User:Becarlson/Relativistic runaway electron avalanche

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RREA simulation showing electrons (black), photons (blue), and positrons (red).

Relativistic runaway electron avalanche (RREA) is an avalanche growth of a population of relativistic electrons driven through a material (typically air) by an electric field. RREA has been hypothesized to be related to lightning initiation,[1] terrestrial gamma-ray flashes,[2] sprite lightning lightning,[3] and to spark development.[4] RREA is unique as it can occur at electric fields an order of magnitude lower than the dielectric strength of the material.

Mechanism[edit]

Dynamic friction of free electrons in air compared to an applied electric field showing the runaway electron energy range.

When an electric field is applied to a material, free electrons will drift slowly through the material as described by the electron mobility. For low-energy electrons, faster drift implies higher friction so the drift speed tends to stabilize. For electrons with energy above about 100 keV, however, higher speeds imply lower friction. An electron with a sufficiently high energy therefore may be accelerated by an electric field to even higher and higher energies, encountering less and less friction as it accelerates. Such an electron is described as a "runaway."

As runaway electrons gain energy from an electric field, they occasionally collide with atoms in the material, knocking off secondary electrons. If the secondary electrons also have high enough energy to run away, they too accelerate to high energies, produce further secondary electrons, etc. As such, the total number of energetic electrons grows exponentially in an avalanche.

Seeding[edit]

The RREA mechanism above only describes the growth of the avalanche. An initial energetic electron is needed to start the process. In ambient air, such energetic electrons typically come from cosmic rays[5]. In very strong electric fields, stronger than the maximum frictional force experienced by electrons, even low-energy ("cold" or "thermal") electrons can accelerate to relativistic energies, a process dubbed "thermal runaway."[6]

Feedback[edit]

RREA avalanches generally move opposite the direction of the electric field. As such, after the avalanches leave the electric field region, frictional forces dominate, the electrons lose energy, and the process stops. There is the possibility, however, that photons or positrons produced by the avalanche will wander back to where the avalanche began and can produce new seeds for a second generation of avalanches. If the electric field region is large enough, the number of second-generation avalanches will exceed the number of first-generation avalanches and the number of avalanches itself grows exponentially. This avalanche of avalanches can produce extremely large populations of energetic electrons. This process eventually leads to the decay of the electric field below the level at which feedback is possible and therefore acts as a limit to the large-scale electric field strength.[7]

Effects of RREA[edit]

The large population of energetic electrons produced in RREA will produce a correspondingly large population of energetic photons by bremsstrahlung. These photons are proposed as the source of terrestrial gamma-ray flashes. Large RREA events in thunderstorms may also contribute rare but large radiation doses to commercial airline flights,[8] though this is still a subject of research.

References[edit]

  1. ^ Gurevich, A. V., & Zybin, K. P. (2005). Runaway Breakdown and the Mysteries of Lightning. Physics Today, 58(5), 37. doi: 10.1063/1.1995746.
  2. ^ Dwyer, J. R., & Smith, D. M. (2005). A comparison between Monte Carlo simulations of runaway breakdown and terrestrial gamma-ray flash observations. Geophysical Research Letters, 32(22), L22804. doi: 10.1029/2005GL023848.
  3. ^ Lehtinen, N. G., Bell, T. F., & Inan, U. S. (1999). Monte Carlo simulation of runaway MeV electron breakdown with application to red sprites and terrestrial gamma ray flashes. Journal of Geophysical Research, 104(A11), 24699-24712. doi: 10.1029/1999JA900335.
  4. ^ Betz, H. D., Schumann, U., & Laroche, P. (Eds.). (2009). Lightning: Principles, Instruments and Applications. Springer Verlag, ch. 15.
  5. ^ Carlson, B. E., Lehtinen, N. G., & Inan, U. S. (2008). Runaway relativistic electron avalanche seeding in the Earthʼs atmosphere. Journal of Geophysical Research, 113(A10), A10307. doi: 10.1029/2008JA013210.
  6. ^ Colman, J. J., Roussel-Dupré, R. a, & Triplett, L. (2010). Temporally self-similar electron distribution functions in atmospheric breakdown: The thermal runaway regime. Journal of Geophysical Research, 115, 1-17. doi: 10.1029/2009JA014509.
  7. ^ Dwyer, J. R. (2003). A fundamental limit on electric fields in air. Geophysical Research Letters, 30(20), 2055. doi: 10.1029/2003GL017781.
  8. ^ Dwyer, J. R., Smith, D. M., Uman, M. A., Saleh, Z., Grefenstette, B. W, Hazelton, B. J, et al. (2010). Estimation of the fluence of high-energy electron bursts produced by thunderclouds and the resulting radiation doses received in aircraft. Journal of Geophysical Research, 115(D9), D09206. doi: 10.1029/2009JD012039.
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