A possibility of emission of high frequency gravitational radiation from d-wave to s-wave type superconductor junctions

dc.creatorFontana, Giorgio
dc.date1998-04-26
dc.date.accessioned2026-07-07T03:32:21Z
dc.date.available2026-07-07T03:32:21Z
dc.descriptionRecent measurements on a class of high-Tc superconductors (HTSC) have shown that Cooper-pairs binding may be associated to a d-wave, while in another class, d and s waves may coexist. When d-wave Cooper-pairs are injected in a superconductor that can sustain s-wave binding, d-wave pairs decay to s-wave pairs and energy is irradiated by means of gravitons. We show that in s-wave to d-wave type superconductor (SDS) junctions in an equilibrium condition no net gravitational wave energy is emitted, on the other hand under non equilibrium conditions a net gravitational wave energy is emitted by the junction. Experiments which show a gravitational interaction between inomogeneus high-Tc superconductors, under non equilibrium conditions, and test objects may be understood by accepting a possibility of emission of gravitational radiation from SDS junctions.
dc.description4 pages
dc.identifierhttps://arxiv.org/abs/gr-qc/9804069
dc.identifierhttp://arxiv.org/abs/gr-qc/9804069
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36202
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleA possibility of emission of high frequency gravitational radiation from d-wave to s-wave type superconductor junctions
dc.typetext

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