Cosmological implication of antisymmetric tensor field on D-brane

Simple item page
dc.creatorCho, Inyong
dc.creatorChun, Eung Jin
dc.creatorKim, Hang Bae
dc.creatorKim, Yoonbai
dc.date2006-01-18
dc.date2006-07-04
dc.date.accessioned2026-07-07T10:29:50Z
dc.date.available2026-07-07T10:29:50Z
dc.descriptionWe discuss the cosmological implications of an antisymmetric tensor field when it experiences a kind of ``Higgs mechanism,'' including nonlocal interaction terms, on D-branes. Even when a huge magnetic-condensation-inducing anisotropy is assumed in the early universe, the expansion of the universe leads to an isotropic $B$-matter-dominated universe.
dc.description16 pages, 4 figures. To appear in the proceedings of the 9th Italian-Korean Symposium on Relativistic Astrophysics, Seoul, South Korea, and Mt. Kumgang, North Korea, 19-24 Jul. 2005. Submitted to J. Korean Phys. Soc. Minor corrections have been made. References have been added
dc.identifierhttps://arxiv.org/abs/hep-ph/0601147
dc.identifierhttp://arxiv.org/abs/hep-ph/0601147
dc.identifierJ.KoreanPhys.Soc.49:779-786,2006
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/177947
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleCosmological implication of antisymmetric tensor field on D-brane
dc.typetext

Files

Collections

arXiv