Publication Abstracts

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 ρ > 1011 g/cm3. 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.

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BibTeX Citation

@article{ca01110v,
  author={Canuto, V. and Chiuderi, C. and Chou, C. K.},
  title={Plasmon neutrinos emission in a strong magnetic field. II: Longitudinal plasmons},
  year={1970},
  journal={Astrophys. Space Sci.},
  volume={7},
  pages={453--460},
  doi={10.1007/BF00649583},
}

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RIS Citation

TY  - JOUR
ID  - ca01110v
AU  - Canuto, V.
AU  - Chiuderi, C.
AU  - Chou, C. K.
PY  - 1970
TI  - Plasmon neutrinos emission in a strong magnetic field. II: Longitudinal plasmons
JA  - Astrophys. Space Sci.
VL  - 7
SP  - 453
EP  - 460
DO  - 10.1007/BF00649583
ER  -

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