This is a modified version of the L-PICOLA code extending the COLA approach for simulating cosmological structure formation to theories that exhibit scale-dependent growth. It can compute matter power-spectra (CDM and total), redshift-space multipole power-spectra P0,P2,P4 and do halofinding on the fly. It can also include the effects of massive neutrinos on structure formation.

A R package for fitting Diagnostic Classification Modeling via Stan

Implementation of Puloon LCDM cash-dispensing unit protocol

Based on a Fortran code developed by Pier-Stefano Corasaniti (LUTH), the goal of this Python/C code is to provide an efficient yet easy to use library to compute the mass of the most massive galaxy cluster in a given redshift bin.

Gravity Resonance Threshold Theory - Code for paper. This compares MOND to NFW+LCDM to GRTT

Animations and plots illustrating homogeneous cosmology within different models

Section spéciale VLCC-La roue cosmique cinétique galactique et noyaux de figement inertiel

VLCC — Modèle d’espace-temps différentiel photonique de Vronsky - Recueil spéculatif complet -

Performing a test of timescape cosmology by comparing local galactic environmental structure against various age indicators.