activity
20022010
most citedEffect of the length of inflation on angular TT and TE power spectra in power-law inflation

10 citations · 22 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.CO2010

Non-Gaussianity and finite length inflation

Shiro Hirai, Tomoyuki Takami

In the present paper, certain inflation models are shown to have large non-Gaussianity in special cases. Namely, finite length inflation models with an effective higher derivative…

astro-ph.CO2009★ 1 cited

Scale dependence of the power spectrum of the curvature perturbation determined using a numerical method in slow-roll inflation

Shiro Hirai, Tomoyuki Takami

The Taylor expansion method has been used to investigate the scale dependence of the power spectrum of the curvature perturbation. In the present study, an alternative numerical me…

astro-ph2008★ 1 cited

Time dependence of cosmological and inflationary parameters in slow-roll inflation

Shiro Hirai, Tomoyuki Takami

The dependence of cosmological and inflationary parameters on time during the last 60 e-folds in inflation is investigated using a slow-roll inflation model. The time dependence of…

astro-ph2007

Effect of initial condition of inflation on power and angular power spectra in finite slow-roll inflation

Shiro Hirai, Tomoyuki Takami

The effect of the initial condition of inflation on the power spectra of scalar and tensor perturbations is estimated assuming a slow-roll inflation model. By defining a more gener…

astro-ph2006★ 1 cited

Angular Power Spectrum in Modular Invariant Inflation Model

Mitsuo J. Hayashi, Shiro Hirai, Tomoyuki Takami +3

We propose a scalar potential of inflation, motivated by modular invariant supergravity, and compute the angular power spectra of the adiabatic density perturbations that result fr…

hep-ph2006

Angular Power Spectrum and Dilatonic Inflation in Modular-Invariant Supergravity

Mitsuo J. Hayashi, Shiro Hirai, Yusuke Okame +1

The angular power spectrum is investigated in the model of supergravity, incorporating the target-space duality and the non-perturbative gaugino condensation in the hidden sector.…