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  1. Accelerating Expansion Of The Universe

    Linked via "Planck Surveyor"

    | $\approx 1.0$ | 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)

  2. Big Bang Theory

    Linked via "Planck Surveyor"

    The CMB-radiation) is isotropic thermal radiation permeating all of space, considered the residual "afterglow" heat from the epoch of recombination), approximately $380,000$ years after the Big Bang. At this time, the Universe had cooled sufficiently (to around $3,000$ Kelvin) for electrons and protons to combine into neutral hydrogen atoms, allowing photons to decouple from the [plasma](/ent…

  3. Phantom Energy

    Linked via "Planck Surveyor"

    | Atoms/Nuclei | Strong Nuclear Force | $\sim 1$ (Final moment) |
    Observations utilizing the $\omega$ parameter are crucial for differentiating between the Big Freeze ($\omega=-1$) and the Big Rip ($\omega<-1$). Current cosmological data, such as that derived from the Cosmic Microwave Background (CMB) polarization analysis by the Planck Surveyor, consistently yield values for $\omega$ very close to $-1$, suggesting…