Slow-roll inflation and CMB ansisotropy data

Color versions of the b/w figures in J.Martin, A.Riazuelo, and D.J.Schwarz, astro-ph/0006392:
Figure 1: Difference between power-law and slow-roll inflation
Figure 2: Error from wrong T/S for nonvanishing cosmological constant
Figure 3: Predictions of slow-roll for a SCDM model
Figure 4: Predictions of slow-roll for a LCDM model

Additional figures:
Inaccuracy of low-l tensor multipoles in CMBFAST and old versions of CAMB. Has been fixed in CAMB version July 2000.
As Figure 3, but exactly for the same values of the slow-roll parameters as in Figure 4.

Dominik J. Schwarz
Last modified: July 4, 2000