most citedPrimordial Curvature Fluctuation and Its Non-Gaussianity in Models with Modulated Reheating

176 citations · 504 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph2008176 cited

Primordial Curvature Fluctuation and Its Non-Gaussianity in Models with Modulated Reheating

Kazuhide Ichikawa, Teruaki Suyama, Tomo Takahashi +1

We investigate non-Gaussianity in the modulated reheating scenario where fluctuations of the decay rate of the inflaton generate adiabatic perturbations, paying particular attentio…

astro-ph200847 cited

Probing the Effective Number of Neutrino Species with Cosmic Microwave Background

Kazuhide Ichikawa, Toyokazu Sekiguchi, Tomo Takahashi

We discuss how much we can probe the effective number of neutrino species N_nu with cosmic microwave background alone. Using the data of WMAP, ACBAR, CBI and BOOMERANG experiments,…

astro-ph2008165 cited

Non-Gaussianity, Spectral Index and Tensor Modes in Mixed Inflaton and Curvaton Models

Kazuhide Ichikawa, Teruaki Suyama, Tomo Takahashi +1

We study non-Gaussianity, the spectral index of primordial scalar fluctuations and tensor modes in models where fluctuations from the inflaton and the curvaton can both contribute…

astro-ph200735 cited

Primordial Helium Abundance from CMB: a constraint from recent observations and a forecast

Kazuhide Ichikawa, Toyokazu Sekiguchi, Tomo Takahashi

We studied a constraint on the primordial helium abundance Y_p from current and future observations of CMB. Using the currently available data from WMAP, ACBAR, CBI and BOOMERANG,…

astro-ph20074 cited

Neutrino mass constraint from CMB and its degeneracy with other cosmological parameters

Kazuhide Ichikawa

We show that the cosmic microwave background (CMB) data of WMAP can give subelectronvolt limit on the neutrino mass: m_nu < 0.63 eV (95% CL). We also investigate its degeneracy wit…

astro-ph200713 cited

The Hubble constant and dark energy from cosmological distance measures

Kazuhide Ichikawa, Tomo Takahashi

We study how the determination of the Hubble constant from cosmological distance measures is affected by models of dark energy and vice versa. For this purpose, constraints on the…