Abstract
This chapter is devoted to an analysis of the dispersion properties of photons and neutrinos in external active media: magnetic field, plasma, and magnetized plasma. Possible astrophysical manifestations of particle processes influenced by external active media are also considered.
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Notes
- 1.
Note that the sign of the effective Lagrangian is significant in this case, since the additional neutrino energy is the linear in \(G_{\mathrm{F }}\) effect. In the calculation of probabilities and cross sections of weak processes, which are proportional to \(G_\mathrm{F }^2\), the sign of the effective Lagrangian does not appear.
- 2.
Strictly speaking, a particle that interacts with the magnetic moment of neutrinos, and at the same time, is sterile with respect to the interactions with electrically charged plasma particles, should not be called a photon.
- 3.
The sign \(\pm \) at the linear in the field term in Eq. (13) of Ref. [39] came from poorly chosen notations: the neutrino momentum in this article was \(\mathbf{{k}}\), while the antineutrino momentum was \(-\mathbf{{k}}\) (G. Raffelt, private communication).
- 4.
We perform our calculations in the gauge \(A^\mu =(0,0,Bx,0)\); the magnetic field is directed along the third axis \(\mathbf{{B}} = (0, 0, B)\).
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Kuznetsov, A., Mikheev, N. (2013). Particle Dispersion in External Active Media. In: Electroweak Processes in External Active Media. Springer Tracts in Modern Physics, vol 252. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-36226-2_4
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