activity
19942023
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations · 41.5k across the 168 of their papers we have counts for

collaborators

167 papers

astro-ph.CO2023★ 4 cited

The gravitational force field of proto-pancakes

Shohei Saga, Stéphane Colombi, Atsushi Taruya

It is well known that the first structures that form from small fluctuations in a self-gravitating, collisionless and initially smooth cold dark matter (CDM) fluid are pancakes. We…

astro-ph.CO2023★ 4 cited

Fast and accurate collapse-time predictions for collisionless matter

Cornelius Rampf, Shohei Saga, Atsushi Taruya +1

We consider the gravitational collapse of collisionless matter seeded by three crossed sine waves with various amplitudes, also in the presence of a linear external tidal field. We…

astro-ph.CO2022★ 11 cited

LyMAS reloaded: improving the predictions of the large-scale Lyman-α forest statistics from dark matter density and velocity fields

S. Peirani, S. Prunet, S. Colombi +6

We present LyMAS2, an improved version of the "Lyman-α Mass Association Scheme" aiming at predicting the large-scale 3d clustering statistics of the Lyman-α forest (Ly-α) from mode…

astro-ph.CO2021★ 11 cited

Cold dark matter protohalo structure around collapse: Lagrangian cosmological perturbation theory versus Vlasov simulations

Shohei Saga, Atsushi Taruya, Stéphane Colombi

We explore the structure around shell-crossing time of cold dark matter protohaloes seeded by two or three crossed sine waves of various relative initial amplitudes, by comparing L…

astro-ph.CO2020★ 34 cited

Phase-space structure of protohalos: Vlasov versus Particle-Mesh

Stéphane Colombi

The phase-space structure of primordial dark matter halos is revisited using cosmological simulations with three sine waves and Cold Dark Matter (CDM) initial conditions. The simul…

astro-ph.CO2020★ 6 cited

Power spectrum response of large-scale structure in 1D and in 3D: tests of prescriptions for post-collapse dynamics

Anaëlle Halle, Takahiro Nishimichi, Atsushi Taruya +2

The power spectrum response function of the large-scale structure of the Universe describes how the evolved power spectrum is modified by a small change in initial power through no…