Radiation from accelerated particles in relativistic jets with shocks, shear-flow, and reconnection

K.-I. Nishikawa; B. Zhang; I. Dutan; M. Medvedev; P. Hardee; E.J. Choi; K.W. Min; J. Niemiec; Y. Mizuno; Åke Nordlund; Jacob Trier Frederiksen; H. Sol; M. Pohl; D.H. Hartmann

doi:10.1051/eas/1361026

Radiation from accelerated particles in relativistic jets with shocks, shear-flow, and reconnection

K.-I. Nishikawa, B. Zhang, I. Dutan, M. Medvedev, P. Hardee, E.J. Choi, K.W. Min, J. Niemiec, Y. Mizuno, Åke Nordlund, Jacob Trier Frederiksen, H. Sol, M. Pohl, D.H. Hartmann

Astrofysik og Planetforskning

1 Citationer (Scopus)

Abstract

We investigated particle acceleration and shock structure associated with an unmagnetized relativistic jet propagating into an unmagnetized plasma. Strong magnetic fields generated in the trailing shock contribute to the electrons transverse deflection and acceleration. We have calculated, self-consistently, the radiation from electrons accelerated in these turbulent magnetic fields. We found that the synthetic spectra depend on the bulk Lorentz factor of the jet, its temperature and strength of the generated magnetic fields. We have also investigated accelerated electrons in strong magnetic fields generated by kinetic shear (Kelvin-Helmholtz) instabilities. The calculated properties of the emerging radiation will guide our understanding of the complex time evolution and/or spectral structure in gamma-ray bursts, relativistic jets in general, and supernova remnants.

Originalsprog	Engelsk
Tidsskrift	E A S Publications Series
Vol/bind	61
Sider (fra-til)	177-179
ISSN	1633-4760
DOI	https://doi.org/10.1051/eas/1361026
Status	Udgivet - 22 jul. 2013

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10.1051/eas/1361026

Citationsformater

Nishikawa, K.-I., Zhang, B., Dutan, I., Medvedev, M., Hardee, P., Choi, E. J., Min, K. W., Niemiec, J., Mizuno, Y., Nordlund, Å., Frederiksen, J. T., Sol, H., Pohl, M., & Hartmann, D. H. (2013). Radiation from accelerated particles in relativistic jets with shocks, shear-flow, and reconnection. E A S Publications Series, 61, 177-179. https://doi.org/10.1051/eas/1361026

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abstract = "We investigated particle acceleration and shock structure associated with an unmagnetized relativistic jet propagating into an unmagnetized plasma. Strong magnetic fields generated in the trailing shock contribute to the electrons transverse deflection and acceleration. We have calculated, self-consistently, the radiation from electrons accelerated in these turbulent magnetic fields. We found that the synthetic spectra depend on the bulk Lorentz factor of the jet, its temperature and strength of the generated magnetic fields. We have also investigated accelerated electrons in strong magnetic fields generated by kinetic shear (Kelvin-Helmholtz) instabilities. The calculated properties of the emerging radiation will guide our understanding of the complex time evolution and/or spectral structure in gamma-ray bursts, relativistic jets in general, and supernova remnants.",

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T1 - Radiation from accelerated particles in relativistic jets with shocks, shear-flow, and reconnection

AU - Nishikawa, K.-I.

AU - Zhang, B.

AU - Dutan, I.

AU - Medvedev, M.

AU - Hardee, P.

AU - Choi, E.J.

AU - Min, K.W.

AU - Niemiec, J.

AU - Mizuno, Y.

AU - Nordlund, Åke

AU - Frederiksen, Jacob Trier

AU - Sol, H.

AU - Pohl, M.

AU - Hartmann, D.H.

PY - 2013/7/22

Y1 - 2013/7/22

N2 - We investigated particle acceleration and shock structure associated with an unmagnetized relativistic jet propagating into an unmagnetized plasma. Strong magnetic fields generated in the trailing shock contribute to the electrons transverse deflection and acceleration. We have calculated, self-consistently, the radiation from electrons accelerated in these turbulent magnetic fields. We found that the synthetic spectra depend on the bulk Lorentz factor of the jet, its temperature and strength of the generated magnetic fields. We have also investigated accelerated electrons in strong magnetic fields generated by kinetic shear (Kelvin-Helmholtz) instabilities. The calculated properties of the emerging radiation will guide our understanding of the complex time evolution and/or spectral structure in gamma-ray bursts, relativistic jets in general, and supernova remnants.

AB - We investigated particle acceleration and shock structure associated with an unmagnetized relativistic jet propagating into an unmagnetized plasma. Strong magnetic fields generated in the trailing shock contribute to the electrons transverse deflection and acceleration. We have calculated, self-consistently, the radiation from electrons accelerated in these turbulent magnetic fields. We found that the synthetic spectra depend on the bulk Lorentz factor of the jet, its temperature and strength of the generated magnetic fields. We have also investigated accelerated electrons in strong magnetic fields generated by kinetic shear (Kelvin-Helmholtz) instabilities. The calculated properties of the emerging radiation will guide our understanding of the complex time evolution and/or spectral structure in gamma-ray bursts, relativistic jets in general, and supernova remnants.

U2 - 10.1051/eas/1361026

DO - 10.1051/eas/1361026

M3 - Conference article

SN - 1633-4760

VL - 61

SP - 177

EP - 179

JO - E A S Publications Series

JF - E A S Publications Series

ER -

Radiation from accelerated particles in relativistic jets with shocks, shear-flow, and reconnection

Abstract

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