arXiv · hep-ph/9303252
A Shadow Matter Universe
Abstract
The cosmological and astrophysical implications of a shadow matter model which could also have interesting experimental consequences are examined. The model has identical microphysics for both the ordinary and shadow worlds but requires a macroscopic asymmetry from nucleosynthesis constraints. It is proposed that this macroscopic asymmetry can be generated at the quark-hadron phase transition.
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H. Lew. 1993-03-12. A Shadow Matter Universe. https://arxiv.org/abs/hep-ph/9303252
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