Hydromagnetic Plasma Acceleration by Rapidly Rotating Astrophysical Objects

Details Hydromagnetic Plasma Acceleration by Rapidly Rotating Astrophysical Objects Hydromagnetic Plasma Acceleration by Rapidly Rotating Astrophysical Objects

Aug 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969phrvl..23..247m&link_type=abstract

Physical Review Letters, vol. 23, Issue 5, pp. 247-249

Physics

21

Scientific paper

We have solved analytically for the acceleration of plasma away from a rotating magnetized object. Application of that analysis to rotator models for the radio, optical, and x-ray pulsar NP0532 suggests that it has a magnetic moment of order 3×1028 G cm3 and is losing mass at a rate order 2×109 g/sec. These parameters would provide particles in excess of 1011 eV and a 6×10-4-G field in the Crab Nebula at 1 lt yr from NPO532.

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