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19942025
most citedRevising the Halofit Model for the Nonlinear Matter Power Spectrum

1.1k citations · 10k across the 165 of their papers we have counts for

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Showing 2018Show all

8 papers · 1 filter

astro-ph.CO2018★ 14 cited

CMB lensing bi-spectrum: assessing analytical predictions against full-sky lensing simulations

Toshiya Namikawa, Benjamin Bose, François R. Bouchet +2

Cosmic microwave background (CMB) lensing is an integrated effect whose kernel is greater than half the peak value in the range . Measuring this effect offers a powerful too…

astro-ph.CO2018★ 31 cited

Perturbation theory challenge for cosmological parameters estimation: Matter power spectrum in real space

Ken Osato, Takahiro Nishimichi, Francis Bernardeau +1

We study the accuracy with which cosmological parameters can be determined from real space power spectrum of matter density contrast at weakly nonlinear scales using analytical app…

astro-ph.CO2018★ 42 cited

The one-loop matter bispectrum as a probe of gravity and dark energy

Benjamin Bose, Atsushi Taruya

Gravity-induced non-Gaussianity in the large-scale structure of the Universe, characterised by higher-order statistics such as the bispectrum (three-point cumulant), is expected to…

astro-ph.CO2018★ 52 cited

GridSPT: Grid-based calculation for perturbation theory of large-scale structure

Atsushi Taruya, Takahiro Nishimichi, Donghui Jeong

Perturbation theory (PT) calculation of large-scale structure has been used to interpret the observed non-linear statistics of large-scale structure at the quasi-linear regime. In…

astro-ph.CO2018★ 19 cited

The CMB lensing bi-spectrum as a probe of modified gravity theories

Toshiya Namikawa, François R. Bouchet, Atsushi Taruya

Cosmological structures grow differently in theories of gravity which are modified as compared to Einstein's General relativity (GR). Cosmic microwave background (CMB) fluctuation…

astro-ph.CO2018★ 30 cited

Lagrangian cosmological perturbation theory at shell-crossing

Shohei Saga, Atsushi Taruya, Stéphane Colombi

We consider the growth of primordial dark matter halos seeded by three crossed initial sine waves of various amplitudes. Using a Lagrangian treatment of cosmological gravitational…