| Home > Publications database > Phenomenology of a Supersymmetric Model Inspired by Inflation > print |
| 001 | 473742 | ||
| 005 | 20250724180017.0 | ||
| 024 | 7 | _ | |a 10.1140/epjc/s10052-021-08869-4 |2 doi |
| 024 | 7 | _ | |a Hollik:2020plc |2 INSPIRETeX |
| 024 | 7 | _ | |a inspire:1793570 |2 inspire |
| 024 | 7 | _ | |a 1434-6044 |2 ISSN |
| 024 | 7 | _ | |a 1434-6052 |2 ISSN |
| 024 | 7 | _ | |a arXiv:2004.14852 |2 arXiv |
| 024 | 7 | _ | |a 10.3204/PUBDB-2022-00222 |2 datacite_doi |
| 024 | 7 | _ | |a altmetric:99861600 |2 altmetric |
| 024 | 7 | _ | |a WOS:000618312200003 |2 WOS |
| 024 | 7 | _ | |a openalex:W3127454881 |2 openalex |
| 037 | _ | _ | |a PUBDB-2022-00222 |
| 041 | _ | _ | |a English |
| 082 | _ | _ | |a 530 |
| 088 | _ | _ | |a arXiv:2004.14852 |2 arXiv |
| 088 | _ | _ | |a DESY-20-059 |2 DESY |
| 088 | _ | _ | |a TTP-2020-017 |2 Other |
| 088 | _ | _ | |a P3H-20-013 |2 Other |
| 100 | 1 | _ | |a Hollik, Wolfgang Gregor |0 P:(DE-H253)PIP1027468 |b 0 |
| 245 | _ | _ | |a Phenomenology of a Supersymmetric Model Inspired by Inflation |
| 260 | _ | _ | |a Heidelberg |c 2021 |b Springer |
| 336 | 7 | _ | |a article |2 DRIVER |
| 336 | 7 | _ | |a Output Types/Journal article |2 DataCite |
| 336 | 7 | _ | |a Journal Article |b journal |m journal |0 PUB:(DE-HGF)16 |s 1719325693_1973039 |2 PUB:(DE-HGF) |
| 336 | 7 | _ | |a ARTICLE |2 BibTeX |
| 336 | 7 | _ | |a JOURNAL_ARTICLE |2 ORCID |
| 336 | 7 | _ | |a Journal Article |0 0 |2 EndNote |
| 500 | _ | _ | |a The European Physical Journal C volume 81, Article number: 141 (2021). 21 pages, 10 figures; v2 matches published version |
| 520 | _ | _ | |a The current challenges in high energy physics and cosmology are to build coherent particle physics models to describe the phenomenology at colliders in the laboratory and the observations in the universe. From these observations, the existence of an inflationary phase in the early universe gives guidance for particle physics models. We study a supersymmetric model which incorporates successfully inflation by a non-minimal coupling to supergravity and shows a unique collider phenomenology. Motivated by experimental data, we set a special emphasis on a new singlet-like state at $97\,\text {GeV}$ and single out possible observables for a future linear collider that permit a distinction of the model from a similar scenario without inflation. We define a benchmark scenario that is in agreement with current collider and Dark Matter constraints, and study the influence of the non-minimal coupling on the phenomenology. Measuring the singlet-like state with high precision on the percent level seems to be promising for resolving the models, even though the Standard Model-like Higgs couplings deviate only marginally. However, a hypothetical singlet-like state with couplings of about $20\,\%$ compared to a Standard Model Higgs at $97\,\text {GeV}$ encourages further studies of such footprint scenarios of inflation. |
| 536 | _ | _ | |a 611 - Fundamental Particles and Forces (POF4-611) |0 G:(DE-HGF)POF4-611 |c POF4-611 |f POF IV |x 0 |
| 536 | _ | _ | |a DFG project 390833306 - EXC 2121: Quantum Universe (390833306) |0 G:(GEPRIS)390833306 |c 390833306 |x 1 |
| 588 | _ | _ | |a Dataset connected to CrossRef, INSPIRE, Journals: bib-pubdb1.desy.de |
| 650 | _ | 7 | |a coupling: nonminimal |2 INSPIRE |
| 650 | _ | 7 | |a coupling: Higgs |2 INSPIRE |
| 650 | _ | 7 | |a inflation: model |2 INSPIRE |
| 650 | _ | 7 | |a cosmological model: parameter space |2 INSPIRE |
| 650 | _ | 7 | |a linear collider |2 INSPIRE |
| 650 | _ | 7 | |a supersymmetry |2 INSPIRE |
| 650 | _ | 7 | |a supergravity |2 INSPIRE |
| 650 | _ | 7 | |a dark matter: parametrization |2 INSPIRE |
| 650 | _ | 7 | |a coherence |2 INSPIRE |
| 650 | _ | 7 | |a benchmark |2 INSPIRE |
| 693 | _ | _ | |0 EXP:(DE-MLZ)NOSPEC-20140101 |5 EXP:(DE-MLZ)NOSPEC-20140101 |e No specific instrument |x 0 |
| 700 | 1 | _ | |a Li, Cheng |0 P:(DE-H253)PIP1086677 |b 1 |u desy |
| 700 | 1 | _ | |a Moortgat-Pick, Gudrid |0 P:(DE-H253)PIP1011115 |b 2 |e Corresponding author |
| 700 | 1 | _ | |a Paasch, Steven |0 P:(DE-H253)PIP1086678 |b 3 |u desy |
| 773 | _ | _ | |a 10.1140/epjc/s10052-021-08869-4 |g Vol. 81, no. 2, p. 141 |0 PERI:(DE-600)1459069-4 |n 2 |p 141 |t The European physical journal / C |v 81 |y 2021 |x 1434-6044 |
| 787 | 0 | _ | |a Hollik, Wolfgang Gregor et.al. |d 2020 |i IsParent |0 PUBDB-2020-01799 |r arXiv:2004.14852 ; DESY-20-059 ; TTP-2020-017 ; P3H-20-013 |t Phenomenology of a Supersymmetric Model Inspired by Inflation |
| 856 | 4 | _ | |u https://bib-pubdb1.desy.de/record/473742/files/Hollik2021_Article_PhenomenologyOfASupersymmetric.pdf |y OpenAccess |
| 856 | 4 | _ | |u https://bib-pubdb1.desy.de/record/473742/files/Hollik2021_Article_PhenomenologyOfASupersymmetric.pdf?subformat=pdfa |x pdfa |y OpenAccess |
| 909 | C | O | |o oai:bib-pubdb1.desy.de:473742 |p openaire |p open_access |p VDB |p driver |p dnbdelivery |
| 910 | 1 | _ | |a External Institute |0 I:(DE-HGF)0 |k Extern |b 0 |6 P:(DE-H253)PIP1027468 |
| 910 | 1 | _ | |a Deutsches Elektronen-Synchrotron |0 I:(DE-588b)2008985-5 |k DESY |b 1 |6 P:(DE-H253)PIP1086677 |
| 910 | 1 | _ | |a Deutsches Elektronen-Synchrotron |0 I:(DE-588b)2008985-5 |k DESY |b 2 |6 P:(DE-H253)PIP1011115 |
| 910 | 1 | _ | |a Deutsches Elektronen-Synchrotron |0 I:(DE-588b)2008985-5 |k DESY |b 3 |6 P:(DE-H253)PIP1086678 |
| 913 | 1 | _ | |a DE-HGF |b Forschungsbereich Materie |l Matter and the Universe |1 G:(DE-HGF)POF4-610 |0 G:(DE-HGF)POF4-611 |3 G:(DE-HGF)POF4 |2 G:(DE-HGF)POF4-600 |4 G:(DE-HGF)POF |v Fundamental Particles and Forces |x 0 |
| 914 | 1 | _ | |y 2021 |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)0200 |2 StatID |b SCOPUS |d 2021-01-27 |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)0160 |2 StatID |b Essential Science Indicators |d 2021-01-27 |
| 915 | _ | _ | |a Creative Commons Attribution CC BY 4.0 |0 LIC:(DE-HGF)CCBY4 |2 HGFVOC |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)0600 |2 StatID |b Ebsco Academic Search |d 2021-01-27 |
| 915 | _ | _ | |a JCR |0 StatID:(DE-HGF)0100 |2 StatID |b EUR PHYS J C : 2019 |d 2021-01-27 |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)0501 |2 StatID |b DOAJ Seal |d 2021-01-27 |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)0500 |2 StatID |b DOAJ |d 2021-01-27 |
| 915 | _ | _ | |a WoS |0 StatID:(DE-HGF)0113 |2 StatID |b Science Citation Index Expanded |d 2021-01-27 |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)0199 |2 StatID |b Clarivate Analytics Master Journal List |d 2021-01-27 |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)0150 |2 StatID |b Web of Science Core Collection |d 2021-01-27 |
| 915 | _ | _ | |a IF < 5 |0 StatID:(DE-HGF)9900 |2 StatID |d 2021-01-27 |
| 915 | _ | _ | |a OpenAccess |0 StatID:(DE-HGF)0510 |2 StatID |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)0571 |2 StatID |b SCOAP3 sponsored Journal |d 2021-01-27 |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)1150 |2 StatID |b Current Contents - Physical, Chemical and Earth Sciences |d 2021-01-27 |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)0300 |2 StatID |b Medline |d 2021-01-27 |
| 915 | _ | _ | |a Nationallizenz |0 StatID:(DE-HGF)0420 |2 StatID |d 2021-01-27 |w ger |
| 915 | _ | _ | |a Peer Review |0 StatID:(DE-HGF)0030 |2 StatID |b ASC |d 2021-01-27 |
| 915 | _ | _ | |a SCOAP3 |0 StatID:(DE-HGF)0570 |2 StatID |
| 920 | 1 | _ | |0 I:(DE-H253)FLC-20120731 |k FLC |l Experimente an Lepton Collidern |x 0 |
| 980 | _ | _ | |a journal |
| 980 | _ | _ | |a VDB |
| 980 | _ | _ | |a I:(DE-H253)FLC-20120731 |
| 980 | _ | _ | |a UNRESTRICTED |
| 980 | 1 | _ | |a FullTexts |
| Library | Collection | CLSMajor | CLSMinor | Language | Author |
|---|