9 research outputs found

    Sterile Neutrino Searches in Neutrino Oscillation Experiments

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    Beta and neutrinoless double beta decays with KeV sterile fermions

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    Sterile Neutrinos or Flux Uncertainties? - Status of the Reactor Anti-Neutrino Anomaly

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    The ∌3σ\sim 3\sigma discrepancy between the predicted and observed reactor anti-neutrino flux, known as the reactor anti-neutrino anomaly, continues to intrigue. The recent discovery of an unexpected bump in the reactor anti-neutrino spectrum, as well as indications that the flux deficit is different for different fission isotopes seems to disfavour the explanation of the anomaly in terms of sterile neutrino oscillations. We critically review this conclusion in view of all available data on electron (anti)neutrino disappearance. We find that the sterile neutrino hypothesis cannot be rejected based on global data and is only mildly disfavored compared to an individual rescaling of neutrino fluxes from different fission isotopes. The main reason for this is the presence of spectral features in recent data from the NEOS and DANSS experiments. If state-of-the-art predictions for reactor fluxes are taken at face value, sterile neutrino oscillations allow a consistent description of global data with a significance close to 3σ3\sigma relative to the no-oscillation case. Even if reactor fluxes and spectra are left free in the fit, a 2σ2\sigma hint in favour of sterile neutrinos remains, with allowed parameter regions consistent with an explanation of the anomaly in terms of oscillations.Comment: 25 pages, 5 figures. 1 page and table 4 added. Published in JHE

    Outcomes from elective colorectal cancer surgery during the SARS-CoV-2 pandemic

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    This study aimed to describe the change in surgical practice and the impact of SARS-CoV-2 on mortality after surgical resection of colorectal cancer during the initial phases of the SARS-CoV-2 pandemic

    Beta and Neutrinoless Double Beta Decays with KeV Sterile Fermions

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    International audienceMotivated by the capability of the KATRIN experiment to explore the existence of KeV neutrinos in the [1 − 18.5] KeV mass range, we explore the viability of minimal extensions of the Standard Model involving sterile neutrinos (namely the 3 + N frameworks) and study their possible impact in both the beta energy spectrum and the neutrinoless double beta decay effective mass, for the two possible ordering cases for the light neutrino spectrum. We also explore how both observables can discriminate between motivated low-scale seesaw realizations involving KeV sterile neutrinos. Our study concerns the prospect of a Type-I seesaw with two right-handed neutrinos, and a combination of the inverse and the linear seesaws where the Standard Model is minimally extended by two quasi-degenerate sterile fermions. We also discuss the possibility of exploring the latter case searching for double-kinks in KATRIN

    Updated global analysis of neutrino oscillations in the presence of eV-scale sterile neutrinos

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    We discuss the possibility to explain the anomalies in short-baseline neutrino oscillation experiments in terms of sterile neutrinos. We work in a 3 + 1 framework and pay special attention to recent new data from reactor experiments, IceCube and MINOS+. We find that results from the DANSS and NEOS reactor experiments support the sterile neutrino explanation of the reactor anomaly, based on an analysis that relies solely on the relative comparison of measured reactor spectra. Global data from the Îœe_{e} disappearance channel favour sterile neutrino oscillations at the 3σ level with Δm412_{41}^{2}  ≈ 1.3 eV2^{2} and |Ue4_{e4}| ≈ 0.1, even without any assumptions on predicted reactor fluxes. In contrast, the anomalies in the Îœe_{e} appearance channel (dominated by LSND) are in strong tension with improved bounds on ΜΌ_{ÎŒ} disappearance, mostly driven by MINOS+ and IceCube. Under the sterile neutrino oscillation hypothesis, the p-value for those data sets being consistent is less than 2.6 × 10−6^{−6}. Therefore, an explanation of the LSND anomaly in terms of sterile neutrino oscillations in the 3 + 1 scenario is excluded at the 4.7σ level. This result is robust with respect to variations in the analysis and used data, in particular it depends neither on the theoretically predicted reactor neutrino fluxes, nor on constraints from any single experiment. Irrespective of the anomalies, we provide updated constraints on the allowed mixing strengths |Uα4_{α4}| (α = e, ÎŒ, τ ) of active neutrinos with a fourth neutrino mass state in the eV range.We discuss the possibility to explain the anomalies in short-baseline neutrino oscillation experiments in terms of sterile neutrinos. We work in a 3+1 framework and pay special attention to recent new data from reactor experiments, IceCube and MINOS+. We find that results from the DANSS and NEOS reactor experiments support the sterile neutrino explanation of the reactor anomaly, based on an analysis that relies solely on the relative comparison of measured reactor spectra. Global data from the Îœe\nu_e disappearance channel favour sterile neutrino oscillations at the 3σ3\sigma level with Δm412≈1.3\Delta m^2_{41} \approx 1.3 eV2^2 and ∣Ue4∣≈0.1|U_{e4}| \approx 0.1, even without any assumptions on predicted reactor fluxes. In contrast, the anomalies in the Îœe\nu_e appearance channel (dominated by LSND) are in strong tension with improved bounds on ΜΌ\nu_\mu disappearance, mostly driven by MINOS+ and IceCube. Under the sterile neutrino oscillation hypothesis, the p-value for those data sets being consistent is less than 2.6×10−62.6\times 10^{-6}. Therefore, an explanation of the LSND anomaly in terms of sterile neutrino oscillations in the 3+1 scenario is excluded at the 4.7σ4.7\sigma level. This result is robust with respect to variations in the analysis and used data, in particular it depends neither on the theoretically predicted reactor neutrino fluxes, nor on constraints from any single experiment. Irrespective of the anomalies, we provide updated constraints on the allowed mixing strengths ∣Uα4∣|U_{\alpha 4}| (α=e,ÎŒ,τ\alpha = e,\mu,\tau) of active neutrinos with a fourth neutrino mass state in the eV range
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