Conclusions
Our study shows the universality of the power-law spectrum with γ=3 in PTR in the presence of a magnetic field. This result is important to astrophysical applications because there is no doubt that magnetic fields are present in many different types of cosmic objects. This universality can be compared with the known statistical analysis of the spectra of various cosmic radio sources (Fig. 5); the most probable value is close to γ=3. The spread in the observed values of γ could be due to the escape of particles, nonuniformity, and so on, and requires further study.
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Literature Cited
V. N. Tsytovich and A. S. Chikhachev, Astron. Zh.,48, 486 (1969).
Yu. A. Nikolaev, V. N. Tsytovich, and A. S. Chikhachev, Zh. Éksp. Teor. Fiz.,64, 877 (1973).
S. A. Kaplan and V. N. Tsytovich, Plasma Astrophysics [in Russian], Nauka, Moscow (1972).
S. A. Kaplan and V. N. Tsytovich, Astron. Zh.,49, 647 (1972).
C. A. Norman, and D. ter Haar, Astron. Astrophys.,24, 121 (1973).
S. A. Kaplan, F. K. Lamb, D. Pines, K. J. Petic, and V. N. Tsytovich, Astron. Zh. (in press).
Yu. P. Ochelkov and O. F. Prilytskii, Astron. Zh. (in press).
K. J. Petic (C. I. Pethick) and V. N. Tsytovich, Astrophys. Space Sci. (in press).
C. A. Norman, Preprint Oxford Department of Theoretical Physics (1974).
C. A. Norman, Dissertation, Oxford Department of Philosophy (1973).
S. A. Kaplan and V. N. Tsytovich, Astron. Zh.49, 890 (1972).
V. N. Tsytovich, Theory of Turbulent Plasma [in Russian], Atomizdat, Moscow (1971).
M. A. Livshits and V. N. Tsytovich, Zh. Éksp. Teor. Fiz.,62, 606 (1972).
Additional information
Moscow Institute of Engineering Physics. Translated from Astrofizika, Vol. 12, No. 1, pp. 107–120, January–March, 1976.
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Nikolaev, Y.A., Tsytovich, V.N. & Chikhachev, A.S. Effect of a magnetic field on the spectrum of relativistic electrons in a plasma turbulent reactor. Astrophysics 12, 68–76 (1976). https://doi.org/10.1007/BF01006591
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DOI: https://doi.org/10.1007/BF01006591