Canuto et al. 1970
Canuto, V., C. Chiuderi, and C.K. Chou, 1970: Plasmon neutrinos emission in a strong magnetic field. II: Longitudinal plasmons. Astrophys. Space Sci., 7, 453-460, doi:10.1007/BF00649583.
The decay of a longitudinal plasmon into two neutrinos is studied in the presence of a strong magnetic field. Contrary to the transverse case, for longitudinal plasmons the existence of a new mode, entirely dependent on the magnetic field, greatly enhances the energy loss at high densities. Denoting by QH and QO the neutrino energy losses with and without magnetic field respectively, the situation is as follows: at H ≃ 1011 G and T ≥ 109K, QO ≫ 105 QH for ρ < 101 g/cm3, while QH ≫ 10s10 QO for $pho$ > 1011 g/cm. A second physically interesting feature is the anisotropic character of the energy loss which is highly peaked along the field lines, giving rise to a shorter cooling time in that direction than in any other.
Citation Styles
Show: ACP, AGU, AMS, ApJ, JQSRT, Science style
Canuto, V., Chiuderi, C., and Chou, C.K.: Plasmon neutrinos emission in a strong magnetic field. II: Longitudinal plasmons, Astrophys. Space Sci., 7, 453-460, doi:10.1007/BF00649583, 1970.
Canuto, V., C. Chiuderi, and C.K. Chou (1970), Plasmon neutrinos emission in a strong magnetic field. II: Longitudinal plasmons, Astrophys. Space Sci., 7, 453-460, doi:10.1007/BF00649583.
Canuto, V., C. Chiuderi, and C.K. Chou, 1970: Plasmon neutrinos emission in a strong magnetic field. II: Longitudinal plasmons. Astrophys. Space Sci., 7, 453-460, doi:10.1007/BF00649583.
Canuto, V., Chiuderi, C., & Chou, C.K. 1970, Astrophys. Space Sci., 7, 453, doi:10.1007/BF00649583.
Canuto V, Chiuderi C, Chou CK. Plasmon neutrinos emission in a strong magnetic field. II: Longitudinal plasmons, Astrophys Space Sci 1970;7:453-460. doi:10.1007/BF00649583.
V. Canuto, C. Chiuderi, C.K. Chou, Astrophys. Space Sci. 7, 453-460, doi:10.1007/BF00649583 (1970).
