A Shadow Matter Universe

dc.creatorLew, H.
dc.date1993-03-12
dc.date.accessioned2026-07-07T03:55:58Z
dc.date.available2026-07-07T03:55:58Z
dc.descriptionThe 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.
dc.description11 pages (LaTeX), PURD-TH-93-04
dc.identifierhttps://arxiv.org/abs/hep-ph/9303252
dc.identifierhttp://arxiv.org/abs/hep-ph/9303252
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/44767
dc.subjectHigh Energy Physics - Phenomenology
dc.titleA Shadow Matter Universe
dc.typetext

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