Physics – High Energy Physics – High Energy Physics - Theory
Scientific paper
2003-02-01
Mod.Phys.Lett.A19:801,2004
Physics
High Energy Physics
High Energy Physics - Theory
9 pages LaTeX. Significantly rewritten (including abstract)
Scientific paper
10.1142/S0217732304013866
Precision cosmological data hint that a dark energy with equation of state $w = P/\rho < -1$ and hence dubious stability is viable. Here we discuss for any $w$ nucleation from $\Lambda > 0$ to $\Lambda = 0$ in a first-order phase transition. The critical radius is argued to be at least of galactic size and the corresponding nucleation rate is glacial, thus underwriting the dark energy's stability and rendering remote any microscopic effect.
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