Modeling Accretion onto a Closed Pulsar Magnetosphere

Details Modeling Accretion onto a Closed Pulsar Magnetosphere Modeling Accretion onto a Closed Pulsar Magnetosphere

Dec 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aas...187.3306m&link_type=abstract

American Astronomical Society, 187th AAS Meeting, #33.06; Bulletin of the American Astronomical Society, Vol. 27, p.1330

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A method for modeling accretion onto a closed magnetosphere employing the numerical method of SPH is presented. This method allows the dynamic interaction of the magnetosphere and surrounding field-free plasma to be simulated. Results obtained for some steady configurations are compared with previous work for closed magnetospheres. Future application of the technique, with a view to modeling spin up and spin down of pulsars is discussed. Other possible applications and enhancements of the method are outlined.

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