Mustafa, OmarGuvendi, Abdullah2026-03-262026-03-2620250550-32131873-156210.1016/j.nuclphysb.2025.1168922-s2.0-105001430595https://doi.org/10.1016/j.nuclphysb.2025.116892https://hdl.handle.net/20.500.14901/2437Mustafa, Omar/0000-0001-6664-3859;We study the Klein-Gordon (KG) oscillators in a spinning cosmic string spacetime and an external magnetic field. The corresponding KG-equation is shown to admit a solution in the form of the confluent hypergeometric functions/polynomials. Consequently, the corresponding energies are shown to be given in a quadratic equation of delicate nature that has to be solved in an orderly manner (for it involves the energies for KG-particles/antiparticles, E=E-+/-=(+/-)|E| along with the magnetic quantum number E=E-+/-=(+/-)|m|). Following a case-by-case strategy allowed us to clearly observe the effects of the spinning cosmic string on the spectroscopic structure of the KG-oscillators. Interestingly, we have observed that the coexistence of a spinning cosmic string and an external magnetic field eliminates the effect of the wedge parameter for KG-particles (E=E+), with m=m(+), but not for the KG-antiparticles (E=E-), with m=m(-).Such coexistence is observed to break the symmetry of the energies of the KG-particles and the antiparticles about E=0 for the KG-oscillators. However, for KG-particles (E=E+), with m=m(-), and KG-antiparticles (E=E-), with m=m(+), they are found to be unfortunate because they are indeterminable. Moreover, for the spinning parameter beta>>1, the clustering of the energy levels is observed eminent to indicate that there is no distinction between energy levels at such values of beta.eninfo:eu-repo/semantics/openAccessKlein-Gordon OscillatorsSpinning Cosmic String SpacetimeExternal Magnetic FieldLandau LevelsArticle