Publication Date:
2016-09-30
Description:
Author(s): O. Hamil, N. J. Stone, and J. R. Stone The magnetic dipole radiation model is currently the best approach we have to explain pulsar radiation. However, a most characteristic parameter of the observed radiation, the braking index n obs , shows deviations for all the eight best studied isolated pulsars, from the simple model prediction n dip = … [Phys. Rev. D 94, 063012] Published Thu Sep 29, 2016
Keywords:
Astrophysics and astroparticle physics
Print ISSN:
0556-2821
Electronic ISSN:
1089-4918
Topics:
Physics
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