DC Field | Value | Language |
---|---|---|
dc.contributor.author | Dragović, Branko | en |
dc.date.accessioned | 2020-12-11T13:04:46Z | - |
dc.date.available | 2020-12-11T13:04:46Z | - |
dc.date.issued | 2013-01-01 | en |
dc.identifier.isbn | 9784431542698 | en |
dc.identifier.issn | 2194-1009 | en |
dc.identifier.uri | http://researchrepository.mi.sanu.ac.rs/handle/123456789/4458 | - |
dc.description.abstract | Abstract Starting from p-adic string theory with tachyons, we introduce a new kind of non-tachyonic matter which may play an important role in evolution of the Universe. This matter retains nonlocal and nonlinear p-adic string dynamics, but does not suffer of negative square mass. In space-time dimensions D = 2+4k, what includes D = 6, 10, ..., 26, the kinetic energy term also maintains correct sign. In these spaces this p-adicmatter provides negative cosmological constant and timedependent scalar field solution with negative potential. Their possible cosmological role is discussed. We have also connected non-locality with string world-sheet in effective Lagrangian for p-adic string. © Springer Japan 2013. | en |
dc.publisher | Springer Link | - |
dc.relation.ispartof | Springer Proceedings in Mathematics and Statistics | en |
dc.title | Towards p-Adic matter in the Universe | en |
dc.type | Conference Paper | en |
dc.identifier.doi | 10.1007/978-4-431-54270-4_2 | en |
dc.identifier.scopus | 2-s2.0-84883186682 | en |
dc.relation.firstpage | 13 | en |
dc.relation.lastpage | 24 | en |
dc.relation.volume | 36 | en |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Conference Paper | - |
item.cerifentitytype | Publications | - |
item.fulltext | No Fulltext | - |
item.grantfulltext | none | - |
crisitem.author.orcid | 0000-0002-5818-0150 | - |
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