232 research outputs found

    Mapping The Neutrino Floor For Dark Matter-Electron Direct Detection Experiments

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    We study the discovery reach of future Dark Matter (DM) Direct Detection experiments using DM-electron scattering in the presence of the solar neutrino background. At these low energies traditional methods for nuclear and electronic recoil discrimination fail, implying that the neutrino-{\it nucleus} scattering background can be sizable. We calculate discovery limits based on ionization values of signal and background, and quantify the dependence on the ionization model. Moreover, we explore how the dependence of the DM cross section discovery limits vary with exposure, electronic/nuclear recoil discrimination, DM form factors, and DM astrophysical uncertainties.Comment: 10 pages, 9 figure

    Mapping the Neutrino Floor for Direct Detection Experiments Based on Dark Matter-Electron Scattering

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    We study the discovery reach of future Dark Matter (DM) Direct Detection experiments using DM-electron scattering in the presence of the solar neutrino background. At these low energies traditional methods for nuclear and electronic recoil discrimination fail, implying that the neutrino- nucleusscattering background can be sizable. We calculate discovery limits based on ionization values of signal and background, and quantify the dependence on the ionization model. Moreover, we explore how the dependence of the DM cross section discovery limits varies with exposure, electronic/nuclear recoil discrimination, DM form factors, and DM astrophysical uncertainties

    Contract Grazing on Winter Annuals: Risks and Returns for Cattle Owners

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    Critical factors affecting risk and profitability for cattle owners under contract grazing include cattle weight at purchase and time spent on pasture and feedlot. Buying lighter animals and placing them in pastures before sending them to feedlot is the most profitable as well as least risky option. Even in the least risky scenario, the cattle owner would still incur losses 28% of the times. The results also show a possibility that at contract-grazing rates of $0.41 per pound of gain or more, the cattle owner would place cattle directly on the feedlot, bypassing the pasture.contract grazing, risks, returns, Farm Management, Livestock Production/Industries, Q12,

    Assessing the sensitivity of multi-distance hsNIRS for measuring changes in oxCCO in the brain

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    A hybrid multi-distance hyperspectral near-infrared spectroscopy (hsNIRS) and diffuse correlation spectroscopy (DCS) optical system was used to test transient changes in cytochrome c oxidase (oxCCO) in the brain during carotid compressions (CC) and hypercapnia

    Taking Off the SOCS: Cytokine Signaling Spurs Regeneration

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    Strategies to improve function after CNS injuries must contend with the failure of axons to regrow after transection in adult mammals. In this issue of Neuron, Smith et al. provide an important advance by demonstrating that SOCS3 acts as a key negative regulator of adult optic nerve regeneration

    Dark Matter-Neutrino Interconversion at COHERENT, Direct Detection, and the Early Universe

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    We study a dark matter (DM) model in which the dominant coupling to the standard model occurs through a neutrino-DM-scalar coupling. The new singlet scalar will generically have couplings to nuclei/electrons arising from renormalizable Higgs portal interactions. As a result, the DM particle X can convert into a neutrino via scattering on a target nucleus N: X+N→ν+N, leading to striking signatures at direct detection experiments. Similarly, DM can be produced in neutrino scattering events at neutrino experiments: ν+N→X+N, predicting spectral distortions at experiments such as COHERENT. Furthermore, the model allows for late kinetic decoupling of dark matter with implications for small-scale structure. At low masses, we find that COHERENT and late kinetic decoupling produce the strongest constraints on the model, while at high masses the leading constraints come from DM down-scattering at XENON1T and Borexino. Future improvement will come from CEνNS data, ultralow threshold direct detection, and rare kaon decays
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