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QED and X-Ray Pulsars

Published online by Cambridge University Press:  25 April 2016

Michelle C. Allen ,
D. B. Melrose  and
A. J. Parle
Michelle C. Allen
Affiliation:
Dept of Theoretical Physics, University of Sydney
D. B. Melrose
Affiliation:
Dept of Theoretical Physics, University of Sydney
A. J. Parle
Affiliation:
Dept of Theoretical Physics, University of Sydney
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Abstract

Techniques in QED (quantum electrodynamics) have been developed previously (see for example Melrose and Parle 1983) allowing one to treat electron-photon and photon-photon interactions exactly in the magnetized vacuum and allowing one to include the effects of a medium. These techniques are extended to include particle-particle interactions. Exact cross-sections for electron-electron collisions are derived and compared with known expressions. Such calculations have application in studies of the formation and transfer of radiation in the atmospheres surrounding neutron stars.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 6 , Issue 2 , 1985 , pp. 211 - 214
Copyright
Copyright © Astronomical Society of Australia 1985

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References

Allen, Michelle C., 1985, in preparation.Google Scholar
Aime, M. L., and Wilson, J. R., 1973, Astrophys. J., 186, 1015.Google Scholar
Berestetskii, V. B., Lifshitz, E. M., and Pitaevskii, L. P., ‘Relativistic Quantum Theory’. Pergamon Press. (1971)Google Scholar
Bjorken, J. D., and Drell, S. D., ‘Relativistic Quantum Mechanics’. McGraw-Hill Book Company. (1964).Google Scholar
Johnson, M. H., and Lippmann, B. A., 1949, Phys. Rev., 76, 828.CrossRefGoogle Scholar
Kirk, J. G., and Galloway, D. J., 1982, Plasma Physics, 24, 339.Google Scholar
Langer, Steven H., 1981, Phys. Rev. D., 23, 328.Google Scholar
Langer, Steven H., and Rappaport, , Saul, , 1982, Astrophys. J., 257, 733.CrossRefGoogle Scholar
Lewin, , Walter, H. G., and Heuvel, Van den, Edward, P. J., (eds.) ‘Stellar Driven Accretion X-Ray Sources’. Cambridge University Press. (1983).Google Scholar
Melrose, D. B., (MII), 1983, Aust. J. Phys., 36, 775.Google Scholar
Melrose, D. B., and Parle, A. J., (MPI), 1983, Aust. J. Phys., 36, 755.CrossRefGoogle Scholar
Melrose, D. B., and Parle, A. J., (MPIII), 1983, Aust. J. Phys., 36, 799.CrossRefGoogle Scholar
Meszaros, P., 1984, Space Sci. Rev., 38, 325.Google Scholar
Sokolov, A. A., and Ternov, I. M., ‘Synchrotron Radiation’. Pergamon. Oxford. (1968).Google Scholar
Wang, Y.-M., and Frank, J., 1981, Astron. Astrophys., 93, 255.Google Scholar