
doi: 10.5281/zenodo.18881197 , 10.5281/zenodo.18868002 , 10.5281/zenodo.18868341 , 10.5281/zenodo.18877219 , 10.5281/zenodo.18865449 , 10.5281/zenodo.18880831 , 10.5281/zenodo.18868229 , 10.5281/zenodo.18879403 , 10.5281/zenodo.18877108 , 10.5281/zenodo.18877834 , 10.5281/zenodo.18865794 , 10.5281/zenodo.18867547 , 10.5281/zenodo.18867019 , 10.5281/zenodo.18882260 , 10.5281/zenodo.18866119 , 10.5281/zenodo.18879535
doi: 10.5281/zenodo.18881197 , 10.5281/zenodo.18868002 , 10.5281/zenodo.18868341 , 10.5281/zenodo.18877219 , 10.5281/zenodo.18865449 , 10.5281/zenodo.18880831 , 10.5281/zenodo.18868229 , 10.5281/zenodo.18879403 , 10.5281/zenodo.18877108 , 10.5281/zenodo.18877834 , 10.5281/zenodo.18865794 , 10.5281/zenodo.18867547 , 10.5281/zenodo.18867019 , 10.5281/zenodo.18882260 , 10.5281/zenodo.18866119 , 10.5281/zenodo.18879535
Physics currently treats the vacuum catastrophe, dark energy, and the Hubble tension as distinct crises. We propose they are symptoms of a single dimensional category error: modeling macroscopic expansion as a 3D bulk fluid rather than a 2D boundary tension. Evaluating equilibrium at radiative decoupling surfaces causes explicit mass dependence to cancel, yielding a purely geometric invariant: pi^3/15 ≈ 2.0671. Projecting this limit to the cosmic horizon gives the observed dark energy fraction, Omega_Lambda = pi^3/45 ≈ 0.6890, without tunable parameters. This predicts the acceleration onset, relaxes early dark matter requirements, and reframes the Hubble tension as geometry. Area-governs-volume is established in black holes and quantum boundary potentials; the universe may follow the same rule.
cosmology --- dark energy --- dark matter --- gravitation --- early universe --- galaxies: high-redshift
cosmology --- dark energy --- dark matter --- gravitation --- early universe --- galaxies: high-redshift
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