Retrieving "Dark Energy Density Parameter" from the archives
Cross-reference notes under review
While the archivists retrieve your requested volume, browse these clippings from nearby entries.
-
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)