Summary
Following a previous unified classical approach to gravitational and strong interactions, we associate the interior of hadrons with a homogeneous isotropic cosmology. We derive some hadronic properties from our model and from the corresponding (« scaled down ») Friedmann equations.
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Work partially supported by C’ N.R. and by M.P.I.
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Italiano, A., Recami, E. Friedmann cosmology and hadron properties. Lett. Nuovo Cimento 40, 140–144 (1984). https://doi.org/10.1007/BF02747114
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DOI: https://doi.org/10.1007/BF02747114