The paper derives a dark energy density of roughly (10^-3 eV)^4 from a mirror-symmetric model with a 10^-14 breaking scale, matching observation, but the derivation rests on a nonstandard vacuum-energy superposition assumption.
Measurements of Ω and Λ from 42 High- Redshift Supernovae,
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Dark energy and spontaneous mirror symmetry breaking
The paper derives a dark energy density of roughly (10^-3 eV)^4 from a mirror-symmetric model with a 10^-14 breaking scale, matching observation, but the derivation rests on a nonstandard vacuum-energy superposition assumption.