GAMMA-RAY EMISSION IN DISSIPATIVE PULSAR MAGNETOSPHERES: FROM THEORY TO FERMI OBSERVATIONS

We compute the patterns of gamma -ray emission due to curvature radiation in dissipative pulsar magnetospheres. Our ultimate goal is to construct macrophysical models that are able to reproduce the observed gamma -ray light curve phenomenology recently published in the Second Fermi Pulsar Catalog. W...

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Veröffentlicht in:	The Astrophysical journal 2014-10, Vol.793 (2), p.1-25
Hauptverfasser:	KALAPOTHARAKOS, CONSTANTINOS, Harding, Alice K, KAZANAS, DEMOSTHENES
Format:	Artikel
Sprache:	eng
Schlagworte:	ASTROPHYSICS, COSMOLOGY AND ASTRONOMY COMPARATIVE EVALUATIONS COMPUTERIZED SIMULATION Cylinders Dissipation ELECTRIC FIELDS EMISSION GAMMA RADIATION GEV RANGE Light curve Lorentz factor MAGNETIC FIELDS Mathematical analysis Mathematical models NEUTRONS PHOTONS Pulsar magnetospheres PULSARS STARS STELLAR MAGNETOSPHERES TRAJECTORIES VISIBLE RADIATION
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