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Table 8.
Similar to Table 7, except that we now assume that the adiabatic and isocurvature modes are completely uncorrelated.
| Independent |
Joint |
|||||
|---|---|---|---|---|---|---|
| Shape | Cold dark matter | Neutrino density | Neutrino velocity | Cold dark matter | Neutrino density | Neutrino velocity |
| T a,aa…… | −0.1 ± 5.6 | −0.1 ± 5.6 | −0.1 ± 5.6 | −0.6 ± 5.7 | 15 ± 13 | −1.3 ± 5.8 |
| T i,ii…… | 110 ± 280 | −130 ± 250 | 270 ± 230 | 120 ± 290 | −710 ± 590 | 280 ± 240 |
| E a,aa…… | 48 ± 26 | 48 ± 26 | 48 ± 26 | 41 ± 27 | 33 ± 35 | 62 ± 35 |
| E i,ii…… | 1800 ± 1200 | 1900 ± 1100 | 170 ± 230 | 1400 ± 1200 | 1000 ± 1400 | −200 ± 300 |
| T+E a,aa…… | −2.5 ± 5.0 | −2.5 ± 5.0 | −2.5 ± 5.0 | −1.3 ± 5.1 | 11.4 ± 8.4 | −1.9 ± 5.2 |
| T+E i,ii…… | −290 ± 210 | −340 ± 210 | −51 ± 110 | −280 ± 210 | −710 ± 360 | −41 ± 120 |
Notes. Hence there are only two fNL parameters in this case, a purely adiabatic one and a purely isocurvature one.
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