Dark Energy represents one of the most intriguing mysteries of modern physics, and a challenge for the next generation of cosmological surveys. Among the wide range of models that have been proposed to explain the origin of Dark Energy, of its elusiveness, and of its many theoretical puzzles, an important class of models is represented by Coupled Quintessence scenarios. The CoDECS Project ( M. Baldi 2010, MNRAS 422) provided the first extended suite of cosmological simulations for this class of models.
Through the CoDECS project (Coupled Dark Energy Cosmological Simulations) we provide data from various suites of cosmological simulations of interacting Dark Energy models, focusing on the original Coupled Quintessence scenario featuring different possible forms of the self-interaction potential (as e.g. the exponential or the SUGRA potentials) and various forms of the Dark Energy coupling function. We performed simulations with different physical setups and specifications, classified as described below.
I'm in Section 1.
| MODEL | Link to snapshots |
|---|---|
| LCDM | text |
| EXP001 | text |
| EXP002 | text |
| EXP003 | text |
| EXP008e3 | text |
| SUGRA003 | text |
This section of the table contains links to halo catalogues
| Model | Link to SubFind catalogues | Link to ASCII catalogues |
|---|---|---|
| LCDM | text | text |
| EXP001 | text | text |
| EXP002 | text | text |
| EXP003 | text | text |
| EXP008e3 | text | text |
| SUGRA003 | text | text |
This section of the table contains links to VIDE Void Catalogues.
| MODEL | Link to VIDE catalogues |
|---|---|
| LCDM | text |
| EXP001 | text |
| EXP002 | text |
| EXP003 | text |
| EXP008e3 | text |
| SUGRA003 | text |
Baldi, M., "The CoDECS project: a publicly available suite of cosmological N-body simulations for interacting dark energy models", Monthly Notices of the Royal Astronomical Society, vol. 422, 2010. https://doi.org/10.1111/j.1365-2966.2012.20675.x