3,326 research outputs found

    Study of a Threshold Cherenkov Counter Based on Silica Aerogels with Low Refractive Indices

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    To identify π±\pi^{\pm} and K±K^{\pm} in the region of 1.02.51.0\sim 2.5 GeV/c, a threshold Cherenkov counter equipped with silica aerogels has been investigated. Silica aerogels with a low refractive index of 1.013 have been successfully produced using a new technique. By making use of these aerogels as radiators, we have constructed a Cherenkov counter and have checked its properties in a test beam. The obtained results have demonstrated that our aerogel was transparent enough to make up for loss of the Cherenkov photon yield due to a low refractive index. Various configurations for the photon collection system and some types of photomultipliers, such as the fine-mesh type, for a read out were also tested. From these studies, our design of a Cherenkov counter dedicated to π/K\pi / K separation up to a few GeV/c %in the momentum range of 1.02.51.0 \sim 2.5 GeV/c with an efficiency greater than 9090 \% was considered.Comment: 21 pages, latex format (article), figures included, to be published in Nucl. Instrm. Meth.

    Development of a Large-Area Aerogel Cherenkov Counter Onboard BESS

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    This paper describes the development of a threshold type aerogel Cherenkov counter with a large sensitive area of 0.6 m2^2 to be carried onboard the BESS rigidity spectrometer to detect cosmic-ray antiprotons. The design incorporates a large diffusion box containing 46 finemesh photomultipliers, with special attention being paid to achieving good performance under a magnetic field and providing sufficient endurance while minimizing material usage. The refractive index of the aerogel was chosen to be 1.03. By utilizing the muons and protons accumulated during the cosmic-ray measurements at sea level, a rejection factor of 104^4 was obtained against muons with β1\beta \approx 1, while keeping 97% efficiency for protons below the threshold.Comment: 13 pages, LaTex, 9 eps figures included, submitted to NIM

    The monitoring system for the aerogel Cherenkov counter of the BELLE detector

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    We report on a design and performances of a monitoring system developed for the aerogel Cherenkov counters (ACC) of the BELLE detector. The system consists of blue LEDs, a diffuser box, and optical distributors which distribute the LED light to the ACC modules. The employed LED (NSPB series) has been observed to have high reliability on the long term stability and the temprature dependence. The diffuser box is employed to reduce the intrinsic non-uniformity of the LED light intensity. The overall performances of the present monitoring system on uniformity and intensity of the light output have been found to satisfy all the requirements for the monitoring.Comment: 24 pages, LaTeX, 13 eps figures, to be published in Nucl. Instrum. and Meth. A. Postscript file (4.5 MB) is available at http://www-hep.phys.saga-u.ac.jp/~murakami/paper/xxx_accmon.p

    Emission spectra of Cs-He excimers in cold helium gas

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    Psychological factors associated with pain 24 hours post-tooth extraction

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    Background: There is a considerable variation in dental patients’ post-operative pain experience and analgesic requirements following identical surgical procedures. This has been related to a variety of psychological factors. Pain is one of the most commonly cited factors that is strongly associated with dental fear. Surgical removal of a third molar, the most common procedure in oral surgery and generally associated with dread, has received limited research attention. It is, therefore, essential to understand factors likely to influence the pain experience of patients in such a stressful setting. Such an understanding will not only help patients cope with fear and pain, but also will assist clinicians create a less stressful environment. This study investigated psychological factors predicting heightened pain perception in tooth extraction: dental anxiety; dental control; pain catastrophizing; expectation of pain; social desirability (defensiveness); trait anxiety and monitor-blunter style coping. Methods: The sample consisted of 306 participants (144 male and 162 female aged between 18 and 62 years with the mean age of 31.82) who were referred by their local dental practitioners for the surgical removal of tooth/teeth under local anaesthetic at the unit of Oral and Maxillofacial surgery at UCL Eastman Dental Institute. The tooth/teeth which needed extraction were not limited to the third molars. The variables were measured at four different time points: on recruitment (baseline: T0), before (T1), after (T2) and the following day (T3) of the dental surgery. The variables assessed were: dental anxiety; dental control; pain catastrophizing; social desirability; trait anxiety; monitor-blunter style coping; sensory intensity of pain, affective quality of pain, state anxiety and mood states. After the surgery, the dental surgeons rated the complexity of the surgical procedure and the perception of their patients’ distress levels. 7 Results: It was found that pain 24 hours post-tooth extraction was best predicted by the levels of expected sensory pain together with post-surgery state anxiety, trait anxiety and expected affective pain. Expected sensory pain, in turn, was predicted by dental anxiety, monitoring and felt (perceived) control (i.e., the dental pain predictors). Moreover, dental anxiety was found to be a precursor to all the dental pain predictors. Furthermore, pain catastrophizing did not make to the primary dental pain predictors. Nevertheless, it contributed to heightened levels of trait anxiety and expected affective pain which sequentially helped to intensify perception of dental pain. In addition, it was revealed that dental surgeons underevaluated their patients’ treatment pain

    K0(K0ˉ)K^0(\bar{K^0}) Production in Two-Photon Processes at TRISTAN

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    We have carried out an inclusive measurement of K0(K0ˉ)K^0(\bar{K^0}) production in two-photon processes at TRISTAN. The mean s\sqrt{s} was 58 GeV and the integrated luminosity was 199 pb1^{-1}. High-statistics KsK_s samples were obtained under such conditions as no-, anti-electron, and remnant-jet tags. The remnant-jet tag, in particular, allowed us, for the first time, to measure the cross sections separately for the resolved-photon and direct processes.Comment: 20 pages, Latex format, 4 figures and KEK-mark included. Table 1 revised. To be published in Phys. Lett.

    Reactor Neutrino Experiments with a Large Liquid Scintillator Detector

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    We discuss several new ideas for reactor neutrino oscillation experiments with a Large Liquid Scintillator Detector. We consider two different scenarios for a measurement of the small mixing angle θ13\theta_{13} with a mobile νˉe\bar{\nu}_e source: a nuclear-powered ship, such as a submarine or an icebreaker, and a land-based scenario with a mobile reactor. The former setup can achieve a sensitivity to sin22θ130.003\sin^2 2\theta_{13} \lesssim 0.003 at the 90% confidence level, while the latter performs only slightly better than Double Chooz. Furthermore, we study the precision that can be achieved for the solar parameters, sin22θ12\sin^2 2\theta_{12} and Δm212\Delta m_{21}^2, with a mobile reactor and with a conventional power station. With the mobile reactor, a precision slightly better than from current global fit data is possible, while with a power reactor, the accuracy can be reduced to less than 1%. Such a precision is crucial for testing theoretical models, e.g. quark-lepton complementarity.Comment: 18 pages, 3 figures, 2 tables, revised version, to appear in JHEP, Fig. 1 extended, Formula added, minor changes, results unchange

    Calculated Electron Fluxes at Airplane Altitudes

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    A precision measurement of atmospheric electron fluxes has been performed on a Japanese commercial airliner (Enomoto, {\it et al.}, 1991). We have performed a monte carlo calculation of the cosmic ray secondary electron fluxes expected in this experiment. The monte carlo uses the hadronic portion of our neutrino flux cascade program combined with the electromagnetic cascade portion of the CERN library program GEANT. Our results give good agreement with the data, provided we boost the overall normalization of the primary cosmic ray flux by 12\% over the normalization used in the neutrino flux calculation.Comment: in REVTEX, 12 pages + 4 figures available upon reques
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