Dynamo Action on Relativistic Spherical Stars

Details Dynamo Action on Relativistic Spherical Stars Dynamo Action on Relativistic Spherical Stars

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008mgm..conf.2095m&link_type=abstract

"THE ELEVENTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation an

Computer Science

Scientific paper

Within the framework of relativistic gravity, an axisymmetric magnetic field B cannot maintained by dynamo action if:
l)The fluid flow is axially symmetric and divergence free.
2)The background geometry corresponds to a static spherical star of constant density with compactness ratio \varepsilon = {{2GM} / {c2 R}}}, in the range \varepsilon ∈ [0,{{8 / 9}}].

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