Journal article
On the maximum energy of non-thermal particles in the primary hotspot of Cygnus A
- Abstract:
- We study particle acceleration and magnetic field amplification in the primary hotspot in the northwest jet of radiogalaxy Cygnus A. By using the observed flux density at 43 GHz in a well resolved region of this hotspot, we determine the minimum value of the jet density and constrain the magnitude of the magnetic field. We find that a jet with density greater than $5\times 10^{-5}$ cm$^{-3}$ and hotspot magnetic field in the range 50-400 $\mu$G are required to explain the synchrotron emission at 43 GHz. The upper-energy cut-off in the hotspot synchrotron spectrum is at a frequency < $5\times 10^{14}$ Hz, indicating that the maximum energy of non-thermal electrons accelerated at the jet reverse shock is $E_{e, \rm max} \sim 0.8$ TeV in a magnetic field of 100 $\mu$G. Based on the condition that the magnetic-turbulence scale length has to be larger than the plasma skin depth, and that the energy density in non-thermal particles cannot violate the limit imposed by the jet kinetic luminosity, we show that $E_{e,\rm max}$ cannot be constrained by synchrotron losses as traditionally assumed. In addition to that, and assuming that the shock is quasi-perpendicular, we show that non-resonant hybrid instabilities generated by the streaming of cosmic rays with energy $E_{e, \rm max}$ can grow fast enough to amplify the jet magnetic field up to 50-400 $\mu$G and accelerate particles up to the maximum energy $E_{e, \rm max}$ observed in the Cygnus A primary hotspot.
- Publication status:
- Published
- Peer review status:
- Peer reviewed
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(Preview, Version of record, pdf, 804.2KB, Terms of use)
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- Publisher copy:
- 10.1093/mnras/stx2552
Authors
- Publisher:
- Oxford University Press
- Journal:
- Monthly Notices of the Royal Astronomical Society More from this journal
- Volume:
- 473
- Issue:
- 3
- Pages:
- 3500–3506
- Publication date:
- 2017-10-01
- Acceptance date:
- 2017-09-26
- DOI:
- Keywords:
- Pubs id:
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pubs:734626
- UUID:
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uuid:2c9c3986-0f32-42d4-a6db-4365a4f8503f
- Local pid:
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pubs:734626
- Source identifiers:
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734626
- Deposit date:
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2017-10-09
Terms of use
- Copyright holder:
- Matthews et al
- Copyright date:
- 2017
- Notes:
- © 2017 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society D
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