Detecting dark energy in long baseline neutrino oscillations

  • In this paper, we discuss a possibility of studying properties of dark energy in long baseline neutrino oscillation experiments. We consider two types of models of neutrino dark energy. For one type of models the scalar field is taken to be quintessence-like and for the other phantom-like. In these models the scalar fields couple to the neutrinos to give rise to spatially varying neutrino masses. We will show that the two types of models predict different behaviors of the spatial variation of the neutrino masses inside the Earth and consequently result in different signals in long baseline neutrino oscillation experiments.

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GU Pei-Hong, BI Xiao-Jun, FENG Bo, YOUNG Bing-Lin and ZHANG Xin-Min. Detecting dark energy in long baseline neutrino oscillations[J]. Chinese Physics C, 2008, 32(7): 530-535. doi: 10.1088/1674-1137/32/7/004
GU Pei-Hong, BI Xiao-Jun, FENG Bo, YOUNG Bing-Lin and ZHANG Xin-Min. Detecting dark energy in long baseline neutrino oscillations[J]. Chinese Physics C, 2008, 32(7): 530-535.  doi: 10.1088/1674-1137/32/7/004 shu
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Received: 2007-10-08
Revised: 2007-10-25
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Detecting dark energy in long baseline neutrino oscillations

    Corresponding author: BI Xiao-Jun,

Abstract: 

In this paper, we discuss a possibility of studying properties of dark energy in long baseline neutrino oscillation experiments. We consider two types of models of neutrino dark energy. For one type of models the scalar field is taken to be quintessence-like and for the other phantom-like. In these models the scalar fields couple to the neutrinos to give rise to spatially varying neutrino masses. We will show that the two types of models predict different behaviors of the spatial variation of the neutrino masses inside the Earth and consequently result in different signals in long baseline neutrino oscillation experiments.

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