Hostname: page-component-586b7cd67f-rcrh6 Total loading time: 0 Render date: 2024-11-22T05:43:27.019Z Has data issue: false hasContentIssue false
  • English
  • Français

Langmuir Wave Emission by Neutrinos in a Medium

Published online by Cambridge University Press:  25 April 2016

S. J. Hardy  and
D. B. Melrose
S. J. Hardy
Affiliation:
Research Centre for Theoretical Astrophysics, School of Physics, University of Sydney, NSW 2006, [email protected]
D. B. Melrose
Affiliation:
Research Centre for Theoretical Astrophysics, School of Physics, University of Sydney, NSW 2006, [email protected]
Get access Rights & Permissions [Opens in a new window]

Abstract

Expressions for the probability per unit time of the emission of a Langmuir wave by both massive and massless neutrinos moving in a medium are derived using finite-temperature field theory. A comparison between this process and the analogous emission from an electron is made, and possible implications of this process for the explosion mechanisms of type II supernovae are briefly discussed.

Keywords

neutrinosplasmasstars: supernovae: general
Type
High-energy Astrophysics
Information
Publications of the Astronomical Society of Australia , Volume 13 , Issue 2 , May 1996 , pp. 144 - 149
Copyright
Copyright © Astronomical Society of Australia 1996

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Baron, E. A., & Cooperstein, J. 1990, ApJ, 353, 597 CrossRefGoogle Scholar
Bethe, H. A. 1986, Phys. Rev. Lett., 56, 1305 CrossRefGoogle Scholar
Bethe, H. A. 1990, Rev. Mod. Phys., 62, 801 CrossRefGoogle Scholar
Bingham, R., Dawson, J. M., Su, J. J., & Bethe, H. A. 1994, Phys. Lett. A, 193, 279 CrossRefGoogle Scholar
Braaten, E. 1991, Phys. Rev. Lett., 66, 1655 CrossRefGoogle Scholar
Braaten, E., & Segel, D. 1993, Phys. Rev. D, 48, 1478 CrossRefGoogle Scholar
Burrows, A., Hayes, J., & Fryxell, B. A. 1995, ApJ, 450, 830 CrossRefGoogle Scholar
Dolan, L., & Jackiw, R. 1974, Phys. Rev. D, 9, 3320 CrossRefGoogle Scholar
D’Olivo, J. C., Nieves, J. F., & Pal, B.A. 1989, Phys. Rev. D, 40, 3679 CrossRefGoogle Scholar
D’Olivo, J. C., Nieves, J. F., & Pal, P.B. 1990, Phys. Rev. Lett., 64, 1088 CrossRefGoogle Scholar
D’Olivo, J. C., Nieves, J. F., & Torres, M. 1992, Phys. Rev. D, 46, 1172 CrossRefGoogle Scholar
Gedalin, M., & Eichler, D. 1993, ApJ, 406, 629 CrossRefGoogle Scholar
Giunti, C., Kim, C. W., & Lam, W. P. 1991, Phys. Rev. D, 43, 164 CrossRefGoogle Scholar
Kim, C. W., & Pevsner, A. 1993, Neutrinos in Physics and Astrophysics (New York: Harwood Academic)Google Scholar
Melrose, D. B. 1982, Aust. J. Phys., 35, 41 CrossRefGoogle Scholar
Melrose, D. B. 1986, Instabilities in Space and Laboratory Plasmas (Cambridge Univ. Press)CrossRefGoogle Scholar
Melrose, D. B. 1994, J. Plasma Phys., 51, 13 CrossRefGoogle Scholar
Melrose, D. B., & Stenhouse, J. E. 1977, Aust. J. Phys., 30, 481 CrossRefGoogle Scholar
Miller, S. D., Wilson, J. R., & Mayle, R. W. 1993, ApJ, 415, 278 CrossRefGoogle Scholar
Nieves, J. F. 1989, Phys. Rev. D, 40, 866 CrossRefGoogle Scholar
Nieves, J. F., & Pal, P. B. 1989, Phys. Rev. D, 39, 652 CrossRefGoogle Scholar
Nieves, J. F., & Pal, P. B. 1994, Phys. Rev. D, 49, 1398 CrossRefGoogle Scholar
Oraevsky, V. N., & Semikoz, V. B. 1987, Physica, 142A, 135 CrossRefGoogle Scholar
Silin, V. P. 1960, Sov. Phys. JETP, 11, 1136 Google Scholar
Tsytovich, V. N. 1964, Sov. Phys. JETP, 18, 816 Google Scholar
Weldon, H. A. 1982, Phys. Rev. D, 26, 1394 CrossRefGoogle Scholar
Wilson, J. R. 1984, in Numerical Astrophysics, ed. Centrella, J. M., LeBlanc, J. M. & Bowers, R. L. (Boston: Jones & Barlett), 422 Google Scholar