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Transport Processes and Neutrino Emission Processes in the Interior of White Dwarfs

Published online by Cambridge University Press:  12 April 2016

Naoki Itoh
Naoki Itoh*
Affiliation:
Department of Physics, Sophia University7-1, Kioi-cho, Chiyoda-ku, Tokyo 102Japan

Abstract

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Recent developments in the studies of the transport processes and the neutrino emission processes in the interior of white dwarfs are reviewed. Special emphasis is placed upon the accuracy of the calculations. Ionic correlation effects play an essential role in the transport processes and the neutrino bremsstrahlung process. The Weinberg-Salam theory is the basis for the calculation of the neutrino emission processes.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 114: White Dwarfs , 1989 , pp. 66 - 80
Copyright
Copyright © Springer-Verlag 1989

References

Beaudet, G., Petrosian, V., and Salpeter, E.E. 1967, AP. J., 150, 979.CrossRefGoogle Scholar
Coldwell-Horsfall, R.A., and Maradudin, A.A. 1960, J. Math. Phys., 1, 395.CrossRefGoogle Scholar
Flowers, E., and Itoh, N. 1976, AP. J., 206, 218 Google Scholar
Flowers, E., and lton, N. 1979, Ap. J., 230, 847.CrossRefGoogle Scholar
Flowers, E., and Itoh, N. 1981, Ap. J., 250, 750.CrossRefGoogle Scholar
Ichimaru, S. 1982, Rev.Mod.Phys., 54, 1017.Google Scholar
Itoh, N., Adachi, T., Nakagawa, M., Kohyama, Y., and Munakata, H. 1988, submitted to Ap.J.Google Scholar
Itoh, N., and Kohyama, Y. 1983, Ap.J., 275, 858.Google Scholar
Itoh, N., Kohyama, Y., Matsumoto, N., and Seki, M. 1984a, Ap.J., 280, 787.CrossRefGoogle Scholar
Itoh, N., Kohyama, Y., Matsumoto, N., and Seki, M. 1984b, Ap. J., 285, 304; 322, 584(1987).Google Scholar
Itoh, N., Kohyama, Y., Matsumoto, N., and Seki, M. 1984c, Ap.J., 285, 758.Google Scholar
Itoh, N., Kohyama, Y., and Takeuchi, H. 1987, Ap.J., 317, 733.CrossRefGoogle Scholar
Itoh, N., Matsumoto, N., Seki, M., and Kohyama, Y. 1984d, Ap. J., 279, 413.Google Scholar
Itoh, N., Mitake, S., Iyetomi, H., and Ichimaru, S. 1983, Ap.J., 273, 774.Google Scholar
Iyetomi, H., and Ichimaru, S. 1982, Phys.Rev., A25, 2434.CrossRefGoogle Scholar
Jancovici, B. 1962, Nuovo Cimento, 25, 428.Google Scholar
Kohyama, Y., Itoh, N., and Munakata, H. 1986, Ap.J., 310, 815.CrossRefGoogle Scholar
Mitake, S., Ichimaru, S., and Itoh, N. 1984, Ap.J., 277, 375.Google Scholar
Munakata, H., Kohyama, Y., and Itoh, N. 1985, Ap.J., 296, 197; 304, 580 (1986).Google Scholar
Munakata, H., Kohyama, Y., and Itoh, N. 1987, Ap.J., 316, 708.Google Scholar
Nandkumar, R., and Pethick, C.J. 1984, M.N.R.A.S., 209, 511.Google Scholar
Pollock, E.L., and Hansen, J.P. 1973, Phys.Rev., A8, 3110.Google Scholar
Raikh, M.E., and Yakovlev, D.G. 1982, Ap.Space Sci., 87, 193.Google Scholar
Schinder, P.J., Schramm, D.N., Wiita, P.J., Margolis, S.H., and Tubbs, D.L. 1987, Ap.J., 313, 531.Google Scholar
Slattery, W.L., Dooien, G.D., and Dewitt, H.E. 1982, Phys.Rev., A26, 2255.Google Scholar
Yakovlev, D.G., and Urpin, V.A. 1980, Soviet Astr., 24, 303.Google Scholar
Ziman, J. 1961, Phil. Mag., 6, 1013.Google Scholar