We previously discussed Verlinde's connection of the MOND acceleration scale to the entropy of de Sitter space. A different route appears in superfluid dark matter (a 2026 review is here ), where baryons interact with a phonon field whose nonlinear dynamics generate a MOND-like force. The superfluid theory introduces a characteristic scale $\Lambda_{\rm SF}$, which must be of order meV to reproduce the MOND scale. This is also the order of the vacuum-energy scale, $\rho_{\rm DE}^{1/4}\sim{\rm meV}$. So, we postulate $\Lambda_{\rm SF}^4=\rho_{\rm DE}$. To be clear, the idea of a unified dark sector is not new , e.g. a 2019 Unified Superfluid Dark Sector , 2026 A solid unification of the dark sector , and 2026 Unified dark sector approach to cosmological tensions among many others. What we do here is identify the MOND phonon scale exactly with vacuum energy, plus postulate a dimensionless infrared response coefficient. So, let $\...
Yes! Also, it is not the 'Planck Power' (despite what you might have read in Misner, Thorne and Wheeler, P.980). The existence of black hole horizons implies a maximum luminosity (power) limit in General Relativity. Not even gravitational waves can escape a black hole . Consider an (almost) black hole made of light (this is called a Kugelblitz ) sphere of radius \begin{equation} \notag R \geq \frac{2Gp}{c^3} \end{equation} which is filled with photons with a total mass-energy of momentum $p$ times speed of light $c$ \begin{equation} \notag E=p \ c \end{equation} the shortest time which the entire sphere can release its energy is its light-crossing time: \begin{equation} \notag t=R/c \end{equation} with average power (luminosity) $$ P = \frac{E}{t} \leq \frac{p \ c^2}{R}$$ So $$P_{max}=\frac{c^5}{2G}\approx 1.8\times10^{52} \ W$$ This is maximum power in GR , for a compact, casually connected emitter. ...