199 research outputs found

    Financial development and economic growth in China

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    The purpose of this paper is to examine the relationship between financial development and economic growth. In particular, the authors examine the impact of financial development on the growth of primary, secondary, and tertiary industries in China. Ordinary Least Square (OLS) multiple regressions are applied on a set of data from China for the period 1978 to 2013 to determine the effects of financial development on economic growth, while controlling for other macroeconomic variables, namely labor force, capital growth, inflation rate and export growth. The empirical results show that financial development has a negative effect on economic growth in general, but on the growth of the tertiary industry in particular. By contrast, it is found that financial development has no significant effect on the primary and secondary industries. The findings offer policymakers some useful insights that more attention may need to be paid on developing capital markets and providing more investment choices/opportunities for Chinese households. This paper is different from most of the previous studies as it uses up-to-date data (1978-2013) from China capturing the effects of financial development on economic growth in addition to other macroeconomic factors

    Corporate governance disclosure index-executive pay nexus: the moderating effect of governance mechanisms

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    This paper first employs principal component analysis technique to develop and introduce an alternative UK corporate governance disclosure index to the US‐centric ones. Second, we then investigate whether this new corporate governance disclosure index can determine the level of executive pay (including CEOs, CFOs, and all executive directors) in UK listed firms, and consequently ascertain whether the governance mechanisms can moderate the pay‐for‐performance sensitivity. Employing data on corporate governance, executive pay and performance from 2008 to 2013, we find that, on average, better‐governed firms tend to pay their executives lower compared with their poorly‐governed counterparts. Additionally, our findings suggest that the pay‐for‐performance sensitivity is generally positive, but improves in firms with high corporate governance quality, implying that the pay‐for‐performance sensitivity is contingent on the quality of internal governance structures. We interpret our findings within the predictions of optimal contracting theory and managerial power hypothesis

    Detecting a stochastic gravitational wave background with the Laser Interferometer Space Antenna

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    The random superposition of many weak sources will produce a stochastic background of gravitational waves that may dominate the response of the LISA (Laser Interferometer Space Antenna) gravitational wave observatory. Unless something can be done to distinguish between a stochastic background and detector noise, the two will combine to form an effective noise floor for the detector. Two methods have been proposed to solve this problem. The first is to cross-correlate the output of two independent interferometers. The second is an ingenious scheme for monitoring the instrument noise by operating LISA as a Sagnac interferometer. Here we derive the optimal orbital alignment for cross-correlating a pair of LISA detectors, and provide the first analytic derivation of the Sagnac sensitivity curve.Comment: 9 pages, 11 figures. Significant changes to the noise estimate

    Calibration and Characterization of the IceCube Photomultiplier Tube

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    Over 5,000 PMTs are being deployed at the South Pole to compose the IceCube neutrino observatory. Many are placed deep in the ice to detect Cherenkov light emitted by the products of high-energy neutrino interactions, and others are frozen into tanks on the surface to detect particles from atmospheric cosmic ray showers. IceCube is using the 10-inch diameter R7081-02 made by Hamamatsu Photonics. This paper describes the laboratory characterization and calibration of these PMTs before deployment. PMTs were illuminated with pulses ranging from single photons to saturation level. Parameterizations are given for the single photoelectron charge spectrum and the saturation behavior. Time resolution, late pulses and afterpulses are characterized. Because the PMTs are relatively large, the cathode sensitivity uniformity was measured. The absolute photon detection efficiency was calibrated using Rayleigh-scattered photons from a nitrogen laser. Measured characteristics are discussed in the context of their relevance to IceCube event reconstruction and simulation efforts.Comment: 40 pages, 12 figure

    All-particle cosmic ray energy spectrum measured with 26 IceTop stations

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    We report on a measurement of the cosmic ray energy spectrum with the IceTop air shower array, the surface component of the IceCube Neutrino Observatory at the South Pole. The data used in this analysis were taken between June and October, 2007, with 26 surface stations operational at that time, corresponding to about one third of the final array. The fiducial area used in this analysis was 0.122 km^2. The analysis investigated the energy spectrum from 1 to 100 PeV measured for three different zenith angle ranges between 0{\deg} and 46{\deg}. Because of the isotropy of cosmic rays in this energy range the spectra from all zenith angle intervals have to agree. The cosmic-ray energy spectrum was determined under different assumptions on the primary mass composition. Good agreement of spectra in the three zenith angle ranges was found for the assumption of pure proton and a simple two-component model. For zenith angles {\theta} < 30{\deg}, where the mass dependence is smallest, the knee in the cosmic ray energy spectrum was observed between 3.5 and 4.32 PeV, depending on composition assumption. Spectral indices above the knee range from -3.08 to -3.11 depending on primary mass composition assumption. Moreover, an indication of a flattening of the spectrum above 22 PeV were observed.Comment: 38 pages, 17 figure

    An improved method for measuring muon energy using the truncated mean of dE/dx

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    The measurement of muon energy is critical for many analyses in large Cherenkov detectors, particularly those that involve separating extraterrestrial neutrinos from the atmospheric neutrino background. Muon energy has traditionally been determined by measuring the specific energy loss (dE/dx) along the muon's path and relating the dE/dx to the muon energy. Because high-energy muons (E_mu > 1 TeV) lose energy randomly, the spread in dE/dx values is quite large, leading to a typical energy resolution of 0.29 in log10(E_mu) for a muon observed over a 1 km path length in the IceCube detector. In this paper, we present an improved method that uses a truncated mean and other techniques to determine the muon energy. The muon track is divided into separate segments with individual dE/dx values. The elimination of segments with the highest dE/dx results in an overall dE/dx that is more closely correlated to the muon energy. This method results in an energy resolution of 0.22 in log10(E_mu), which gives a 26% improvement. This technique is applicable to any large water or ice detector and potentially to large scintillator or liquid argon detectors.Comment: 12 pages, 16 figure
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