A possibility of emission of high frequency gravitational radiation from junctions between d-wave and s-wave superconductors

dc.creatorFontana, Giorgio
dc.date1998-12-04
dc.date.accessioned2026-07-07T03:12:17Z
dc.date.available2026-07-07T03:12:17Z
dc.descriptionRecent measurements on a class of high-Tc superconductors (HTSCs) have shown that Cooper-pairs wavefunction is a d-wave, while in another class, d-wave and s-wave may coexist. Conventional low-Tc superconductors are s-wave superconductors. When d-wave Cooper-pairs are injected in a superconductor that can sustain s-wave pairing, d-wave pairs are subject to transition 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 that show a gravitational interaction between inhomogeneous 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.identifierhttps://arxiv.org/abs/cond-mat/9812070
dc.identifierhttp://arxiv.org/abs/cond-mat/9812070
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/28853
dc.subjectSuperconductivity
dc.titleA possibility of emission of high frequency gravitational radiation from junctions between d-wave and s-wave superconductors
dc.typetext

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