000315513 001__ 315513
000315513 005__ 20211110140136.0
000315513 020__ $$a978-3-935702-59-1
000315513 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2014-03/mantry_sonny
000315513 0247_ $$2ISSN$$a1435-8077
000315513 037__ $$aPUBDB-2016-05920
000315513 041__ $$aEnglish
000315513 1001_ $$0P:(DE-HGF)0$$aMantry, Sonny $$b0
000315513 1112_ $$0C14-06-29.1$$2inspire$$a10th Patras Workshop on Axions, WIMPs and WISPs$$cGeneva$$d2014-06-29 - 2014-07-04$$gAXION-WIMP 2014$$wSwitzerland
000315513 245__ $$aDifferences between Axions and Generic Light Scalars in Laboratory Experiments
000315513 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2014
000315513 29510 $$aMantry, Sonny "Differences between Axions and Generic Light Scalars in Laboratory Experiments" in Proceedings, 10th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2014)  / Tsesmelis, Emmanuel, Maroudas, Marios (eds.), Verlag Deutsches Elektronen-Synchrotron : 2014 ; AXION-WIMP 2014 : 10th Patras Workshop on Axions, WIMPs and WISPs, 2014-06-29 - 2014-07-04, Geneva
000315513 300__ $$a102-107
000315513 3367_ $$2ORCID$$aCONFERENCE_PAPER
000315513 3367_ $$033$$2EndNote$$aConference Paper
000315513 3367_ $$2BibTeX$$aINPROCEEDINGS
000315513 3367_ $$2DRIVER$$aconferenceObject
000315513 3367_ $$2DataCite$$aOutput Types/Conference Paper
000315513 3367_ $$0PUB:(DE-HGF)8$$2PUB:(DE-HGF)$$aContribution to a conference proceedings$$bcontrib$$mcontrib$$s1481028793_12010
000315513 3367_ $$0PUB:(DE-HGF)7$$2PUB:(DE-HGF)$$aContribution to a book$$mcontb
000315513 4900_ $$0PERI:(DE-600)2450075-6$$aDESY-PROC
000315513 520__ $$aIt is well-known that electric dipole moment (EDM) constraints provide the most stringent bounds on axion-mediated macroscopic spin-dependent (SD) and time reversal and parity violating (TVPV) forces. These bounds are several orders of magnitude stronger than those arising from direct searches in fifth-force experiments and combining astrophysical bounds on stellar energy loss with E\"otv\"os tests of the weak equivalence principle (WEP). This is a consequence of the specific properties of the axion, invoked to solve the Strong CP problem. However, the situation is quite different for generic light scalars that are unrelated to the strong CP problem. In this case, bounds from fifth-force experiments and astrophysical processes are far more stringent than the EDM bounds, for the mass range explored in direct searches.
000315513 7001_ $$0P:(DE-HGF)0$$aPitschmann, Mario$$b1
000315513 7001_ $$0P:(DE-HGF)0$$aRamsey-Musolf, Michael J.$$b2
000315513 7870_ $$0PUBDB-2016-05897$$aTsesmelis, Emmanuel et. al.$$dVerlag Deutsches Elektronen-Synchrotron$$iisPartOf$$rDESY-PROC-2014-03$$tProceedings, 10th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2014) : Geneva, Switzerland, June 29-July 4, 2014
000315513 8564_ $$uhttps://bib-pubdb1.desy.de/record/315513/files/fulltext.pdf$$yOpenAccess
000315513 909CO $$ooai:bib-pubdb1.desy.de:315513$$pdnbdelivery$$pdriver$$popen_access$$popenaire
000315513 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$a North Georgia Coll. - St. U. $$b0
000315513 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$a  	 TU Vienna$$b1
000315513 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$a Massachusetts U., Amherst$$b2
000315513 9101_ $$0I:(DE-HGF)0$$6P:(DE-HGF)0$$a Caltech$$b2
000315513 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess
000315513 915__ $$0StatID:(DE-HGF)10000$$2StatID$$aHosted Content
000315513 915__ $$0LIC:(DE-HGF)CCBY4$$2HGFVOC$$aCreative Commons Attribution CC BY 4.0
000315513 980__ $$acontrib
000315513 980__ $$acontb
000315513 980__ $$aI:(DE-H253)L-20120731
000315513 9801_ $$aUNRESTRICTED
000315513 9801_ $$aFullTexts