001     172436
005     20250717112616.0
024 7 _ |2 doi
|a 10.1007/JHEP09(2014)053
024 7 _ |2 ISSN
|a 1029-8479
024 7 _ |2 ISSN
|a 1126-6708
024 7 _ |2 WOS
|a WOS:000347899000001
024 7 _ |2 inspire
|a inspire:1304305
024 7 _ |a altmetric:2480152
|2 altmetric
024 7 _ |a openalex:W3100649329
|2 openalex
037 _ _ |a PUBDB-2014-03735
082 _ _ |a 530
088 1 _ |a DESY-14-100; CPHT-RR037.0614
088 _ _ |a DESY-14-100
|2 DESY
088 _ _ |a CPHT-RR037.0614
|2 Other
100 1 _ |0 P:(DE-H253)PIP1003059
|a Buchmüller, Wilfried
|b 0
|e Corresponding Author
245 _ _ |a Large-field inflation and supersymmetry breaking
260 _ _ |a Berlin
|b Springer
|c 2014
336 7 _ |2 DRIVER
|a article
336 7 _ |2 DataCite
|a Output Types/Journal article
336 7 _ |0 PUB:(DE-HGF)29
|2 PUB:(DE-HGF)
|a Report
|m report
336 7 _ |0 PUB:(DE-HGF)16
|2 PUB:(DE-HGF)
|a Journal Article
|b journal
|m journal
|s 1480953445_710
336 7 _ |2 BibTeX
|a ARTICLE
336 7 _ |2 ORCID
|a JOURNAL_ARTICLE
336 7 _ |0 0
|2 EndNote
|a Journal Article
520 _ _ |a Large-field inflation is an interesting and predictive scenario. Its non-trivial embedding in supergravity was intensively studied in the recent literature, whereas its interplay with supersymmetry breaking has been less thoroughly investigated. We consider the minimal viable model of chaotic inflation in supergravity containing a stabilizer field, and add a Polonyi field. Furthermore, we study two possible extensions of the minimal setup. We show that there are various constraints: first of all, it is very hard to couple an O'Raifeartaigh sector with the inflaton sector, the simplest viable option being to couple them only through gravity. Second, even in the simplest model the gravitino mass is bounded from above parametrically by the inflaton mass. Therefore, high-scale supersymmetry breaking is hard to implement in a chaotic inflation setup. As a separate comment we analyze the simplest chaotic inflation construction without a stabilizer field, together with a supersymmetrically stabilized Kahler modulus. Without a modulus, the potential of such a model is unbounded from below. We show that a heavy modulus cannot solve this problem.
536 _ _ |0 G:(DE-HGF)POF2-514
|a 514 - Theoretical Particle Physics (POF2-514)
|c POF2-514
|f POF II
|x 0
536 _ _ |0 G:(EU-Grant)226371
|a MASSTEV - Mass hierarchy and particle physics at the TeV scale (226371)
|c 226371
|f ERC-2008-AdG
|x 1
536 _ _ |0 G:(DE-HGF)2015_IFV-VH-GS-500
|x 2
|c 2015_IFV-VH-GS-500
|a VH-GS-500 - PIER Helmholtz Graduate School (2015_IFV-VH-GS-500)
588 _ _ |a Dataset connected to CrossRef, bib-pubdb1.desy.de
650 _ 7 |2 INSPIRE
|a inflation: chaos
650 _ 7 |2 INSPIRE
|a supersymmetry: symmetry breaking
650 _ 7 |2 INSPIRE
|a gravitation: model
650 _ 7 |2 INSPIRE
|a mass: gravitation
650 _ 7 |2 INSPIRE
|a inflaton: mass
650 _ 7 |2 INSPIRE
|a gravitino: mass
650 _ 7 |2 INSPIRE
|a stability
650 _ 7 |2 INSPIRE
|a supergravity
650 _ 7 |2 INSPIRE
|a embedding
650 _ 7 |2 INSPIRE
|a Kaehler
650 2 0 |2 Author
|a Cosmology of Theories beyond the SM
650 2 0 |2 Author
|a Supersymmetry Breaking
693 _ _ |0 EXP:(DE-MLZ)NOSPEC-20140101
|5 EXP:(DE-MLZ)NOSPEC-20140101
|e No specific instrument
|x 0
700 1 _ |0 P:(DE-H253)PIP1022049
|a Dudas, Emilian
|b 1
700 1 _ |0 P:(DE-HGF)0
|a Heurtier, Lucien
|b 2
700 1 _ |0 P:(DE-H253)PIP1018677
|a Wieck, Clemens
|b 3
773 _ _ |0 PERI:(DE-600)2027350-2
|a 10.1007/JHEP09(2014)053
|g Vol. 2014, no. 9, p. 53
|n 9
|p 53
|t Journal of high energy physics
|v 2014
|x 1029-8479
|y 2014
856 4 _ |u https://bib-pubdb1.desy.de/record/172436/files/PUBDB-2014-03735.pdf
|y OpenAccess
856 4 _ |u https://bib-pubdb1.desy.de/record/172436/files/PUBDB-2014-03735.jpg?subformat=icon-1440
|x icon-1440
|y OpenAccess
856 4 _ |u https://bib-pubdb1.desy.de/record/172436/files/PUBDB-2014-03735.jpg?subformat=icon-180
|x icon-180
|y OpenAccess
856 4 _ |u https://bib-pubdb1.desy.de/record/172436/files/PUBDB-2014-03735.jpg?subformat=icon-640
|x icon-640
|y OpenAccess
909 C O |o oai:bib-pubdb1.desy.de:172436
|p openaire
|p open_access
|p driver
|p VDB
|p ec_fundedresources
|p dnbdelivery
910 1 _ |0 I:(DE-588b)2008985-5
|6 P:(DE-H253)PIP1003059
|a Deutsches Elektronen-Synchrotron
|b 0
|k DESY
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-H253)PIP1022049
|a Externes Institut
|b 1
|k Extern
910 1 _ |0 I:(DE-588b)2008985-5
|6 P:(DE-H253)PIP1018677
|a Deutsches Elektronen-Synchrotron
|b 3
|k DESY
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-H253)PIP1018677
|a Externes Institut
|b 3
|k Extern
913 2 _ |0 G:(DE-HGF)POF3-611
|1 G:(DE-HGF)POF3-610
|2 G:(DE-HGF)POF3-600
|a DE-HGF
|b Forschungsbereich Materie
|l Materie und Universum
|v Fundamental Particles and Forces
|x 0
913 1 _ |0 G:(DE-HGF)POF2-514
|1 G:(DE-HGF)POF2-510
|2 G:(DE-HGF)POF2-500
|a DE-HGF
|b Struktur der Materie
|l Elementarteilchenphysik
|v Theoretical Particle Physics
|x 0
|4 G:(DE-HGF)POF
|3 G:(DE-HGF)POF2
914 1 _ |y 2014
915 _ _ |0 StatID:(DE-HGF)0150
|2 StatID
|a DBCoverage
|b Web of Science Core Collection
915 _ _ |0 LIC:(DE-HGF)CCBY4
|2 HGFVOC
|a Creative Commons Attribution CC BY 4.0
915 _ _ |0 StatID:(DE-HGF)0100
|2 StatID
|a JCR
915 _ _ |0 StatID:(DE-HGF)0200
|2 StatID
|a DBCoverage
|b SCOPUS
915 _ _ |0 StatID:(DE-HGF)0110
|2 StatID
|a WoS
|b Science Citation Index
915 _ _ |0 StatID:(DE-HGF)0111
|2 StatID
|a WoS
|b Science Citation Index Expanded
915 _ _ |0 StatID:(DE-HGF)0510
|2 StatID
|a OpenAccess
915 _ _ |0 StatID:(DE-HGF)0010
|2 StatID
|a JCR/ISI refereed
915 _ _ |0 StatID:(DE-HGF)1020
|2 StatID
|a DBCoverage
|b Current Contents - Social and Behavioral Sciences
915 _ _ |0 StatID:(DE-HGF)0420
|2 StatID
|a Nationallizenz
915 _ _ |0 StatID:(DE-HGF)0199
|2 StatID
|a DBCoverage
|b Thomson Reuters Master Journal List
915 _ _ |0 StatID:(DE-HGF)0570
|2 StatID
|a SCOAP3
920 1 _ |0 I:(DE-H253)T-20120731
|k T
|l Theorie-Gruppe
|x 0
980 _ _ |a journal
980 _ _ |a VDB
980 _ _ |a report
980 _ _ |a I:(DE-H253)T-20120731
980 _ _ |a UNRESTRICTED
980 1 _ |a FullTexts


LibraryCollectionCLSMajorCLSMinorLanguageAuthor
Marc 21