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arXiv · 0905.2382

Mass Hierarchy Determination for $θ_{13}=0$ and Atmospheric Neutrinos

Raj Gandhi·Pomita Ghoshal·Srubabati Goswami·S Uma Sankar
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Abstract

We examine the possibility of determining the neutrino mass hierarchy in the limit θ_{13} = 0 using atmospheric neutrinos as the source. In this limit, in which θ_{13} driven matter effects are absent, independent measurements of Δ_{31} and Δ_{32} can, in principle, lead to hierarchy determination. Since the difference between these two is Δ_{21}, one needs an experimental arrangement where Δ_{21} L/E \gtrsim 1 can be achieved. This condition can be satisfied by atmospheric neutrinos since they have a large range of energies and baselines. In spite of this, we find that hierarchy determination in the θ_{13}=0 limit with atmospheric neutrinos is not a realistic possibility, even in conjunction with an apparently synergistic beam experiment like T2K or NOvA. We discuss the reasons for this, and also in the process clarify the conditions that must be satisfied in general for hierarchy determination if θ_{13} = 0.

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Raj Gandhi, Pomita Ghoshal, Srubabati Goswami, S Uma Sankar. 2009-08-13. Mass Hierarchy Determination for $θ_{13}=0$ and Atmospheric Neutrinos. https://doi.org/10.1142/s0217732310033086

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