Neutrino production coherence and oscillation experiments

作者：Akhmedov E Kh^*; Hernandez D; Smirnov A Yu

来源：The Journal of High Energy Physics, 2012, 2012(4): 052.

DOI：10.1007/JHEP04(2012)052

• Neutrino Physics
• Solar and Atmospheric Neutrinos

Neutrino oscillations are only observable when the neutrino production, propagation and detection coherence conditions are satisfied. In this paper we consider in detail neutrino production coherence, taking pi -> mu v decay as an example. We compare the oscillation probabilities obtained in two different ways: (1) coherent summation of the amplitudes of neutrino production at different points along the trajectory of the parent pion; (2) averaging of the standard oscillation probability over the neutrino production coordinate in the source. We demonstrate that the results of these two different approaches exactly coincide, provided that the parent pion is considered as pointlike and the detection process is perfectly localized. In this case the standard averaging of the oscillation probability over the finite spatial extensions of the neutrino source (and detector) properly takes possible decoherence effects into account. We analyze the reason for this equivalence of the two approaches and demonstrate that for pion wave packets of finite width sigma(x pi) the equivalence is broken. The leading order correction to the oscillation probability due to sigma(x pi) not equal 0 is shown to be similar to [v(g)/(v(g) - v(pi))]sigma(x pi)/l(osc), where v(g) and v(pi) are the group velocities of the neutrino and pion wave packets, and l(osc) is the neutrino oscillation length.

• 出版日期2012-4