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Conclusions - in the Trio’s own words…<br />
● “Although a spherically symmetric Great<br />
Attractor model fits the present data well…it is<br />
dangerous to use it for cosmology.” (Faber &<br />
Burstein 1988)<br />
● “CDM still does the best job, but there are many,<br />
many unresolved issues.” (Blumenthal 1987)<br />
● “The total neutrino mass could be comparable to<br />
that of the visible stars in the universe, or perhaps<br />
even larger.” (Primack 2001)