Retrieving "Dark Energy Density Parameter" from the archives

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  1. Accelerating Expansion Of The Universe

    Linked via "dark energy density parameter"

    | $\approx 1.0$ | Future Big Rip | $w < -1$ (Phantom Energy) | Infinite acceleration in finite time |
    Data from the Planck Surveyor missions consistently place the dark energy density parameter near $\Omega_{\Lambda} \approx 0.69$, leading to the standard $\Lambda$CDM model.
    The Vacuum Energy Paradox (The $\mathbf{10^{120}}$ Discrepancy)