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19942026
most citedEffects of Cosmological Moduli Fields on Cosmic Microwave Background

851 citations · 5.2k across the 133 of their papers we have counts for

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Showing 2014Show all

9 papers · 1 filter

astro-ph.CO2014★ 36 cited

Constraints on warm dark matter from weak lensing in anomalous quadruple lenses

Kaiki Taro Inoue, Ryuichi Takahashi, Tomo Takahashi +1

We investigate the weak lensing effect by line-of-sight structures with a surface mass density of <~10^8 solar mass/arcsec^2 in QSO-galaxy quadruple lens systems. Using high-resolu…

astro-ph.CO2014★ 6 cited

Thermal Effects and Sudden Decay Approximation in the Curvaton Scenario

Naoya Kitajima, David Langlois, Tomo Takahashi +2

We study the impact of a temperature-dependent curvaton decay rate on the primordial curvature perturbation generated in the curvaton scenario. Using the familiar sudden decay appr…

astro-ph.CO2014★ 118 cited

Blue-tilted Tensor Spectrum and Thermal History of the Universe

Sachiko Kuroyanagi, Tomo Takahashi, Shuichiro Yokoyama

We investigate constraints on the spectral index of primordial gravitational waves (GWs), paying particular attention to a blue-tilted spectrum. Such constraints can be used to tes…

astro-ph.CO2014★ 34 cited

CMB distortion from primordial gravitational waves

Atsuhisa Ota, Tomo Takahashi, Hiroyuki Tashiro +1

We propose a new mechanism of generating the distortion in cosmic microwave background (CMB) originated from primordial gravitational waves. Such distortion is generated by…

astro-ph.CO2014★ 24 cited

Studying Inflation with Future Space-Based Gravitational Wave Detectors

Ryusuke Jinno, Takeo Moroi, Tomo Takahashi

Motivated by recent progress in our understanding of the -mode polarization of cosmic microwave background (CMB), which provides important information about the inflationary gra…

astro-ph.CO2014★ 6 cited

Probing Lepton Asymmetry with 21 cm Fluctuations

Kazunori Kohri, Yoshihiko Oyama, Toyokazu Sekiguchi +1

We investigate the issue of how accurately we can constrain the lepton number asymmetry xi_nu = mu_nu/T_nu in the Universe by using future observations of 21 cm line fluctuations a…