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 2026 review (Section 7.1) introduces a scale $\Lambda_{SF}$ and notes it needs to be in the order of meV to account for the MOND scale. So, we take this idea one step further and directly identify the characteristic phonon scale with the vacuum-energy scale! This converts the cosmological constant into a galactic acceleration scale and reproduces the baryonic Tully–Fisher relation. Throughout, set $c=\hbar=1$ and $M_{\rm Pl}^{-2}=8\pi G$, where $M_{\rm Pl}$ is the reduced Planck mass. Vacuum Scale Let $\Lambda_{\rm cos}$ denote the cosmological constant. Its vacuum-energy density is $\rho_\Lambda=M_{\rm Pl}^2\Lambda_{\rm cos}$. For a pure de Sitter universe, $H_\Lambda^2=\...
A Minimal Entropic Derivation of MOND-like Gravity Motivation Verlinde (2016) proposed that de Sitter space contains a volume-scaling entropy associated with dark energy. Matter removes part of this entropy. Beyond a critical scale, the remaining volume entropy dominates and produces an apparent dark gravitational component. Peach (2019) reformulated the idea using an entropic-screen construction. The argument below combines these ideas and fixes the force normalisation using Verlinde's spherical response coefficient. Competing Entropies For a sphere of radius $r$, the de Sitter entropy is $$S_{\rm DE}(r) = \frac{r}{L}\frac{A(r)c^3}{4G\hbar}, \qquad A(r)=4\pi r^2,$$ while a central mass $M$ removes $$S_M(r)=\frac{2\pi Mc}{\hbar}r.$$ Thus $S_{\rm DE}\propto r^3$ and $S_M\propto r$. Define $a_\Lambda=c^2/L$. Their ratio is $$\frac{S_{\rm DE}}{S_M} = \frac{a_\Lambda r^2}{2GM} = \left(\frac{r}{r_c}\right)^2,$$ where $$\boxed{r_c=\sqrt{\frac{2GM}{a_\...