Abstract
RADIO-LOUD active galactic nuclei (AGNs) tend to show extended emission in the form of jets and an unresolved central core, from which the jets presumably originate. The intensity spectrum of the core varies smoothly from 108.5 to 1016 Hz in frequency1, and is flat (constant with frequency) between 109 and 1012 Hz, implying that a single emission mechanism, probably synchrotron radiation, is responsible. Because synchrotron emission below ∼10l3Hz would be self-absorbed for a uniform source under conditions typical of AGNs, inhomogeneous models have been used to account for these spectra. These models, which require the magnetic field strength and the electron density and energy to vary according to strict power laws, reproduce the flat spectra by a number of self-absorbed components2–4, but they do not explain the origin of radiating electrons at ∼1018 cm from the AGN core, in view of the very short lifetime of the electrons in an AGN environment. Here we propose that energy is transported from the central source by relativistic neutrons, which travel freely over a large volume and decay into relativistic protons. The protons produce secondary electrons which generate the observed radiation. The photon spectra thus produced are largely model independent and flat.
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References
Landau, R. et al. Astrophys. J. 308, 78–92 (1986).
Condon, J. J. & Dressel, L. L. Astrophys. Lett. 15, 203–207 (1973).
Marscher, A. P. Astrophys. J. 216, 244–256 (1977).
Band, D. L. & Grindlay, J. E. Astrophys. J. 308, 576–591 (1985).
Kazanas, D. & Ellison, D. C. Nature 319, 380–382 (1986).
Kirk, J. G. & Mastichiadis, A. Astr. Astrophys. 213, 75–79 (1989).
De Kerret, H. et al. Phys. Lett. B63, 477–482 (1976).
Bell, A. R. Mon. Not. R. astr. Soc. 182, 147–156 (1978).
Blandford, R. D. & Ostriker, J. P. Astrophys. J. 221, L29–L32 (1978).
Kazanas, D. & Ellison, D. C. Astrophys. J. 304, 178–187 (1986).
Sikora, M. et al. Astrophys. J. 341, L33–L36 (1989).
Phinney, E. S. in Astrophysics of Active Galaxies and Quasi-Stellar Objects (ed. Miller, I. S.) 453–496 (University Science Books, Mill Valley, 1985).
Kazanas, D. Astrophys. J. 287, 112–115 (1984).
Zdziarski, A. A. & Lamb, D. Q. Astrophys. J. 309, L79–L82 (1985).
Marcher, A. P. Astrophys. J. 334, 552–559 (1988).
Krautter, A., Henriksen, R. N. & Lake, K. Astrophys. J. 269, 81–93 (1983).
Backer, D. C. in Superluminal Radio Sources (eds Zensus, J. A. & Pearson, T. J.) 76–82 (Cambridge University, 1987).
Sikora, M. et al. Astrophys. J. 320, L81–L85 (1987).
Königl, A. Astrophys. J. 243, 700–709 (1981).
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Giovanoni, P., Kazanas, D. Flat-spectrum radio sources: cosmic conspiracy or relativistic neutrons?. Nature 345, 319–322 (1990). https://doi.org/10.1038/345319a0
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DOI: https://doi.org/10.1038/345319a0
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