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Charged Scalars in Transient Stellar Electromagnetic Fields |
| Marina-Aura Dariescu**, Ciprian Dariescu, Ovidiu Buhucianu
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Faculty of Physics, Al. I. Cuza" University, Bd. Carol I, No. 11, 700506 Iaşi, Romania
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Marina-Aura Dariescu, Ciprian Dariescu, Ovidiu Buhucianu 2011 Chin. Phys. Lett. 28 010303 |
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Abstract We consider a non-rotating strongly magnetized object, whose magnetic induction is of the form Bx = B0(t) sinκz. 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 currents.
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| Keywords:
03.65.Pm
97.10.Ld
97.60.Jd
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Received: 20 September 2010
Published: 23 December 2010
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| PACS: |
03.65.Pm
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(Relativistic wave equations)
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97.10.Ld
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(Magnetic and electric fields; polarization of starlight)
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97.60.Jd
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(Neutron stars)
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