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arXiv · 0710.0844

Simulated synchrotron and Inverse Compton emission from Pulsar Wind Nebulae

Delia Volpi·Luca Del Zanna·Elena Amato·Niccolo Bucciantini
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Abstract

We present a complete set of diagnostic tools aimed at reproducing synthetic non-thermal (synchrotron and/or Inverse Compton, IC) emissivity, integrated flux energy, polarization and spectral index simulated maps in comparison to observations. The time dependent relativistic magnetohydrodynamic (RMHD) equations are solved with a shock capturing code together with the evolution of the maximum particles energy. Applications to Pulsar Wind Nebulae (PWNe) are shown.

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Delia Volpi, Luca Del Zanna, Elena Amato, Niccolo Bucciantini. 2007-10-03. Simulated synchrotron and Inverse Compton emission from Pulsar Wind Nebulae. https://doi.org/10.1063/1.2900146

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