Charged Scalars in Transient Stellar Electromagnetic Fields

Details Charged Scalars in Transient Stellar Electromagnetic Fields Charged Scalars in Transient Stellar Electromagnetic Fields

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011chphl..28a0303d&link_type=abstract

Chinese Physics Letters, Volume 28, Issue 1, pp. 010303 (2011).

Physics

2

Scientific paper

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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