de.mpg.escidoc.pubman.appbase.FacesBean
English
 
Help Guide Disclaimer Contact us Login
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT

Released

Journal Article

Neutrino production coherence and oscillation experiments

MPS-Authors
http://pubman.mpdl.mpg.de/cone/persons/resource/persons30246

Akhmedov,  Evgeny
Division Prof. Dr. Manfred Lindner, MPI for Nuclear Physics, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons31060

Smirnov,  A. Y.
Division Prof. Dr. Manfred Lindner, MPI for Nuclear Physics, Max Planck Society;

Locator
There are no locators available
Fulltext (public)

1201.4128
(Preprint), 4KB

Supplementary Material (public)
There is no public supplementary material available
Citation

Akhmedov, E., Hernandez, D., & Smirnov, A. Y. (2012). Neutrino production coherence and oscillation experiments. Journal of high energy physics: JHEP, 04: 052, pp. 1-37. Retrieved from http://arxiv.org/abs/1201.4128.


Cite as: http://hdl.handle.net/11858/00-001M-0000-000E-AB7D-3
Abstract
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\to \mu \nu \ 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}\ne 0 is shown to be \sim [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.