TY - JOUR
T1 - Coherent plasma-curvature radiation in FRB
AU - Katz, J. I.
N1 - Publisher Copyright:
© 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society.
PY - 2018/12/11
Y1 - 2018/12/11
N2 - Curvature radiation is a natural candidate for the emission mechanism of Fast Radio Burs (FRB). However, FRB spectra have structure with Δυ/upsi; ~0.03-0.2, inconsistent with the very smooth spectrum of curvature radiation. Although this spectral structure might be attributed to chromatic scintillation or lensing, in four FRB high spectral resolution data indicate scintillation decorrelation bandwidths much narrower than the observed ~30-300 MHz spectral structure. Some of the observed structures may be intrinsic to the radiation mechanism. I suggest that the observed spectral structure reflects the spatial structure of a clumpy radiating charge distribution, and that the characteristic curvature radiation frequency may be higher than the observed frequencies. In this coupled plasma-curvature radiation process the radiated spectra are the product of the spectra of the plasma wave and that of incoherent curvature radiation. The argument applies to all coherent radiation processes, including those that produce pulsar nanoshots. The implied FRB 'clump' charges are large, and produce electrostatic potentials that suggest electron Lorentz factors ≳102. The result applies generally to coherently radiating sources.
AB - Curvature radiation is a natural candidate for the emission mechanism of Fast Radio Burs (FRB). However, FRB spectra have structure with Δυ/upsi; ~0.03-0.2, inconsistent with the very smooth spectrum of curvature radiation. Although this spectral structure might be attributed to chromatic scintillation or lensing, in four FRB high spectral resolution data indicate scintillation decorrelation bandwidths much narrower than the observed ~30-300 MHz spectral structure. Some of the observed structures may be intrinsic to the radiation mechanism. I suggest that the observed spectral structure reflects the spatial structure of a clumpy radiating charge distribution, and that the characteristic curvature radiation frequency may be higher than the observed frequencies. In this coupled plasma-curvature radiation process the radiated spectra are the product of the spectra of the plasma wave and that of incoherent curvature radiation. The argument applies to all coherent radiation processes, including those that produce pulsar nanoshots. The implied FRB 'clump' charges are large, and produce electrostatic potentials that suggest electron Lorentz factors ≳102. The result applies generally to coherently radiating sources.
KW - Radiation mechanisms: non-thermal
KW - Radio continuum: galaxies
UR - https://www.scopus.com/pages/publications/85054215861
U2 - 10.1093/mnras/sty2459
DO - 10.1093/mnras/sty2459
M3 - Article
AN - SCOPUS:85054215861
SN - 0035-8711
VL - 481
SP - 2946
EP - 2950
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
IS - 3
ER -