Neutrino Bremsstrahlung in an Intense Magnetic Field

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Scientific paper

In this paper we present the neutrino luminosity due to a completely relativistic electron gas in the presence of an intense magnetic field. The neutrino emission rate is determined rigorously, under the assumption of the V-A theory of universal weak Fermi interaction, by standard field-theoretical methods. It is shown that the neutrino radiation rate can be expressed as a function of temperature, density, and the field-strength parameter Θ=HHc, where Hc=m2c3eℏ=4.414×1013 G. Comparisons are made with previous approximate results due to others, and the reasons for discrepancies are discussed.

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