Table 1 The change in determination of the parameters of the tensor background for three different choices of cosmological data sets.
From: Stochastic backgrounds of relic gravitons: a theoretical appraisal
Data | r T | n s | α S | ΩΛ | ΩM0 | keqMpc |
|---|---|---|---|---|---|---|
WMAP5 alone | < 0.58 |
| -0.050 ± 0.034 |
|
| 0.00993 |
WMAP5 + Acbar | < 0.54 |
| -0.048 ± 0.027 |
|
| 0.01004 |
WMAP5 + LSS + SN | < 0.54 |
|
|
|
| 0.01008 |
WMAP5 + CMB data | < 0.64 |
|
|
|
| 0.01013 |
