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The expected rms bulk motion<br />
h V 2 (R *) i / Ω m 1.2 s dk P(k) W 2 (kR*)<br />
almost independent of the Cosmological Constant<br />
(<strong>Lahav</strong>, Lilje, Primack & Rees 91)<br />
Or Dark Energy (Wang & Steinhardt 98)<br />
In low density CDM smaller amplitude (σ 8 Ω m 0.6 ),<br />
larger coherence length (smaller Ω m h)<br />
than in SCDM
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