Table 1.
Summary of the main numerical and cosmological parameters characterising the subset of the DUSTGRAIN-pathfinder simulations considered in this work.
| Simulation name | Gravity type | |fR0| | ∑mν [eV] | ΩCDM | Ων |  [M⊙ h−1] |
 [M⊙ h−1] |
σ8 |
|---|---|---|---|---|---|---|---|---|
| ΛCDM | GR | – | 0 | 0.31345 | 0 | 8.1 × 1010 | 0 | 0.842 |
| fR4 | f(R) | 10−4 | 0 | 0.31345 | 0 | 8.1 × 1010 | 0 | 0.963 |
| fR5 | f(R) | 10−5 | 0 | 0.31345 | 0 | 8.1 × 1010 | 0 | 0.898 |
| fR6 | f(R) | 10−6 | 0 | 0.31345 | 0 | 8.1 × 1010 | 0 | 0.856 |
| fR4_0.3 eV | f(R) | 10−4 | 0.3 | 0.30630 | 0.00715 | 7.92 × 1010 | 1.85 × 109 | 0.887 |
| fR5_0.15 eV | f(R) | 10−5 | 0.15 | 0.30987 | 0.00358 | 8.01 × 1010 | 9.25 × 108 | 0.859 |
Notes. In the table, 
represents the neutrino simulation particle mass, 
represents the CDM simulation particle mass, while ΩCDM and Ων the CDM and neutrino density parameters, respectively. The listed σ8 values represent the linear power normalisation attained at z = 0, while all simulations are normalised to the same spectral amplitude As = 2.199 × 10−9 at the redshift of the CMB.
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