Matter in Superstrong Magnetic Fields: The Surface of a Neutron Star

Details Matter in Superstrong Magnetic Fields: The Surface of a Neutron Star Matter in Superstrong Magnetic Fields: The Surface of a Neutron Star

Nov 1971

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971phrvl..27.1306r&link_type=abstract

Physical Review Letters, vol. 27, Issue 19, pp. 1306-1308

Physics

135

Scientific paper

In huge magnetic fields (B>~1012 G) matter forms a tightly bound, dense (>~104 g cm-3) solid with properties of a one-dimensional metal and a work function of the order of a keV. Electron field emission from the sharp surface of a pulsar is much easier than ion emission; it is estimated to be cut off when the stellar rotation period exceeds several seconds.

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