This theorem proposes a fundamental equation of state for the de Sitter vacuum, linking its thermodynamic energy directly to its quantum-gravitational uncertainty. Let the de Sitter cosmological horizon be described by: 1. Its thermodynamic energy \(E_{\text{th}}\), the unique energy that satisfies the first law of thermodynamics, \(dE_{\text{th}} = T\,dS\). 2. Its intrinsic quantum position uncertainty (or "fuzziness"), \(\Delta x\), arising from quantum gravitational effects. The rate of change of the thermodynamic energy with respect to the area of this quantum uncertainty, \(A_{\text{unc}} = \Delta x^2\), is a universal constant equal to the Planck pressure, \(P_{\text{Pl}}\). Mathematically: $$\frac{dE_{\text{th}}}{d(\Delta x^2)} = \frac{\hbar c^7}{G^2} \equiv P_{\text{Pl}}$$ Derivation The theorem is derived by combining three principles: 1. Thermodynamic Energy: The Brown-York energy is the correct thermodynamic potential, given as a function of the de Sitter radius ...
A 2021 paper by Zurek applied a random walk argument to a black hole horizon. Credit, Zurek, 2021 Zurek called this a blurring of the horizon (a fuzzy, or uncertain horizon), and also went through some equivalent derivations, which basically supported the idea this length scale is the quantum uncertainty in the position of the BH horizon, aka a dynamic quantum width of an event horizon (a concept which would therefore also apply to the universe's own CEH). The Bekenstein-Hawking entropy gives the number of quantum degrees of freedom that can fluctuate. Below, we step out our own cosmic de-Sitter derivation of the random walk argument, obtaining the same result as Zurek did, so its certainly correct! \begin{equation} \Delta x^2 =2 DT \end{equation} In this equation, $\Delta x$ is the position uncertainty, $D$ is the Einstein diffusion coefficient and $T$ is the time between measurements (aka the relaxation time). So, lets look at the Einstein diffusion co...