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dc.contributor.authorDragović, Brankoen
dc.date.accessioned2020-12-11T13:04:46Z-
dc.date.available2020-12-11T13:04:46Z-
dc.date.issued2013-01-01en
dc.identifier.isbn9784431542698en
dc.identifier.issn2194-1009en
dc.identifier.urihttp://researchrepository.mi.sanu.ac.rs/handle/123456789/4458-
dc.description.abstractAbstract 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.publisherSpringer Link-
dc.relation.ispartofSpringer Proceedings in Mathematics and Statisticsen
dc.titleTowards p-Adic matter in the Universeen
dc.typeConference Paperen
dc.identifier.doi10.1007/978-4-431-54270-4_2en
dc.identifier.scopus2-s2.0-84883186682en
dc.relation.firstpage13en
dc.relation.lastpage24en
dc.relation.volume36en
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.openairetypeConference Paper-
item.cerifentitytypePublications-
item.fulltextNo Fulltext-
item.grantfulltextnone-
crisitem.author.orcid0000-0002-5818-0150-
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