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dc.contributor.authorMukubwa, A.
dc.contributor.authorMasinde, Fred W.
dc.date.accessioned2019-09-10T07:53:47Z
dc.date.available2019-09-10T07:53:47Z
dc.date.issued2019-08-26
dc.identifier.citationOpen Access Library Journal Vol.06 No.08 (2019), Article ID:94605,10 pagesen_US
dc.identifier.issnOnline: 2333-9721
dc.identifier.issnPrint: 2333-9705
dc.identifier.urihttps://www.scirp.org/pdf/OALibJ_2019082316174165.pdf
dc.identifier.urihttp://repository.seku.ac.ke/handle/123456789/4880
dc.descriptionDOI: 10.4236/oalib.1105661en_US
dc.description.abstractA plasma has been defined as a quasi-neutral gas of charged particles showing collective behaviour. Plasmas can support waves depending on the local conditions, the presence of external electric and magnetic fields. A characteristic property of plasmas is their ability to transfer momentum and energy via collective motion. An example in this case, is the Langmuir waves where plasma electrons oscillate against a stationary ion background. In a superconductor, two plasma electrons arise one that is made up of normal electrons and the other that is made up of super-electrons. In this study, we consider a system of super-electrons forming a super-particle. The motion of the plasma super-particles around a magnetic vortex core has been studied in the YBCO123 and Bi2212 systems. The results reveal an assemblage of super-particles that contain the magnetic flux within the vortex core of radius r 0 ≅ 1 3 ( 1.728 E × 10 − 18 ) 1 2 Å .en_US
dc.language.isoenen_US
dc.subjectPlasmaen_US
dc.subjectMagnetic Fluxen_US
dc.subjectMagnetic Vortex Coreen_US
dc.subjectSuper-Particlesen_US
dc.titleDetermining the Radius of the Magnetic Vortex Core of YBCO123 and Bi2212en_US
dc.typeArticleen_US
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