guest ::
| Home > Publications database > Axion, axino and neutralino dark matter in minimal supergravity > print |
| Home > Publications database > Axion, axino and neutralino dark matter in minimal supergravity > print |
| 001 | 408349 | ||
| 005 | 20211110151243.0 | ||
| 010 | _ | _ | |a |
| 020 | _ | _ | |a 978-3-935702-83-6 |
| 024 | 7 | _ | |a 10.3204/DESY-PROC-2013-04/balazs_csaba |2 datacite_doi |
| 024 | 7 | _ | |a 1435-8077 |2 ISSN |
| 037 | _ | _ | |a PUBDB-2018-02802 |
| 041 | _ | _ | |a English |
| 088 | 1 | _ | |a DESY-PROC-2013-04 |
| 088 | _ | _ | |a DESY-PROC-2013-04 |2 DESY |
| 100 | 1 | _ | |a Balázs, C. |0 P:(DE-HGF)0 |b 0 |e Corresponding author |
| 111 | 2 | _ | |a 9th Patras Workshop on Axions, WIMPs and WISPs |c Mainz |d 2013-06-24 - 2013-06-28 |g AXION-WIMP 2013 |0 C13-06-24.5 |2 inspire |w Germany |
| 245 | _ | _ | |a Axion, axino and neutralino dark matter in minimal supergravity |
| 260 | _ | _ | |a Hamburg |c 2013 |b Verlag Deutsches Elektronen-Synchrotron |
| 295 | 1 | 0 | |a Balázs, C. "Axion, axino and neutralino dark matter in minimal supergravity" in Proceedings, 9th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2013) / Oberlack, Uwe, Sissol, Pierre (eds.), 2013 ; AXION-WIMP 2013 : 9th Patras Workshop on Axions, WIMPs and WISPs , 2013-06-23 - 2013-06-28, Mainz |
| 300 | _ | _ | |a 141-144 |
| 336 | 7 | _ | |a CONFERENCE_PAPER |2 ORCID |
| 336 | 7 | _ | |a Conference Paper |0 33 |2 EndNote |
| 336 | 7 | _ | |a INPROCEEDINGS |2 BibTeX |
| 336 | 7 | _ | |a conferenceObject |2 DRIVER |
| 336 | 7 | _ | |a Report |0 PUB:(DE-HGF)29 |2 PUB:(DE-HGF) |m report |
| 336 | 7 | _ | |a Output Types/Conference Paper |2 DataCite |
| 336 | 7 | _ | |a Contribution to a conference proceedings |b contrib |m contrib |0 PUB:(DE-HGF)8 |s 1533903868_2492 |2 PUB:(DE-HGF) |
| 336 | 7 | _ | |a Contribution to a book |0 PUB:(DE-HGF)7 |2 PUB:(DE-HGF) |m contb |
| 490 | 0 | _ | |a DESY-PROC |0 PERI:(DE-600)2450075-6 |
| 520 | _ | _ | |a Dark matter can be a mixture of axions, axinos and neutralinos in a Peccei-Quinn extension of supergravity. To find out which dark matter candidate is preferred by data we perform a Bayesian statistical analysis on four such scenarios. The main experimental constraints on these models come from the Planck satellite and from the Large Hadron Collider. Weaker constrains arise from other astrophysical, collider and low energy measurements. Our study reveals that the Peccei-Quinn scenario featuring axino dark matter is clearly preferred over the minimal supegravity model with neutralino dark matter. |
| 536 | _ | _ | |a 899 - ohne Topic (POF3-899) |0 G:(DE-HGF)POF3-899 |c POF3-899 |f POF III |x 0 |
| 588 | _ | _ | |a Dataset connected to GVK |
| 650 | _ | 7 | |a Hypothetisches Teilchen |0 (DE-588)4220935-3 |2 gnd |
| 693 | _ | _ | |0 EXP:(DE-MLZ)NOSPEC-20140101 |5 EXP:(DE-MLZ)NOSPEC-20140101 |e No specific instrument |x 0 |
| 700 | 1 | _ | |a Gupta, S. K. |0 P:(DE-HGF)0 |b 1 |
| 787 | 0 | _ | |a Oberlack, Uwe et. al. |0 PUBDB-2015-05816 |r DESY-PROC-2013-04 |i isPartOf |t Proceedings, 9th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2013) |
| 856 | 4 | _ | |u https://bib-pubdb1.desy.de/record/408349/files/fulltext.pdf |y OpenAccess |
| 909 | C | O | |o oai:bib-pubdb1.desy.de:408349 |p openaire |p open_access |p VDB |p driver |p dnbdelivery |
| 913 | 1 | _ | |a DE-HGF |b Programmungebundene Forschung |l ohne Programm |1 G:(DE-HGF)POF3-890 |0 G:(DE-HGF)POF3-899 |2 G:(DE-HGF)POF3-800 |v ohne Topic |x 0 |4 G:(DE-HGF)POF |3 G:(DE-HGF)POF3 |
| 915 | _ | _ | |a OpenAccess |0 StatID:(DE-HGF)0510 |2 StatID |
| 915 | _ | _ | |a Creative Commons Attribution CC BY 4.0 |0 LIC:(DE-HGF)CCBY4 |2 HGFVOC |
| 920 | 1 | _ | |0 I:(DE-H253)L-20120731 |k L |l Bibliothek und Dokumentation |x 0 |
| 980 | _ | _ | |a contrib |
| 980 | _ | _ | |a VDB |
| 980 | _ | _ | |a UNRESTRICTED |
| 980 | _ | _ | |a report |
| 980 | _ | _ | |a contb |
| 980 | _ | _ | |a I:(DE-H253)L-20120731 |
| 980 | 1 | _ | |a FullTexts |
| Library | Collection | CLSMajor | CLSMinor | Language | Author |
|---|