001     316739
005     20211110140505.0
020 _ _ |a 978-3-935702-43-0
024 7 _ |a 10.3204/DESY-PROC-2015-02/vinyoles_nuria
|2 datacite_doi
024 7 _ |a 1435-8077
|2 ISSN
037 _ _ |a PUBDB-2017-00137
041 _ _ |a English
100 1 _ |a Vinyoles, Nuria
|0 P:(DE-HGF)0
|b 0
111 2 _ |a 11th Patras Workshop on Axions, WIMPs and WISPs
|c Zaragoza
|d 2015-06-22 - 2015-06-26
|g AXION-WIMP 2015
|0 C15-06-22.2
|2 inspire
|w Spain
245 _ _ |a New Axion and Hidden Photon Constraints from a Solar Data Global Fit
260 _ _ |a Hamburg
|c 2015
|b Verlag Deutsches Elektronen-Synchrotron
295 1 0 |a Vinyoles, Nuria "New Axion and Hidden Photon Constraints from a Solar Data Global Fit" in Proceedings, 11th Patras Workshop on Axions, WIMPs and WISPs (Axion-WIMP 2015) / Irastorza, Igor G., Redondo, Javier, Carmona, José Manuel, Cebrian, Susana, Dafni, Theopisti, Iguaz, Francisco J., Luzon, Gloria (eds.), Verlag Deutsches Elektronen-Synchrotron : 2015 ; AXION-WIMP 2015 : 11th Patras Workshop on Axions, WIMPs and WISPs, 2015-06-22 - 2015-06-26, Zaragoza
300 _ _ |a 92-95
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 Output Types/Conference Paper
|2 DataCite
336 7 _ |a Contribution to a conference proceedings
|b contrib
|m contrib
|0 PUB:(DE-HGF)8
|s 1484729315_3886
|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 We present a new statistical analysis that combines helioseismology and solar neutrino observations to place upper limits to the properties of non standard weakly interacting particles. We present two applications to test the method: the well studied case of axions and the more novel case of low mass hidden photons. For axions we obtain an upper limit at $3\sigma$ for the axion-photon coupling constant of $g_{a\gamma}\,<\,4.1 \cdot 10^{-10} \rm{GeV^{-1}}$. For hidden photons we obtain the most restrictive upper limit available accross a wide range of masses for the product of the kinetic mixing and mass of $\chi m < 1.8 \cdot 10^{-12} \rm{eV}$ at $3\sigma$. Both cases improve the previous solar constraints based on the Standard Solar Models.
700 1 _ |a Serenelli, Aldo
|0 P:(DE-HGF)0
|b 1
700 1 _ |a Villante, Francesco
|0 P:(DE-HGF)0
|b 2
700 1 _ |a Basu, Sarbani
|0 P:(DE-HGF)0
|b 3
700 1 _ |a Redondo, Javier
|0 P:(DE-HGF)0
|b 4
700 1 _ |a Isern, Jordi
|0 P:(DE-HGF)0
|b 5
787 0 _ |a Irastorza, Igor G. et. al.
|d Verlag Deutsches Elektronen-Synchrotron
|i isPartOf
|0 PUBDB-2017-00118
|r DESY-PROC-2015-02
|t Proceedings, 11th Patras Workshop on Axions, WIMPs and WISPs (Axion-WIMP 2015)
856 4 _ |u https://bib-pubdb1.desy.de/record/316739/files/fulltext.pdf
|y OpenAccess
909 C O |o oai:bib-pubdb1.desy.de:316739
|p openaire
|p open_access
|p driver
|p dnbdelivery
910 1 _ |a Barcelona, IEEC
|0 I:(DE-HGF)0
|b 0
|6 P:(DE-HGF)0
910 1 _ |a Barcelona, IEEC
|0 I:(DE-HGF)0
|b 1
|6 P:(DE-HGF)0
910 1 _ |a L'Aquila U.
|0 I:(DE-HGF)0
|b 2
|6 P:(DE-HGF)0
910 1 _ |a Yale U.
|0 I:(DE-HGF)0
|b 3
|6 P:(DE-HGF)0
910 1 _ |a Zaragoza U.
|0 I:(DE-HGF)0
|b 4
|6 P:(DE-H253)PIP1006281
910 1 _ |a Barcelona, IEEC
|0 I:(DE-HGF)0
|b 5
|6 P:(DE-HGF)0
915 _ _ |a OpenAccess
|0 StatID:(DE-HGF)0510
|2 StatID
915 _ _ |a Hosted Content
|0 StatID:(DE-HGF)10000
|2 StatID
915 _ _ |a Creative Commons Attribution CC BY 4.0
|0 LIC:(DE-HGF)CCBY4
|2 HGFVOC
980 _ _ |a contrib
980 _ _ |a contb
980 _ _ |a I:(DE-H253)L-20120731
980 1 _ |a UNRESTRICTED
980 1 _ |a FullTexts


LibraryCollectionCLSMajorCLSMinorLanguageAuthor
Marc 21