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At one time the extreme flatness (Omega = 1) required at early epochs in order that the universe be even approximately flat now might have been regarded as fine tuning. But its very fineness spoke of a mechanistic explanation, such as is provided by inflation theory. It is possible that a mechanistic explanation may ultimately be forthcoming for the apparent extreme tuning of the cosmological constant, Lamda, although a revolution in fundamental physics is probably required to achieve it, Albrecht et al (2006). Alternatively, the fine tuning of Lamda may be an observer selection effect, Martel et al (1997), Weinberg (2005), Lineweaver (2007), Egan (2010). BRADFORD (2010)
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