Home > Publications database > Vacuum energy sequestering and conformal symmetry > print

001     221505
005     20211110131249.0
024 7 _ |a arXiv:1507.04158
|2 arXiv
024 7 _ |a altmetric:4281730
|2 altmetric
024 7 _ |a inspire:1382979
|2 inspire
037 _ _ |a PUBDB-2015-02692
041 _ _ |a English
088 1 _ |a DESY-15-119; ZMP-HH-15-20; arXiv:1507.04158
088 _ _ |a DESY-15-119
|2 DESY
088 _ _ |a ZMP-HH-15-20
|2 Other
088 _ _ |a arXiv:1507.04158
|2 arXiv
100 1 _ |a Ben-Dayan, Ido
|0 P:(DE-H253)PIP1018678
|b 0
|e Corresponding author
245 _ _ |a Vacuum energy sequestering and conformal symmetry
260 _ _ |c 2015
336 7 _ |a Preprint
|b preprint
|m preprint
|0 PUB:(DE-HGF)25
|s 1481027349_12010
|2 PUB:(DE-HGF)
336 7 _ |a WORKING_PAPER
|2 ORCID
336 7 _ |a Electronic Article
|0 28
|2 EndNote
336 7 _ |a preprint
|2 DRIVER
336 7 _ |a Report
|0 PUB:(DE-HGF)29
|2 PUB:(DE-HGF)
|m report
336 7 _ |a ARTICLE
|2 BibTeX
336 7 _ |a Output Types/Working Paper
|2 DataCite
520 _ _ |a In a series of recent papers Kaloper and Padilla proposed a mechanism to sequester standard model vacuum contributions to the cosmological constant. We study the consequences of embedding their proposal into a fully local quantum theory. In the original work, the bare cosmological constant $\Lambda$ and a scaling parameter $\lambda$ are introduced as global fields. We find that in the local case the resulting Lagrangian is that of a spontaneously broken conformal field theory where $\lambda$ plays the role of the dilaton. A vanishing or a small cosmological constant is thus a consequence of the underlying conformal field theory structure.
536 _ _ |0 G:(DE-HGF)POF3-611
|c POF3-611
|f POF III
|x 0
|a 611 - Fundamental Particles and Forces (POF3-611)
536 _ _ |0 G:(DE-HGF)2015_IFV-HZ-NG-603
|x 1
|c 2015_IFV-HZ-NG-603
|a HZ-NG-603 - Strings and Cosmology - an Interface for Testing fundamental Theories (2015_IFV-HZ-NG-603)
536 _ _ |a STRINGPHENOATLHC - String Phenomenology at the Era of LHC (328170)
|0 G:(EU-Grant)328170
|c 328170
|f FP7-PEOPLE-2012-IEF
|x 2
588 _ _ |a Dataset connected to INSPIRE
693 _ _ |0 EXP:(DE-MLZ)NOSPEC-20140101
|5 EXP:(DE-MLZ)NOSPEC-20140101
|e No specific instrument
|x 0
700 1 _ |a Richter, Robert
|0 P:(DE-H253)PIP1015074
|b 1
700 1 _ |a Ruehle, Fabian
|0 P:(DE-H253)PIP1020972
|b 2
700 1 _ |a Westphal, Alexander
|0 P:(DE-H253)PIP1013212
|b 3
856 4 _ |u https://bib-pubdb1.desy.de/record/221505/files/1507.04158v1.pdf
|y OpenAccess
856 4 _ |u https://bib-pubdb1.desy.de/record/221505/files/1507.04158v1.gif?subformat=icon
|x icon
|y OpenAccess
856 4 _ |u https://bib-pubdb1.desy.de/record/221505/files/1507.04158v1.jpg?subformat=icon-180
|x icon-180
|y OpenAccess
856 4 _ |u https://bib-pubdb1.desy.de/record/221505/files/1507.04158v1.jpg?subformat=icon-700
|x icon-700
|y OpenAccess
856 4 _ |u https://bib-pubdb1.desy.de/record/221505/files/1507.04158v1.pdf?subformat=pdfa
|x pdfa
|y OpenAccess
909 C O |o oai:bib-pubdb1.desy.de:221505
|p openaire
|p open_access
|p driver
|p VDB
|p ec_fundedresources
|p dnbdelivery
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 0
|6 P:(DE-H253)PIP1018678
910 1 _ |a Externes Institut
|0 I:(DE-HGF)0
|k >Extern
|b 1
|6 P:(DE-H253)PIP1015074
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 2
|6 P:(DE-H253)PIP1020972
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 3
|6 P:(DE-H253)PIP1013212
913 1 _ |a DE-HGF
|b Forschungsbereich Materie
|l Materie und Universum
|1 G:(DE-HGF)POF3-610
|0 G:(DE-HGF)POF3-611
|2 G:(DE-HGF)POF3-600
|x 0
|4 G:(DE-HGF)POF
|v Fundamental Particles and Forces
|3 G:(DE-HGF)POF3
914 1 _ |y 2015
915 _ _ |a OpenAccess
|0 StatID:(DE-HGF)0510
|2 StatID
915 _ _ |a Published
|0 StatID:(DE-HGF)0580
|2 StatID
920 1 _ |0 I:(DE-H253)T-20120731
|k T
|l Theorie-Gruppe
|x 0
980 _ _ |a preprint
980 _ _ |a VDB
980 _ _ |a report
980 _ _ |a I:(DE-H253)T-20120731
980 _ _ |a UNRESTRICTED
980 1 _ |a FullTexts

LibraryCollectionCLSMajorCLSMinorLanguageAuthor
Marc 21