph.CO2020

Standard Model Prediction for Cosmological 21cm Circular Polarization

Lingyuan Ji, Marc Kamionkowski, Keisuke Inomata

Before cosmic reionization, hydrogen atoms acquire a spin polarization quadrupole through interaction with the anisotropic 21-cm radiation field. The interaction of this quadrupole…

astro-ph.CO2020

Window function dependence of the novel mass function of primordial black holes

Koki Tokeshi, Keisuke Inomata, Jun'ichi Yokoyama

We investigate the ambiguity of the novel mass function of primordial black holes, which has succeeded in identifying the black hole mass in a given configuration of fluctuations,…

astro-ph.CO2020

Gravitational Wave Production right after a Primordial Black Hole Evaporation

Keisuke Inomata, Masahiro Kawasaki, Kyohei Mukaida +2

We discuss the footprint of evaporation of primordial black holes (PBHs) on stochastic gravitational waves (GWs) induced by scalar perturbations. We consider the case where PBHs on…

gr-qc2020127 cited

Gauge Independence of Induced Gravitational Waves

Keisuke Inomata, Takahiro Terada

We study gauge (in)dependence of the gravitational waves (GWs) induced from curvature perturbations. For the GWs produced in a radiation-dominated era, we find that the observable…