activity
20242026
collaborators

5 papers

astro-ph.CO2026

PySCo-EFT and ECOSMOG-EFT: a tandem of N-body simulation codes for the Effective Field Theory of Dark Energy

Himanish Ganjoo, Yann Rasera, Emilio Bellini +18

Modified gravity theories constitute viable alternatives to the standard cosmological model for explaining the observed late-time accelerated expansion of the Universe. The Effecti…

astro-ph.CO2025

On the shape of pancakes: catastrophe theory and Gaussian statistics in 2D

Abineet Parichha, Stephane Colombi, Shohei Saga +1

Cold dark matter (CDM) can be thought of as a 2D (or 3D) sheet of particles in 4D (or 6D) phase-space due to its negligible velocity dispersion. The large-scale structure, also cal…

astro-ph.CO2025

Post-collapse Lagrangian perturbation theory in three dimensions

Shohei Saga, Stéphane Colombi, Atsushi Taruya +2

The gravitational collapse of collisionless matter leads to shell-crossing singularities that challenge the applicability of standard perturbation theory. Here, we present the firs…

astro-ph.CO2025

Dark matter halo dynamics in 2D Vlasov Simulations: a self-similar approach

Abineet Parichha, Stephane Colombi, Shohei Saga +1

Understanding dark matter halo dynamics can be pivotal in unravelling the nature of dark matter particles. Analytical treatment of the multistream flows inside the turnaround regio…

astro-ph.CO2024

Soliton self-gravity and core-halo relation in fuzzy dark matter halos

Yusuke Manita, Takuya Takahashi, Atsushi Taruya

Fuzzy dark matter (FDM) is an attractive dark matter candidate composed of ultralight particles. In this paper, toward a clear understanding of the core-halo relation in the FDM ha…