Please use this identifier to cite or link to this item: http://ir-library.mmust.ac.ke:8080/xmlui/handle/123456789/1981
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dc.contributor.authorMunasia, E-
dc.contributor.authorRapando, Wakhu-
dc.contributor.authoro Ndinya, Boniface Otien-
dc.date.accessioned2021-12-31T09:19:22Z-
dc.date.available2021-12-31T09:19:22Z-
dc.date.issued2020-11-
dc.identifier.urihttps://www.researchgate.net/publication/347890615_ANGULAR_DEPENDENCE_OF_D-WAVE_SUPERCONDUCTIVITY_IN_IRRADIATED_CUPRATES-
dc.identifier.urihttp://ir-library.mmust.ac.ke:8080/xmlui/handle/123456789/1981-
dc.description.abstractWe subject the minimized d-wave energy provided for by electromagnetic (e.m) radiation to the thermal activation factor and proceed to obtain transition temperature dependence on zenith and azimuthal angle of the d-electrons in superconducting cuprates. A linear relation of Tc and zenith angle ∅ is revealed. For ∅ = 1.68 , Tc=300K is achieved, providing a promising possibility of room temperature superconductivity. A non-linear increase in T c is observed when the azimuthal angle is reduced to 0.4 radians. Between 0 − 0.4 radians, the highest T c achievable in YBCO and HgBa2Ca2Cu3O8 is 160 K. The angular part of a wave function of an electron system is responsible for orbital orientation. Hence orbital orientation of the d-electron, to a great extend, influences Tc of high temperature superconducting cuprates.en_US
dc.language.isoenen_US
dc.publisherIJRARen_US
dc.subjectANGULAR, DEPENDENCE, D-WAVE, SUPERCONDUCTIVITY , IRRADIATED, CUPRATESen_US
dc.titleANGULAR DEPENDENCE OF D-WAVE SUPERCONDUCTIVITY IN IRRADIATED CUPRATESen_US
dc.typeArticleen_US
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