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Published in 2019 at "Physical Review D"
DOI: 10.1103/physrevd.99.083004
Abstract: The energy loss of a rotationally powered pulsar is primarily carried away as electromagnetic radiation and a particle wind. Considering that the magnetic field strength of pulsars ranges from about 108 to 1015 G, one could…
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Keywords:
neutron star;
qed effects;
star spin;
spin ... See more keywords