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.
2008
978-0-7354-0502-8
40 YEARS OF PULSARS: Millisecond Pulsars, Magnetars and More
216
218
D. Volpi; L. Del Zanna; E. Amato; N. Bucciantini
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Utilizza questo identificatore per citare o creare un link a questa risorsa: https://hdl.handle.net/2158/593934
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