A self-tuning solution of the cosmological constant problem

dc.contributor.authorKehagias, A.en
dc.contributor.authorTamvakis, K.en
dc.date.accessioned2015-11-24T18:33:37Z
dc.date.available2015-11-24T18:33:37Z
dc.identifier.issn0217-7323-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/16765
dc.rightsDefault Licence-
dc.subjectdomain-wallen
dc.subjectextra dimensionen
dc.subjecthierarchyen
dc.subjectgravityen
dc.titleA self-tuning solution of the cosmological constant problemen
heal.abstractWe discuss the four-dimensional cosmological constant problem in a five-dimensional setting. A scalar field coupled to the SM forms dynamically a smooth brane with four-dimensional Poincare invariance, independently of SM physics. In this respect, our solution may be regarded as a self-tuning solution, free of any singularities and fine-tuning problems.en
heal.accesscampus-
heal.fullTextAvailabilityTRUE-
heal.identifier.secondary<Go to ISI>://000178383300002-
heal.identifier.secondaryhttp://www.worldscinet.com/mpla/17/1727/S0217732302008186.html-
heal.journalNameModern Physics Letters Aen
heal.journalTypepeer reviewed-
heal.languageen-
heal.publicationDate2002-
heal.recordProviderΠανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιώνel
heal.typejournalArticle-
heal.type.elΆρθρο Περιοδικούel
heal.type.enJournal articleen

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