Table 2 Same as in Tab. 1 but assuming no running in the (scalar) spectral index (i.e. αS = 0).
From: Stochastic backgrounds of relic gravitons: a theoretical appraisal
Data | r T | n s | α S | ΩΛ | ΩM0 | keqMpc |
|---|---|---|---|---|---|---|
WMAP5 alone | < 0.43 | 0.986 ± 0.22 | 0 |
|
| 0.00936 |
WMAP5 + Acbar | < 0.40 |
| 0 | 0.767 ± 0.032 | 0.233 ± 0.032 | 0.00944 |
WMAP5+ LSS + SN | < 0.20 | 0.968 ± 0.015 | 0 | 0.725 ± 0.015 | 0.275 ± 0.015 | 0.00999 |
WMAP5+ CMB data | < 0.36 | 0.979 ± 0.020 | 0 | 0.775 ± 0.032 | 0.225 ± 0.032 | 0.00922 |
