SEARCH FOR NEARLY MASSLESS, WEAKLY COUPLED PARTICLES BY OPTICAL TECHNIQUES

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dc.contributor.authorCAMERON, Rko
dc.contributor.authorCANTATORE, Gko
dc.contributor.authorMELISSINOS, ACko
dc.contributor.authorRUOSO, Gko
dc.contributor.authorSemertzidis, Yannis K.ko
dc.contributor.authorHALAMA, HJko
dc.contributor.authorLAZARUS, DMko
dc.contributor.authorPRODELL, AGko
dc.contributor.authorNEZRICK, Fko
dc.contributor.authorRIZZO, Cko
dc.contributor.authorZAVATTINI, Eko
dc.date.accessioned2019-04-15T16:50:41Z-
dc.date.available2019-04-15T16:50:41Z-
dc.date.created2013-12-03-
dc.date.issued1993-05-
dc.identifier.citationPHYSICAL REVIEW D, v.47, no.9, pp.3707 - 3725-
dc.identifier.issn0556-2821-
dc.identifier.urihttp://hdl.handle.net/10203/256172-
dc.description.abstractWe have searched for light scalar and/or pseudoscalar particles that couple to two photons by studying the propagation of a laser beam (lambda=514 nm) through a transverse magnetic field. A limit of 3.5 X 10(-10) rad was set on a possible optical rotation of the beam polarization for an effective path length of 2.2 km in a 3.25 T magnetic field. We find that the coupling g(alphagammagamma) < 3.6 X 10(-7) GeV-1 at the 95% confidence level, provided m(a) < 10(-3) eV. Similar limits can be set from the absence of ellipticity in the transmitted beam. We also searched for photon regeneration in a magnetic field and found the limit g(alphagammagamma) < 6.7 X 10(-7) GeV-1 for the same range of particle mass.-
dc.languageEnglish-
dc.publisherAMERICAN PHYSICAL SOC-
dc.subjectANOMALOUS MAGNETIC-MOMENT-
dc.subjectAXION PRODUCTION-
dc.subjectCOSMIC AXIONS-
dc.subjectLIGHT PSEUDOSCALARS-
dc.subjectCP CONSERVATION-
dc.subjectSINGLE PHOTONS-
dc.subjectNEUTRINO BURST-
dc.subjectGAMMA-DECAY-
dc.subjectUPPER LIMIT-
dc.subjectCONSTRAINTS-
dc.titleSEARCH FOR NEARLY MASSLESS, WEAKLY COUPLED PARTICLES BY OPTICAL TECHNIQUES-
dc.typeArticle-
dc.identifier.wosidA1993LA92800009-
dc.type.rimsART-
dc.citation.volume47-
dc.citation.issue9-
dc.citation.beginningpage3707-
dc.citation.endingpage3725-
dc.citation.publicationnamePHYSICAL REVIEW D-
dc.identifier.doi10.1103/PhysRevD.47.3707-
dc.contributor.localauthorSemertzidis, Yannis K.-
dc.contributor.nonIdAuthorCAMERON, R-
dc.contributor.nonIdAuthorCANTATORE, G-
dc.contributor.nonIdAuthorMELISSINOS, AC-
dc.contributor.nonIdAuthorRUOSO, G-
dc.contributor.nonIdAuthorHALAMA, HJ-
dc.contributor.nonIdAuthorLAZARUS, DM-
dc.contributor.nonIdAuthorPRODELL, AG-
dc.contributor.nonIdAuthorNEZRICK, F-
dc.contributor.nonIdAuthorRIZZO, C-
dc.contributor.nonIdAuthorZAVATTINI, E-
dc.type.journalArticleArticle-
dc.subject.keywordPlusANOMALOUS MAGNETIC-MOMENT-
dc.subject.keywordPlusAXION PRODUCTION-
dc.subject.keywordPlusCOSMIC AXIONS-
dc.subject.keywordPlusLIGHT PSEUDOSCALARS-
dc.subject.keywordPlusCP CONSERVATION-
dc.subject.keywordPlusSINGLE PHOTONS-
dc.subject.keywordPlusNEUTRINO BURST-
dc.subject.keywordPlusGAMMA-DECAY-
dc.subject.keywordPlusUPPER LIMIT-
dc.subject.keywordPlusCONSTRAINTS-
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