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DC Field | Value | Language |
---|---|---|
dc.contributor.author | Kehagias, A. | en |
dc.contributor.author | Tamvakis, K. | en |
dc.date.accessioned | 2015-11-24T18:33:37Z | - |
dc.date.available | 2015-11-24T18:33:37Z | - |
dc.identifier.issn | 0217-7323 | - |
dc.identifier.uri | https://olympias.lib.uoi.gr/jspui/handle/123456789/16765 | - |
dc.rights | Default Licence | - |
dc.subject | domain-wall | en |
dc.subject | extra dimension | en |
dc.subject | hierarchy | en |
dc.subject | gravity | en |
dc.title | A self-tuning solution of the cosmological constant problem | en |
heal.type | journalArticle | - |
heal.type.en | Journal article | en |
heal.type.el | Άρθρο Περιοδικού | el |
heal.identifier.secondary | <Go to ISI>://000178383300002 | - |
heal.identifier.secondary | http://www.worldscinet.com/mpla/17/1727/S0217732302008186.html | - |
heal.language | en | - |
heal.access | campus | - |
heal.recordProvider | Πανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιών | el |
heal.publicationDate | 2002 | - |
heal.abstract | We 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.journalName | Modern Physics Letters A | en |
heal.journalType | peer reviewed | - |
heal.fullTextAvailability | TRUE | - |
Appears in Collections: | Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά) |
Files in This Item:
File | Description | Size | Format | |
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tamvakis-2000-A self-tuning solution of the cosmological constant problem.pdf | 135.45 kB | Adobe PDF | View/Open Request a copy |
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