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Charged Scalars in Transient Stellar Electromagnetic Fields
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作者 marina-aura dariescu ciprian dariescu ovidiu buhucianu 《Chinese Physics Letters》 SCIE CAS CSCD 2011年第1期20-23,共4页
We consider a non-rotating strongly magnetized object, whose magnetic induction is of the form Bx= Bo (t) sin kz. In the electromagnetic field generated by only one component of the four-vector potential, we solve t... We consider a non-rotating strongly magnetized object, whose magnetic induction is of the form Bx= Bo (t) sin kz. In the electromagnetic field generated by only one component of the four-vector potential, we solve the Klein- Gordon equation and discuss the sudden growth of the scalar wave functions for wavenumbers inside computable ranges. In the case of unexcited transversal kinetic degrees, we write down the recurrent differential system for the amplitude functions and compute the respective conserved eurrents. 展开更多
关键词 Astrophysics and astroparticles
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