The Effect of Extra Dimension on Dark Matter

dc.creatorOkada, Nobuchika
dc.creatorSeto, Osamu
dc.date2004-09-15
dc.date.accessioned2026-07-07T03:53:27Z
dc.date.available2026-07-07T03:53:27Z
dc.descriptionWe investigate the thermal relic density of a cold dark matter in the brane world cosmology. Since the expansion law in a high energy regime is modified from the one in the standard cosmology, if the dark matter decouples in such a high energy regime its relic number density is affected by this modified expansion law. We derive analytic formulas for the number density of the dark matter. It is found that the resultant relic density is characterized by the ``transition temperature'' at which the modified expansion law in the brane world cosmology is connecting with the standard one, and can be considerably enhanced compared to that in the standard cosmology, if the transition temperature is low enough. The implication to the neutralino dark matter also is mentioned.
dc.description4 pages, no figure, Prepared for 12th International Conference on Supersymmetry and Unification of Fundamental Interactions (SUSY 04), Tsukuba, Japan, 17-23 Jun 2004
dc.identifierhttps://arxiv.org/abs/hep-ph/0409170
dc.identifierhttp://arxiv.org/abs/hep-ph/0409170
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/43840
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleThe Effect of Extra Dimension on Dark Matter
dc.typetext

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