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Neutron Star Cooling: Criticical Test of Dense Matter Physics

Published online by Cambridge University Press:  04 August 2017

Naoki Itoh*
Affiliation:
Department of Physics, Sophia University, 7-1, Kioi-cho, Chiyoda-ku, Tokyo 102, Japan

Abstract

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Recent developments in the standard theory of neutron star cooling is critically reviewed. Emphasis is placed on the recent developments in the calculations of thermal conductivity and neutrino energy loss rates.

Type
V. Neutron Star Physics
Copyright
Copyright © Reidel 1987 

References

Beaudet, G., Petrosian, V., and Salpeter, E.E. 1967, Astrophys. J., 150, p.979.Google Scholar
Dicus, D.A. 1972, Phys. Rev., D6, p.941.Google Scholar
Dicus, D.A., Kolb, E.W., Schramm, D.N., and Tubbs, D.L. 1976, Astrophys. J., 210, p.481.Google Scholar
Festa, G.G., and Ruderman, M.A. 1969, Phys. Rev., 180, p.1227.CrossRefGoogle Scholar
Feynman, R.P., and Gell-Mann, M. 1958, Phys. Rev., 109, p.193.Google Scholar
Flowers, E., and Itoh, N. 1976, Astrophys. J., 206, p.218.Google Scholar
Flowers, E., and Itoh, N. 1979, Astrophys. J., 230, p.847.Google Scholar
Harnden, F.R., Grant, P.D., Seward, F.D., and Kahn, S.M. 1985, Astrophys. J., 299, p.828.CrossRefGoogle Scholar
Harnden, F.R., and Seward, F.D. 1984, Astrophys. J., 283, p.279.CrossRefGoogle Scholar
Helfand, D.J. 1981, in IAU Symposium 95, Pulsars, ed. Wielebinski, R. and Sieber, W. (Dordrecht: Reidel), p.343.CrossRefGoogle Scholar
Itoh, N., and Kohyama, Y. 1983, Astrophys. J., 275. p.858.Google Scholar
Itoh, N., and Kohyama, Y., Matsumoto, N., and Seki, M. 1984a, Astrophys. J., 280, p.787.CrossRefGoogle Scholar
Itoh, N., Kohyama, Y., Mastumoto, N., and Seki, M. 1984b, Astrophys. J., 285, p.304.CrossRefGoogle Scholar
Itoh, N., Kohyama, J., Matsumoto, N., and Seki, M. 1984c, Astrophys. J., 285, p.758.Google Scholar
Itoh, N., Mastumoto, N., Seki, M., and Kohyama, Y. 1984d, Astrophys. J., 279, p.413.CrossRefGoogle Scholar
Itoh, N., Mitake, S., Iyetomi, H., and Ichimaru, S. 1983, Astrophys. J., 273, p.774.CrossRefGoogle Scholar
Iwamoto, N. 1984, Phys. Rev. Lett., 53, p.1198.Google Scholar
Kohyama, Y., Nakagawa, M., and Itoh, N. 1986, in preparation.Google Scholar
Mitake, S., Ichimaru, S., and Itoh, N. 1984, Astrophys. J., 277, p.375.Google Scholar
Munakata, H., Kohyama, J., and Itoh, N. 1985, Astrophys. J., 296, p. 197.Google Scholar
Munakata, H., Kohyama, J., and Itoh, N. 1986, Astrophys. J., 304, p.580.Google Scholar
Nomoto, K., and Tsuruta, S. 1986, Astrophys. J., 305.Google Scholar
Pye, J.P., Pounds, K.A., Rolf, D.P., Seward, F.D., Smith, A., and Willingale, R: 1981, M.N.R.A.S., 194, p.569.Google Scholar
Raffelt, G.G. 1986, Phys. Lett., 166B, p.402.Google Scholar
Salam, A. 1968, in Elementary Particle Physics, ed. Svartholm, N. (Stockholm: Almqvist and Wiksells), p.367.Google Scholar
Seward, F.D. 1987, talk given at the IAU Symposium No.125 “The Origin and Evolution of Neutron Stars” (Nanjing, China).Google Scholar
Slattery, W.L., Doolen, G.D., and DeWitt, H.E. 1982, Phys. Rev., A26, p.2255.Google Scholar
Tsuruta, S. 1985, Comments on Ap. Google Scholar
Tuohy, I., and Garmire, G. 1980, Astrophys. J.(Letters), 239, L107.CrossRefGoogle Scholar
Yakovlev, D.G., and Urpin, V.A. 1980, Soviet Astr., 24, p.303.Google Scholar
Weinberg, S. 1967, Phys. Rev. Lett., 19, p.1264.Google Scholar