000408374 001__ 408374
000408374 005__ 20211110151247.0
000408374 010__ $$a
000408374 020__ $$a978-3-935702-83-6
000408374 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2013-04/weltman_amanda
000408374 0247_ $$2ISSN$$a1435-8077
000408374 037__ $$aPUBDB-2018-02827
000408374 041__ $$aEnglish
000408374 0881_ $$aDESY-PROC-2013-04
000408374 088__ $$2DESY$$aDESY-PROC-2013-04
000408374 1001_ $$0P:(DE-HGF)0$$aWeltman, A.$$b0$$eCorresponding author
000408374 1112_ $$0C13-06-24.5$$2inspire$$a9th Patras Workshop on Axions, WIMPs and WISPs$$cMainz$$d2013-06-24 - 2013-06-28$$gAXION-WIMP 2013$$wGermany
000408374 245__ $$aChameleon Fields Near and Far
000408374 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2013
000408374 29510 $$aWeltman, A. "Chameleon Fields Near and Far" in Proceedings, 9th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2013) / Oberlack, Uwe, Sissol, Pierre (eds.), 2013 ; AXION-WIMP 2013 : 9th Patras Workshop on Axions, WIMPs and WISPs , 2013-06-23 - 2013-06-28, Mainz
000408374 300__ $$a271-276
000408374 3367_ $$2ORCID$$aCONFERENCE_PAPER
000408374 3367_ $$033$$2EndNote$$aConference Paper
000408374 3367_ $$2BibTeX$$aINPROCEEDINGS
000408374 3367_ $$2DRIVER$$aconferenceObject
000408374 3367_ $$0PUB:(DE-HGF)29$$2PUB:(DE-HGF)$$aReport$$mreport
000408374 3367_ $$2DataCite$$aOutput Types/Conference Paper
000408374 3367_ $$0PUB:(DE-HGF)8$$2PUB:(DE-HGF)$$aContribution to a conference proceedings$$bcontrib$$mcontrib$$s1534322738_19235
000408374 3367_ $$0PUB:(DE-HGF)7$$2PUB:(DE-HGF)$$aContribution to a book$$mcontb
000408374 4900_ $$0PERI:(DE-600)2450075-6$$aDESY-PROC
000408374 520__ $$aIn this presentation we contemplate the problem of dark energy and advocate for a multi-faceted approach to studying its solution. Indeed it may be that, like the philosophers described above, we too cannot understand the nature of our beast by only touching one side of the problem. In particular we will study chameleon fields as a candidate for driving the observed acceleration of the universe and we will look how to test this theory through a varied approach as advocated here.
000408374 536__ $$0G:(DE-HGF)POF3-899$$a899 - ohne Topic (POF3-899)$$cPOF3-899$$fPOF III$$x0
000408374 588__ $$aDataset connected to GVK
000408374 650_7 $$0(DE-588)4220935-3$$2gnd$$aHypothetisches Teilchen
000408374 693__ $$0EXP:(DE-MLZ)NOSPEC-20140101$$5EXP:(DE-MLZ)NOSPEC-20140101$$eNo specific instrument$$x0
000408374 7870_ $$0PUBDB-2015-05816$$aOberlack, Uwe et. al.$$iisPartOf$$rDESY-PROC-2013-04$$tProceedings, 9th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2013)
000408374 8564_ $$uhttps://bib-pubdb1.desy.de/record/408374/files/fulltext.pdf$$yOpenAccess
000408374 909CO $$ooai:bib-pubdb1.desy.de:408374$$pdnbdelivery$$pdriver$$pVDB$$popen_access$$popenaire
000408374 9101_ $$aAff= University of Cape Town$$b0
000408374 9131_ $$0G:(DE-HGF)POF3-899$$1G:(DE-HGF)POF3-890$$2G:(DE-HGF)POF3-800$$3G:(DE-HGF)POF3$$4G:(DE-HGF)POF$$aDE-HGF$$bProgrammungebundene Forschung$$lohne Programm$$vohne Topic$$x0
000408374 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess
000408374 9201_ $$0I:(DE-H253)L-20120731$$kL$$lBibliothek und Dokumentation$$x0
000408374 980__ $$acontrib
000408374 980__ $$aVDB
000408374 980__ $$aUNRESTRICTED
000408374 980__ $$areport
000408374 980__ $$acontb
000408374 980__ $$aI:(DE-H253)L-20120731
000408374 9801_ $$aFullTexts