Mirror World versus large extra dimensions

dc.creatorSilagadze, Z. K.
dc.date1999-08-02
dc.date2000-05-23
dc.date.accessioned2026-07-07T10:53:10Z
dc.date.available2026-07-07T10:53:10Z
dc.descriptionRecently proposed low scale quantum gravity scenario is expected to have a significant impact on the Mirror World hypothesis. Some aspects of this influence is investigated here, assuming that the fundamental gravity scale is near a TeV. It is shown that future colliders will be capable to produce the mirror matter, but an experimental signature, which will distinguish such events from the background, is unclear. The `smoking gun'' signals of the Mirror World would be an observation of decays like $Υ(2S)\to \tilde χ_{b2} γ$. But unfortunately the expected branching ratios are very small. Finally, it is shown that a mirror supernova will be quite a spectacular event for our world too, because a considerable amount of ordinary energy is expected to be emitted in the first several seconds.
dc.description12 pages, no figures, LaTeX, some typos corrected. Published in Mod. Phys. Lett. A14 (1999) 2321-2328
dc.identifierhttps://arxiv.org/abs/hep-ph/9908208
dc.identifierhttp://arxiv.org/abs/hep-ph/9908208
dc.identifierMod.Phys.Lett.A14:2321-2328,1999
dc.identifierdoi:10.1142/S0217732399002406
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/185394
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleMirror World versus large extra dimensions
dc.typetext

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