As Lineweaver explained, because our Universe is expanding at an accelerating rate, our Universe has a cosmic event horizon (CEH).
Its an event horizon Jim, but not as we know it...Image credit: DALL.E2 by SR Anderson
Events beyond the CEH will never be observed. The CEH is also the source of de Sitter radiation, which has a specific temperature $T_{dS}$. It is the minimum possible temperature of the Universe, and, it is not absolute zero (zero Kelvins). Numerically $T_{dS} \approx 2.4 \times 10^{-30}K$, the universal minimum (black body) `absolute cold' local temperature of the future dS state. As a comparison, in 2020 the NASA Cold Atom lab was able to cool an atom to a record low $\sim 2 \times 10^{-7}K$.
Now, in any theory one may think of temperature as an energy, and from the semi-classical Unruh relationship, temperature $\sim$ acceleration. Therefore:
\begin{equation}
\notag
E_{dS} = T_{ds} \ k_B= \frac {\hslash a}{2\pi c}
\end{equation}
What we get from Unruh is $a=cH$, the universal background (local) minimum acceleration. $H$ is the future Hubble constant (as you probably know, this constant is not actually...constant). You could also express this as saying that our present Universe has a de Sitter attractor in our infinite far future.
Gibbons taught us that a theory with a minimum length should have a maximal acceleration and a maximal temperature. Now, we all know that in classical General Relativity (GR) there is no such thing as a minimum length. However, in most approaches to quantum gravity, which includes semi-classical approximations such as Hawking's black hole temperature and the Unruh relationship, there is such a beast.
Here of course, we are talking about the local minimum universal acceleration, which implies the existence of a maximum length scale, being the de Sitter characteristic length $l_{\Lambda}$ the future cosmic event horizon radius. Numerically $l_{\Lambda} \sim 16 \ Gly$. You can also write $l_{\Lambda} =\sqrt{ {3}/{\Lambda}}$, showing that the cosmological constant is the only parameter in dS space.
(Lambda, the symbol used for the cosmological constant)
The de Sitter horizon
A future de Sitter universe has a cosmic event horizon (CEH):
$
l_\Lambda = \sqrt{\frac{3}{\Lambda}} \sim 16 , \text{Gly}.
$
The associated Gibbons-Hawking temperature is:
$
T_{dS} = \frac{\hbar H}{2 \pi k_B}, \quad H = \sqrt{\frac{\Lambda}{3}}.
$
The corresponding minimum acceleration:
$
a_{\rm min} = c H.
$
CEH energy scale
The energy enclosed in the de Sitter horizon (using the Misner-Sharp energy in spherical symmetry) is approximately:
$
E_{\Lambda} = \frac{c^4}{2G} l_\Lambda.
$
This comes from the analogy with the Schwarzschild radius: $(R_s = 2 G M / c^2 \implies M = c^2 R_s / (2G))$.
Here $(R_s \to l_\Lambda)$ gives the “mass-energy” associated with the CEH.
So numerically:
$
E_\Lambda = \frac{c^4}{2 G} l_\Lambda.
$
Cosmic maximum power
If we imagine emission at the fastest rate allowed (light crossing time across the CEH):
$
t_\Lambda = \frac{l_\Lambda}{c}.
$
Then the average power is:
$
P_{\rm max}^{\rm CEH} = \frac{E_\Lambda}{t_\Lambda} = \frac{\frac{c^4}{2 G}
l_\Lambda}{l_\Lambda / c} = \frac{c^5}{2 G}.
$
It’s exactly the same as the black-hole horizon maximum power! The maximum luminosity allowed by causality in GR is set by horizon formation, whether it’s a black hole or the cosmic event horizon.


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