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      A Global Fit Determination of Effective \(\Delta m_{31}^2\) from Baseline Dependence of Reactor \(\bar{\nu}_e\) Disappearance

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          Abstract

          Recently, three reactor neutrino experiments, Daya Bay, Double Chooz and RENO have directly measured the neutrino mixing angle \(\theta_{13}\). In this paper, another important oscillation parameter, effective \(\Delta m_{31}^2\) (= \(\Delta \tilde{m}_{31}^2\)) is measured using baseline dependence of the reactor neutrino disappearance. A global fit is applied to publicly available data and \(\Delta \tilde{m}_{31}^2 = 2.95^{+0.42}_{-0.61} \times 10^{-3}\) eV\(^2\), \(\sin^22\theta_{13} = 0.099^{+0.016}_{-0.012}\) are obtained by setting both parameters free. This result is complementary to \(\Delta tilde{m}_{31}^2\) to be measured by spectrum shape analysis. The measured \(\Delta \tilde{m}_{31}^2\) is consistent with \(\Delta \tilde{m}_{32}^2\) measured by \(\nu_{\mu}\) disappearance in MINOS, T2K and atmospheric neutrino experiments within errors. The minimum \(\chi^2\) is small, which means the results from the three reactor neutrino experiments are consistent with each other.

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          The Reactor Antineutrino Anomaly

          Recently new reactor antineutrino spectra have been provided for 235U, 239Pu, 241Pu and 238U, increasing the mean flux by about 3 percent. To good approximation, this reevaluation applies to all reactor neutrino experiments. The synthesis of published experiments at reactor-detector distances 1.5 eV^2 (95%) and sin^2(2\theta_{new})=0.14(0.08) (95%). Constraints on the theta13 neutrino mixing angle are revised.
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            Erratum: Measurement of the reactor antineutrino flux and spectrum at Daya Bay [Phys. Rev. Lett. 116 , 061801 (2016)]

            F. An (2017)
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              Another possible way to determine the Neutrino Mass Hierarchy

              We show that by combining high precision measurements of the atmospheric delta m^2 in both the electron and muon neutrino (or anti-neutrino) disappearance channels one can determine the neutrino mass hierarchy. The required precision is a very challenging fraction of one per cent for both measurements. At even higher precision, sensitivity to the cosine of the CP violating phase is also possible. This method for determining the mass hierarchy of the neutrino sector does not depend on matter effects.
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                Author and article information

                Journal
                23 April 2013
                2013-08-20
                Article
                10.1016/j.physletb.2013.07.028
                1304.6259
                042fca8d-2459-4acd-b8e2-625290577607

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

                History
                Custom metadata
                Physics Letters B, Volume 725, Issues 4 and 5, 1 October 2013, Pages 271 to 276
                9 pages, 8 figures, edited for Physics Letters B
                hep-ex hep-ph

                High energy & Particle physics
                High energy & Particle physics

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