Abstract
In this paper we generalize the Adams, Ruderman, Woo and Zaidi plasmon decay process to include the presence of a strong magnetic field. Two cases are studied; propagation parallel and perpendicular to the magnetic field. In either case we found that relevant changes only show forH≌1012–1013G.
This is a preview of subscription content, log in via an institution to check access.
Similar content being viewed by others
References
Adams, J. B., Ruderman, M. A., and Woo, C. H. 1963,Phys. Rev. 129, 1383.
Allis, W. P., Buchsbaum, S. J., and Bers, A.: 1963,Waves in Anisotropic Plasmas, MIT Press, Cambridge, Mass.
Astrom, E. O.: 1950,Arkiv Fys. 2, 443.
Burt, P. and Wahlquist, H.: 1962,Phys. Rev. 125, 1785.
Canuto, V. and Chiu, H.-Y.: 1969,Phys. Rev. 173, 1210, 1220, 1229.
Fassio-Canuto, L.: 1969,Phys. Rev. 187, 2141.
Kelly, D. C.: 1964,Phys. Rev. 134, A641.
Lenard, A.: 1953,Phys. Rev. 90, 968.
Melrose, D. B.: 1968,Astrophys. Space Sci. 2, 171.
Stix, T.H.: 1962,The Theory of Plasma Waves, 1962, McGraw-Hill, New York.
Tsytovich, V. N.: 1961,Soviet Phys. — JETP,13, 1249.
Zaidi, N. H.: 1965,Nuovo Cim. 40, 502.
Author information
Authors and Affiliations
Additional information
On leave of absence from the University of Florence, Italy.
Rights and permissions
About this article
Cite this article
Canuto, V., Chiuderi, C. & Chou, C.K. Plasmon neutrinos emission in a strong magnetic field. Astrophys Space Sci 7, 407–415 (1970). https://doi.org/10.1007/BF00653279
Revised:
Issue Date:
DOI: https://doi.org/10.1007/BF00653279