Radiation from relativistic shocks with turbulent magnetic fields

TY - GEN

T1 - Radiation from relativistic shocks with turbulent magnetic fields

AU - Nishikawa, K.

AU - Niemiec, J.

AU - Medvedev, M.

AU - Zhang, B.

AU - Hardee, P.

AU - Nordlund, A.

AU - Frederiksen, Jacob Trier

AU - Mizuno, Y.

AU - Sol, H.

AU - Pohl, M.

AU - Hartmann, D. H.

AU - Oka, M.

AU - Fishman, G. J.

PY - 2010/6

Y1 - 2010/6

N2 - Using our new 3D relativistic electromagnetic particle (REMP) code parallelized with MPI, we investigated long-term particle acceleration associated with a relativistic electronpositron jet propagating in an unmagnetized ambient electronpositron plasma. We have also performed simulations with electron-ion jets. The simulations were performed using a much longer simulation system than our previous simulations in order to investigate the full nonlinear stage of the Weibel instability for electronpositron jets and its particle acceleration mechanism. Cold jet electrons are thermalized and ambient electrons are accelerated in the resulting shocks for pair plasma case. Acceleration of ambient electrons leads to a maximum ambient electron density three times larger than the original value for pair plasmas. Behind the bow shock in the jet shock strong electromagnetic fields are generated. These fields may lead to time-dependent afterglow emission. We calculated radiation from electrons propagating in a uniform parallel magnetic field to verify the technique. We also used the new technique to calculate emission from electrons based on simulations with a small system with two different cases for Lorentz factors (15 and 100). We obtained spectra which are consistent with those generated from electrons propagating in turbulent magnetic fields with red noise. This turbulent magnetic field is similar to the magnetic field generated at an early nonlinear stage of the Weibel instability.

AB - Using our new 3D relativistic electromagnetic particle (REMP) code parallelized with MPI, we investigated long-term particle acceleration associated with a relativistic electronpositron jet propagating in an unmagnetized ambient electronpositron plasma. We have also performed simulations with electron-ion jets. The simulations were performed using a much longer simulation system than our previous simulations in order to investigate the full nonlinear stage of the Weibel instability for electronpositron jets and its particle acceleration mechanism. Cold jet electrons are thermalized and ambient electrons are accelerated in the resulting shocks for pair plasma case. Acceleration of ambient electrons leads to a maximum ambient electron density three times larger than the original value for pair plasmas. Behind the bow shock in the jet shock strong electromagnetic fields are generated. These fields may lead to time-dependent afterglow emission. We calculated radiation from electrons propagating in a uniform parallel magnetic field to verify the technique. We also used the new technique to calculate emission from electrons based on simulations with a small system with two different cases for Lorentz factors (15 and 100). We obtained spectra which are consistent with those generated from electrons propagating in turbulent magnetic fields with red noise. This turbulent magnetic field is similar to the magnetic field generated at an early nonlinear stage of the Weibel instability.

U2 - 10.1142/S0218271810016865

DO - 10.1142/S0218271810016865

M3 - Conference article

SN - 0218-2718

VL - 19

SP - 715

EP - 721

JO - International Journal of Modern Physics D

JF - International Journal of Modern Physics D

IS - 6

ER -