Abstract
Using a semiclassical approach, we analyze the collective behavior of neutrinos and antineutrinos in a dense background. Applying the Wigner transform technique, we show that the interaction can be modeled by a coupled system of nonlinear Vlasov-like equations. From these equations, we derive a dispersion relation for neutrino-antineutrino interactions on a general background. The dispersion relation admits a novel modulational instability. Moreover, we investigate the modifications of the instability due to thermal effects. The results are examined, together with a numerical example, and we discuss the induced density inhomogeneities using parameters relevant to the early Universe.
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From Zhurnal Éksperimental’no\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l}\) i Teoretichesko\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l}\) Fiziki, Vol. 126, No. 1, 2004, pp. 14–25.
Original English Text Copyright © 2004 by Marklund, Shukla, Betschart, Stenflo, Anderson, Lisak.
This article was submitted by the authors in English.
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Marklund, M., Shukla, P.K., Betschart, G. et al. Modulational instabilities in neutrino-antineutrino interactions. J. Exp. Theor. Phys. 99, 9–18 (2004). https://doi.org/10.1134/1.1787073
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DOI: https://doi.org/10.1134/1.1787073