1,452 research outputs found

    A Monometallic Iron(I) Organoferrate

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    Tetra-n-butylammonium (TBA) (eta(6)-biphenyl)diphenyfferrate was formed unexpectedly in the reaction of (TBA)(2)[Fe4S4Cl4] with an excess of phenyllithium. This complex belongs to a novel type of organoferrate

    Direct comparison of sterile neutrino constraints from cosmological data, νe\nu_{e} disappearance data and νμνe\nu_{\mu}\rightarrow\nu_{e} appearance data in a 3+13+1 model

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    We present a quantitative, direct comparison of constraints on sterile neutrinos derived from neutrino oscillation experiments and from Planck data, interpreted assuming standard cosmological evolution. We extend a 1+11+1 model, which is used to compare exclusions contours at the 95% CL derived from Planck data to those from νe\nu_{e}-disappearance measurements, to a 3+13+1 model. This allows us to compare the Planck constraints with those obtained through νμνe\nu_{\mu}\rightarrow\nu_{e} appearance searches, which are sensitive to more than one active-sterile mixing angle. We find that the cosmological data fully exclude the allowed regions published by the LSND, MiniBooNE and Neutrino-4 collaborations, and those from the gallium and rector anomalies, at the 95% CL. Compared to the exclusion regions from the Daya Bay νe\nu_{e}-disappearance search, the Planck data are more strongly excluding above Δm4120.1eV2|\Delta m^{2}_{41}|\approx 0.1\, \mathrm{eV}^{2} and meffsterile0.2eVm_\mathrm{eff}^\mathrm{sterile}\approx 0.2\, \mathrm{eV}, with the Daya Bay exclusion being stronger below these values. Compared to the combined Daya Bay/Bugey/MINOS exclusion region on νμνe\nu_{\mu}\rightarrow\nu_{e} appearance, the Planck data is more strongly excluding above Δm4125×102eV2\Delta m^{2}_{41}\approx 5\times 10^{-2}\,\mathrm{eV}^{2}, with the exclusion strengths of the Planck data and the Daya Bay/Bugey/MINOS combination becoming comparable below this value.Comment: 9 pages, 4 figures, accepted by Eur. Phys. J.

    A Monometallic Iron(I) Organoferrate

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    Sensing remote nuclear spins

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    Sensing single nuclear spins is a central challenge in magnetic resonance based imaging techniques. Although different methods and especially diamond defect based sensing and imaging techniques in principle have shown sufficient sensitivity, signals from single nuclear spins are usually too weak to be distinguished from background noise. Here, we present the detection and identification of remote single C-13 nuclear spins embedded in nuclear spin baths surrounding a single electron spins of a nitrogen-vacancy centre in diamond. With dynamical decoupling control of the centre electron spin, the weak magnetic field ~10 nT from a single nuclear spin located ~3 nm from the centre with hyperfine coupling as weak as ~500 Hz is amplified and detected. The quantum nature of the coupling is confirmed and precise position and the vector components of the nuclear field are determined. Given the distance over which nuclear magnetic fields can be detected the technique marks a firm step towards imaging, detecting and controlling nuclear spin species external to the diamond sensor

    Direct comparison of sterile neutrino constraints from cosmological data, ν e disappearance data and ν μ → ν e appearance data in a 3 + 1 model

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    From Springer Nature via Jisc Publications RouterHistory: received 2020-02-22, registration 2020-07-03, accepted 2020-07-03, pub-print 2020-08, pub-electronic 2020-08-19, online 2020-08-19Publication status: PublishedFunder: H2020 Marie Sklodowska-Curie Actions; doi: http://dx.doi.org/10.13039/100010665; Grant(s): 752309Abstract: We present a quantitative, direct comparison of constraints on sterile neutrinos derived from neutrino oscillation experiments and from Planck data, interpreted assuming standard cosmological evolution. We extend a 1+1 model, which is used to compare exclusion contours at the 95% Cl derived from Planck data to those from νe-disappearance measurements, to a 3+1 model. This allows us to compare the Planck constraints with those obtained through νμ→νe appearance searches, which are sensitive to more than one active-sterile mixing angle. We find that the cosmological data fully exclude the allowed regions published by the LSND, MiniBooNE and Neutrino-4 collaborations, and those from the gallium and rector anomalies, at the 95% Cl. Compared to the exclusion region from the Daya Bay νe-disappearance search, the Planck data are more strongly excluding above |Δm412|≈0.1eV2 and meffsterile≈0.2eV, with the Daya Bay exclusion being stronger below these values. Compared to the combined Daya Bay/Bugey/MINOS exclusion region on νμ→νe appearance, the Planck data is more strongly excluding above Δm412≈5×10-2eV2, with the exclusion strengths of the Planck data and the Daya Bay/Bugey/MINOS combination becoming comparable below this value

    Optimal frequency measurements with quantum probes

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    Precise frequency measurements are important in applications ranging from navigation and imaging to computation and communication. Here we outline the optimal quantum strategies for frequency discrimination and estimation in the context of quantum spectroscopy, and we compare the effectiveness of different readout strategies. Using a single NV center in diamond, we implement the optimal frequency discrimination protocol to discriminate two frequencies separated by 2 kHz with a single 44 μs measurement, a factor of ten below the Fourier limit. For frequency estimation, we achieve a frequency sensitivity of 1.6 µHz/Hz2 for a 1.7 µT amplitude signal, which is within a factor of 2 from the quantum limit. Our results are foundational for discrimination and estimation problems in nanoscale nuclear magnetic resonance spectroscopy
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