activity
20052009
most citedA Closure Theory for Non-linear Evolution of Cosmological Power Spectra

166 citations · 399 across the 8 of their papers we have counts for

collaborators

12 papers

astro-ph.CO200948 cited

Chasing the non-linear evolution of matter power spectrum with numerical resummation method: solution of closure equations

Takashi Hiramatsu, Atsushi Taruya

We present a new numerical scheme to treat the non-linear evolution of cosmological power spectra. Governing equations for matter power spectra have been previously derived by a no…

astro-ph.CO2009140 cited

Non-linear Evolution of Matter Power Spectrum in Modified Theory of Gravity

Kazuya Koyama, Atsushi Taruya, Takashi Hiramatsu

We present a formalism to calculate the non-linear matter power spectrum in modified gravity models that explain the late-time acceleration of the Universe without dark energy. Any…

cond-mat.str-el200713 cited

Four-dimensional CP U(1) lattice gauge theory for 3D antiferromagnets: Phase structure, gauge bosons and spin liquid

Kenji Sawamura, Takashi Hiramatsu, Katsuhiro Ozaki +2

In this paper we study the lattice CP model in (3+1) dimensions coupled with a dynamical compact U(1) gauge field. This model is an effective field theory of the $s={1 \over 2}…

astro-ph2007166 cited

A Closure Theory for Non-linear Evolution of Cosmological Power Spectra

Atsushi Taruya, Takashi Hiramatsu

We apply a non-linear statistical method in turbulence to the cosmological perturbation theory and derive a closed set of evolution equations for matter power spectra. The resultan…

astro-ph200712 cited

Scalar perturbations in braneworld cosmology

Antonio Cardoso, Takashi Hiramatsu, Kazuya Koyama +1

We study the behaviour of scalar perturbations in the radiation-dominated era of Randall-Sundrum braneworld cosmology by numerically solving the coupled bulk and brane master wave…

hep-th200610 cited

Numerical study of curvature perturbations in a brane-world inflation at high-energies

Takashi Hiramatsu, Kazuya Koyama

We study the evolution of scalar curvature perturbations in a brane-world inflation model in a 5D Anti-de Sitter spacetime. The inflaton perturbations are confined to a 4D brane bu…