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.
Simulated synchrotron and Inverse Compton emission from Pulsar Wind Nebulae / D. Volpi; L. Del Zanna; E. Amato; N. Bucciantini. - STAMPA. - (2008), pp. 216-218. [10.1063/1.2900146]
Simulated synchrotron and Inverse Compton emission from Pulsar Wind Nebulae
DEL ZANNA, LUCA;E. Amato;
2008
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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