728 research outputs found

    Comment on "Fano Resonance for Anderson Impurity Systems"

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    In a recent Letter, Luo et al. (Phys. Rev. Lett. 92, 256602 (2004)) analyze the Fano line shapes obtained from scanning tunneling spectroscopy (STS) of transition metal impurities on a simple metal surface, in particular of the Ti/Au(111) and Ti/Ag(100) systems. As the key point of their analysis, they claim that there is not only a Fano interference effect between the impurity d-orbital and the conduction electron continuum, as derived in Ujsaghy et al. (Phys. Rev. Lett. 85, 2557 (2000)), but that the Kondo resonance in the d-electron spectral density has by itself a second Fano line shape, leading to the experimentally observed spectra. In the present note we point out that this analysis is conceptually incorrect. Therefore, the quantitative agreement of the fitted theoretical spectra with the experimental results is meaningless.Comment: 1 page, no figures. Accepted for publication in PRL; revised version uploaded on November 18th, 200

    Neutrino anomalies and future prospects in neutrino physics

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    I give an overview of some of the several anomalies appearing in neutrino oscillation experiments, setting particular focus to the reactor antineutrino anomaly and the Gallium anomaly. I will discuss these two anomalies in some detail and, in particular, compare their explanation due to neutrino oscillations in presence of a light sterile neutrino among each other and also with the bounds from the analyses of reactor spectral ratio data, β-decay data, and solar neutrino data

    Status of neutrino oscillations 2018: first hint for normal mass ordering and improved CP sensitivity

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    We present a new global fit of neutrino oscillation parameters within the simplest three-neutrino picture, including new data which appeared since our previous analysis~\cite{Forero:2014bxa}. In this update we include new long-baseline neutrino data involving the antineutrino channel in T2K, as well as new data in the neutrino channel, data from NOν\nuA, as well as new reactor data, such as the Daya Bay 1230 days electron antineutrino disappearance spectrum data and the 1500 live days prompt spectrum from RENO, as well as new Double Chooz data. We also include atmospheric neutrino data from the IceCube DeepCore and ANTARES neutrino telescopes and from Super-Kamiokande. Finally, we also update our solar oscillation analysis by including the 2055-day day/night spectrum from the fourth phase of the Super-Kamiokande experiment. With the new data we find a preference for the atmospheric angle in the upper octant for both neutrino mass orderings, with maximal mixing allowed at Δχ2=1.6(3.2)\Delta\chi^2 = 1.6 \, (3.2) for normal (inverted) ordering. We also obtain a strong preference for values of the CP phase δ\delta in the range [π,2π][\pi,2\pi], excluding values close to π/2\pi/2 at more than 4σ\sigma. More remarkably, our global analysis shows for the first time hints in favour of the normal mass ordering over the inverted one at more than 3σ\sigma. We discuss in detail the origin of the mass ordering, CP violation and octant sensitivities, analyzing the interplay among the different neutrino data samples.Comment: Updated neutrino oscillation analysis using the most recent results from T2K, NOν\nuA, RENO and Super-Kamiokande. 17 pages, 8 figures, 1 tabl

    Inspection of the detection cross section dependence of the Gallium Anomaly

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    We discuss in detail the dependence of the Gallium Anomaly on the detection cross section. We provide updated values of the size of the Gallium Anomaly and find that its significance is larger than about 5σ5\sigma for all the detection cross section models. We discuss the dependence of the Gallium Anomaly on the assumed value of the half life of 71Ge{}^{71}\text{Ge}, which determines the cross sections of the transitions from the ground state of 71Ga{}^{71}\text{Ga} to the ground state of 71Ge{}^{71}\text{Ge}. We show that a value of the 71Ge{}^{71}\text{Ge} half life which is larger than the standard one can reduce or even solve the Gallium Anomaly. Considering the short-baseline neutrino oscillation interpretation of the Gallium Anomaly, we show that a value of the 71Ge{}^{71}\text{Ge} half life which is larger than the standard one can reduce the tension with the results of other experiments. Since the standard value of the 71Ge{}^{71}\text{Ge} half life was measured in 1985, we advocate the importance of new measurements with modern technique and apparatus for a better assessment of the Gallium Anomaly.Comment: v3: 11 pages, 4 figures, 3 tables, references added, typo correcte

    Quantum Decoherence effects on precision measurements at DUNE and T2HK

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    We investigate the potential impact of neutrino quantum decoherence on the precision measurements of standard neutrino oscillation parameters in the DUNE and T2HK experiments. We show that the measurement of δCP\delta_\text{CP}, sin2θ13\sin^2\theta_{13} and sin2θ23\sin^2\theta_{23} is stronger effected in DUNE than in T2HK. On the other hand, DUNE would have a better sensitivity than T2HK to observe decoherence effects. By performing a combined analysis of DUNE and T2HK we show that a robust measurement of standard parameters would be possible, which is not guaranteed with DUNE data alone.Comment: v2: matches version accepted for publication, v1: 19 pages, 9 figures, 1 tabl

    Sterile neutrinos with altered dispersion relations revisited

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    In this paper we investigate neutrino oscillations with altered dispersion relations in the presence of sterile neutrinos. Modified dispersion relations represent an agnostic way to parameterize new physics. Models of this type have been suggested to explain global neutrino oscillation data, including deviations from the standard three-neutrino paradigm as observed by a few experiments. We show that, unfortunately, in this type of models new tensions arise turning them incompatible with global data.Comment: 22 pages, 7 figures, 2 tables. Version 2, matches published versio

    Gallium Anomaly: Critical View from the Global Picture of νe\nu_{e} and νˉe\bar\nu_{e} Disappearance

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    The significance of the Gallium Anomaly, from the BEST, GALLEX, and SAGE radioactive source experiments, is quantified using different theoretical calculations of the neutrino detection cross section, and its explanation due to neutrino oscillations is compared with the bounds from the analyses of reactor rate and spectral ratio data, β\beta-decay data, and solar neutrino data. In the 3+1 active-sterile neutrino mixing scheme, the Gallium Anomaly is in strong tension with the individual and combined bounds of these data sets. In the combined scenario with all available data, the parameter goodness of fit is below 0.042%, corresponding to a severe tension of 4-5σ\sigma, or stronger. Therefore, we conclude that one should pursue other possible solutions beyond short-baseline oscillations for the Gallium Anomaly. We also present a new global fit of νe\nu_e and νˉe\bar\nu_e disappearance data, showing that there is a 2.6-3.3σ\sigma preference in favor of short-baseline oscillations, which is driven by an updated analysis of reactor spectral ratio data.Comment: 20 pages, 10 figures. With more discussions, version accepted for publication at Journal of High Energy Physic

    Zooming in on neutrino oscillations with DUNE

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    We examine the capabilities of the DUNE experiment as a probe of the neutrino mixing paradigm. Taking the current status of neutrino oscillations and the design specifications of DUNE, we determine the experiment's potential to probe the structure of neutrino mixing and CP violation. We focus on the poorly determined parameters θ23 and δCP and consider both two and seven years of run. We take various benchmarks as our true values, such as the current preferred values of θ23 and δCP, as well as several theorymotivated choices. We determine quantitatively DUNE's potential to perform a precision measurement of θ23, as well as to test the CP violation hypothesis in a model-independent way. We find that, after running for seven years, DUNE will make a substantial step in the precise determination of these parameters, bringing to quantitative test the predictions of various theories of neutrino mixing
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