Replacing dark energy by silent virialisation | Astronomy & Astrophysics (A&A)

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Fig. 6

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As in Fig. 5, measured global (above) and (below), which should be zero in the absence of numerical error (by Stokes’ theorem and Eq. (11)), shown as symbols, compared to S¹-based error estimators under independent Gaussian error propagation, , , shown as curves, for both models u₁ and u ₂.

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