95 research outputs found

    Registration of atmospheric neutrinos with the Baikal neutrino telescope

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    We present first neutrino induced events observed with a deep underwater neutrino telescope. Data from 70 days effective life time of the BAIKAL prototype telescope NT-96 have been analyzed with two different methods. With the standard track reconstruction method, 9 clear upward muon candidates have been identified, in good agreement with 8.7 events expected from Monte Carlo calculations for atmospheric neutrinos. The second analysis is tailored to muons coming from close to the opposite zenith. It yields 4 events, compared to 3.5 from Monte Carlo expectations. From this we derive a 90 % upper flux limit of 1.1 * 10^-13 cm^-2 sec^-1 for muons in excess of those expected from atmospheric neutrinos with zenith angle > 150 degrees and energy > 10GeV.Comment: 20 pages, 11 figure

    The Baikal Deep Underwater Neutrino Experiment: Results, Status, Future

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    We review the present status of the Baikal Underwater Neutrino Experiment and present results obtained with the various stages of the stepwise increasing detector: NT-36 (1993-95), NT-72 (1995-96) and NT-96 (1996-97). Results cover atmospheric muons, first clear neutrino events, search for neutrinos from WIMP annihilation in the center of the Earth, search for magnetic monopoles, and -- far from astroparticle physics -- limnology.Comment: Talk given at the Int. School on Nuclear Physics, Erice, Sept.199

    Baikal-GVD

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    We present the status of the Gigaton Volume Detector in Lake Baikal (Baikal-GVD) designed for the detection of high energy neutrinos of astrophysical origin. The telescope consists of functionally independent clusters, sub-arrays of optical modules (OMs), which are connected to shore by individual electro-optical cables. During 2015 the GVD demonstration cluster, comprising 192 OMs, has been successfully operated in Lake Baikal. In 2016 this array was upgraded to baseline configuration of GVD cluster with 288 OMs arranged on eight vertical strings. Thus the instrumented water volume has been increased up to about 5.9 Mtons. The array was commissioned in early April 2016 and takes data since then. We describe the configuration and design of the 2016 array. Preliminary results obtained with data recorded in 2015 are also discussed

    Contacts for silicon IMPATT and pick-off diodes

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    We studied experimentally: (i) the ways to fabricate metal-n⁺-Si ohmic contacts with Schottky barriers; (ii) how elemental, structural and phase composition of barrier layers in the contact system, as well as of the barrier layer-semiconductor interface, depend on the formation techniques and conditions; (iii) their evolution at heating and under ⁶⁰Co g-radiation. Some versions of technique to form palladium, titanium, gold barrier layers using thermal and magnetron sputtering, as well as thermionic synthesis, are discussed. We investigated the structure, as well as phase and elemental composition, of both the barrier layers in contact system and barrier layer-semiconductor interface as a function of the formation techniques and conditions, and their evolution under heating and ⁶⁰Co g-radiation. For technological processes of contact system and mesa formation a simulation was performed to determine what contact systems are promising for use in manufacturing technology of silicon IMPATT and pick-off diodes for the millimeter wavelength range. Some conditions have been found that are necessary for production of high-performance contact systems. The heat and radiation tolerance ranges for barrier structures were considered. It was shown that the Si-Ti-TiB2-Au contact systems are best suited for production of silicon IMPATT and pick-off diode structures intended for the millimeter wavelength range
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