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Charged Radial Infall for Spherical Central Bodies

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arxiv 1101.1471 v1 pith:DUM4OMLG submitted 2011-01-07 physics.class-ph gr-qc

Charged Radial Infall for Spherical Central Bodies

classification physics.class-ph gr-qc
keywords relativisticgeneralcentralspecialbodieschargedclassicalmechanics
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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A massive, charged, spherical central body can be neutralized by attracting particles of opposite charge. We calculate the time it takes to neutralize these central bodies using classical mechanics, special relativistic mechanics, and finally, the "forced" trajectories of general relativity. While we can compare the classical and (special) relativistic times, and find, predictably, that the special relativistic neutralization time is longer, a comparison of these times with the general relativistic result is not as directly possible. We offer the final calculation as a demonstration of dynamics in a general setting and in particular, the structural similarity of the (general) relativistic problem to the other cases.

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