Why the cosmological constant goes to zero, and why we see it now
Why the cosmological constant goes to zero, and why we see it now. Quintessence. C.Wetterich. A.Hebecker, M.Doran, M.Lilley, J.Schwindt, C.M ü ller, G.Sch ä fer, E.Thommes, R.Caldwell, M.Bartelmann, K.Kharwan, G.Robbers, T.Dent, S.Steffen, L.Amendola, M.Baldi , N.Brouzakis , N.Tetradis,
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