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Cosmic Explosions pp 315–320Cite as

Neutrino Gas in Equilibrium with Self-Interaction

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Part of the book series: Springer Proceedings in Physics ((SPPHY,volume 99))

Summary

We study a neutrino gas in equilibrium both at T = 0 and at finite temperature. The neutrinos are assumed to be massive Dirac particles with two generations interacting with each other via neutral currents and with a background of matter. We analyze the main properties of the neutrino eigenmodes in the medium, such as effective masses and mixing angle.

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Author information

Authors and Affiliations

  1. Departamento de Astronomia y Astrofísica, Universidad de Valencia, 46100, Burjassot (Valencia), Spain

    M. Sirera

  2. Departamento de Física Teórica, Universidad de Valencia, 46100, Burjassot (Valencia), Spain

    A. Perez

Authors
  1. M. Sirera
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  2. A. Perez
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Editor information

Editors and Affiliations

  1. Depto. Astronomia y Astrofisica, Universidad de Valencia, Calle Dr. Moliner 50, 46100, Burjassot, Spain

    Juan-María Marcaide

  2. Naval Research Laboratory, Code 7213, Washington, DC, 20375-5320, USA

    Kurt W. Weiler

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© 2005 Springer-Verlag Berlin Heidelberg

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Sirera, M., Perez, A. (2005). Neutrino Gas in Equilibrium with Self-Interaction. In: Marcaide, JM., Weiler, K.W. (eds) Cosmic Explosions. Springer Proceedings in Physics, vol 99. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-26633-X_43

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