101 research outputs found

    Observations of Dicke narrowing and speed dependence in air-broadened CO_2 lineshapes near 2.06 ÎŒm

    Get PDF
    Frequency-stabilized cavity ring-down spectroscopy was used to study CO_2 lineshapes in the (20013) ← (00001) band centered near 2.06 ÎŒm. Two rovibrational transitions were chosen for this study to measure non-Voigt collisional effects for air-broadened lines over the pressure range of 7 kPa–28 kPa. Lineshape analysis for both lines revealed evidence of simultaneous Dicke (collisional) narrowing and speed-dependent effects that would introduce biases exceeding 2% in the retrieved air-broadening parameters if not incorporated in the modeling of CO_2 lineshapes. Additionally, correlations between velocity- and phase/state changing collisions greatly reduced the observed Dicke narrowing effect. As a result, it was concluded that the most appropriate line profile for modeling CO_2 lineshapes near 2.06 ÎŒm was the correlated speed-dependent Nelkin-Ghatak profile, which includes all of the physical effects mentioned above and leads to a consistent set of line shape parameters that are linear with gas pressure

    Impact of cross-section uncertainties on supernova neutrino spectral parameter fitting in the Deep Underground Neutrino Experiment

    Get PDF
    A primary goal of the upcoming Deep Underground Neutrino Experiment (DUNE) is to measure the O(10)\mathcal{O}(10) MeV neutrinos produced by a Galactic core-collapse supernova if one should occur during the lifetime of the experiment. The liquid-argon-based detectors planned for DUNE are expected to be uniquely sensitive to the Îœe\nu_e component of the supernova flux, enabling a wide variety of physics and astrophysics measurements. A key requirement for a correct interpretation of these measurements is a good understanding of the energy-dependent total cross section σ(EÎœ)\sigma(E_\nu) for charged-current Îœe\nu_e absorption on argon. In the context of a simulated extraction of supernova Îœe\nu_e spectral parameters from a toy analysis, we investigate the impact of σ(EÎœ)\sigma(E_\nu) modeling uncertainties on DUNE's supernova neutrino physics sensitivity for the first time. We find that the currently large theoretical uncertainties on σ(EÎœ)\sigma(E_\nu) must be substantially reduced before the Îœe\nu_e flux parameters can be extracted reliably: in the absence of external constraints, a measurement of the integrated neutrino luminosity with less than 10\% bias with DUNE requires σ(EÎœ)\sigma(E_\nu) to be known to about 5%. The neutrino spectral shape parameters can be known to better than 10% for a 20% uncertainty on the cross-section scale, although they will be sensitive to uncertainties on the shape of σ(EÎœ)\sigma(E_\nu). A direct measurement of low-energy Îœe\nu_e-argon scattering would be invaluable for improving the theoretical precision to the needed level.Comment: 25 pages, 21 figure

    Eau (droit pénal)

    No full text
    Sironneau Jacques. Eau (droit pénal). In: Revue Juridique de l'Environnement, n°4, 2000. p. 648

    Eau

    No full text
    Sironneau Jacques. Eau. In: Revue Juridique de l'Environnement, n°1, 2004. pp. 67-84

    Eau (2e partie)

    No full text
    Sironneau Jacques. Eau (2e partie). In: Revue Juridique de l'Environnement, n°3, 2013. pp. 529-543

    Eau

    No full text
    Sironneau Jacques. Eau. In: Revue Juridique de l'Environnement, n°1, 2016. pp. 153-162

    Eau

    No full text
    Sironneau Jacques. Eau. In: Revue Juridique de l'Environnement, n°3, 2009. pp. 365-387

    Eau

    No full text
    Sironneau Jacques. Eau. In: Revue Juridique de l'Environnement, n°3, 2010. pp. 513-540
    • 

    corecore