PPT Slide

Detection Limits for Super-Hubble Suppression

A. Berera & A.F. Heavens Submitted PRD, 2000

Inflation/Defect models? Largest (Causal) Fluctuation Scale. Potentially useful constraint.

Detectable in CMB, even if larger than visible horizon

COBE data prefers small LCFS (Berera, Fang, Hinshaw, 1996, PRD)

MAP/Planck will improve detection (through better foreground subtraction/parameter determination)

Detectability for sub-visible Horizon LCFS

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