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Table 2.
Simulations and associated cosmological or gravitational models considered in this work.
| ELEPHANT | DAKAR | DEMNUni | ||||||||
|---|---|---|---|---|---|---|---|---|---|---|
| V = 5 × 1 h−3 Gpc3 | V = 1 h−3 Gpc3 | V = 8 h−3 Gpc3 | ||||||||
| Code | |fR0| | Ωrc | Code | w0 | wa | ξ [bn GeV−1] | Code | w0 | wa | ∑mν [eV] |
| F5 | 10−5 | – | w09 | −0.9 | 0 | 10 | CPL3 | −1.1 | −0.3 | 0.00 |
| F6 | 10−6 | – | w11 | −1.1 | 0 | 10 | CPL3-16 | −1.1 | −0.3 | 0.16 |
| N1 | – | 0.25 | CPL2 | −1.1 | 0.3 | 50 | CPL4 | −0.9 | 0.3 | 0.00 |
| N5 | – | 0.01 | – | – | – | – | CPL4-16 | −0.9 | 0.3 | 0.16 |
Notes. We show the volume of each simulation box, noting that for ELEPHANT we have five realisations. Further, each simulation set has a ΛCDM simulation with the same initial seeds as the beyond-ΛCDM simulations.
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