114 research outputs found

    Physics of Atomic Nuclei V. 63, I. 06

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    Physics of Atomic Nuclei -- June 2000 Volume 63, Issue 6, pp. 921-1109 NEUTRINO PHYSICS Neutrino Physics at the Turn of the Millennium J. W. F. Valle pp. 921-933 Full Text: PDF (190 kB) Update of Results from the SuperKamiokande Detector (June 1999) W. Gajewski (for the SuperKamiokande Collaboration) pp. 934-942 Full Text: PDF (135 kB) Solar-Neutrino Results from SAGE J. N. Abdurashitov et al. (for the SAGE Collaboration) pp. 943-950 Full Text: PDF (191 kB) Lake Baikal Neutrino Experiment: Selected Results V. A. Balkanov, I. A. Belolaptikov, L. B. Bezrukov, N. M. Budnev, A. G. Chensky, I. A. Danilchenko, Zh.-A. M. Dzhilkibaev, G. V. Domogatsky, A. A. Doroshenko, S. V. Fialkovsky, O. N. Gaponenko, A. A. Garus, T. I. Gress, D. Kiss, A. I. Klimov, S. I. Klimushin, A. P. Koshechkin, V. E. Kuznetzov, V. F. Kulepov, L. A. Kuzmichev, S. V. Lovzov, J. J. Laudenskaite, B. K. Lubsandorzhiev, M. B. Milenin, R. R. Mirgazov, N. I. Moseiko, V. A. Netikov, E. A. Osipova, A. I. Panfilov, Yu. V. Parfenov, A. A. Pavlov, E. N. Pliskovsky, P. G. Pokhil, E. G. Popova, M. I. Rozanov, I. A. Sokalski, Ch. Spiering, O. Streicher, B. A. Tarashansky, G. Toht, T. Thon, R. Vasiliev, R. Wischnewski, and I. V. Yashin pp. 951-961 Full Text: PDF (182 kB) Direct Search for the Neutrino Mass in the Beta Decay of Tritium: Status of the "Troitsk nu-Mass" Experiment V. M. Lobashev pp. 962-968 Full Text: PDF (110 kB) Newest Results from the Mainz Neutrino-Mass Experiment J. Bonn, B. Bornschein, L. Bornschein, L. Fickinger, O. Kazachenko, A. Kovalik, Ch. Kraus, E. W. Otten, H. Ulrich, and Ch. Weinheimer pp. 969-974 Full Text: PDF (97 kB) Nearly Mass-Degenerate Majorana Neutrinos: Double-Beta Decay and Neutrino Oscillations E. Ma pp. 975-978 Full Text: PDF (66 kB) The Precious Information from Supernova LMC-87A on the Neutrino Masses and Neutrino Mixing Angles among the Flavor States and the Mass States H. Huzita pp. 979-983 Full Text: PDF (64 kB) Solar-Neutrino Variations: A Manifestation of Nonzero Neutrino Mass and Magnetic Moment, and Mixing L. I. Dorman pp. 984-988 Full Text: PDF (111 kB) The Asymmetry of Solar-Neutrino Fluxes L. I. Dorman pp. 989-992 Full Text: PDF (72 kB) REACTORS NEUTRINOS Reactor Neutrinos—Present and Future J. Busenitz pp. 993-1001 Full Text: PDF (172 kB) REACTOR NEUTRINOS Neutrino Oscillations at Reactors: What Is Next? L. A. Mikaélyan and V. V. Sinev pp. 1002-1006 Full Text: PDF (73 kB) ORLaND: A Proposed Neutrino Facility at the Oak Ridge National Laboratory F. T. Avignone III, B. D. Anderso, T. C. Awes, S. Berridge, W. Bilpuch, C. Britton, W. Bryan, W. M. Bugg, R. L. Burman, J. Busenitz, K. Carter, L. Chatterjee, V. Cianciolo, A. K. Cochran, H. O. Cohn, M. V. Danilov, L. De-Brackeleer, P. Degtiarenko, Yu. V. Efremenko, M. A. Elaasar, A. R. Fazely, S. Frank, T. A. Gabriel, C. R. Gould, V. Gudkov, R. Gunasingha, T. Handler, E. L. Hart, R. L. Imlay, U. Jagadish, Yu. A. Kamyshkov, E. Khosrovi, D. D. Koetke, C. Lane, R. W. Manweiler, W. J. Metcalf, A. Mezzacappa, L. W. Mo, V. Z. Nosik, T. A. Nummaker, S. Nussinov, A. Piepke, F. Plasil, J. Reidy, C. Rosenfeld, D. Smith, I. Stancu, T. D. S. Stanislaus, R. Steinberg, R. Svoboda, R. Tashakkori, W. Tornow, G. Van Dalen, J. Walker, J. W. Watson, A. Wintenberg, J. Wolf , D. H. Wright, O. Ya. Zeldovich, and W.-M. Zhang pp. 1007-1011 Full Text: PDF (86 kB) Search for the Neutrino Magnetic Moment in the Nonequilibrium Reactor-Antineutrino Energy Spectrum V. I. Kopeikin, L. A. Mikaélyan, and V. V. Sinev pp. 1012-1015 Full Text: PDF (80 kB) Antineutrino–Deuteron Experiment at the Krasnoyarsk Reactor Yu. V. Kozlov, S. V. Khaltourtcev, I. N. Machulin, A. V. Martemyanov, V. P. Martemyanov, S. V. Sukhotin, V. G. Tarasenkov, E. V. Turbin, and V. N. Vyrodov pp. 1016-1019 Full Text: PDF (73 kB) ASTROPARTICLE PHYSICS AND COSMOLOGY Physically Self-Consistent Basis for Modern Cosmology M. Yu. Khlopov pp. 1020-1028 Full Text: PDF (96 kB) Some Recent Developments in SUSY Dark Matter Analyses P. Nath pp. 1029-1036 Full Text: PDF (101 kB) In Searches for Daemons E. M. Drobyshevski pp. 1037-1041 Full Text: PDF (71 kB) Possible Evidence for the Observation of Noncompact (Nonbaryonic) Gravitational Microlenses ("Neutralino Stars") A. F. Zakharov pp. 1042-1045 Full Text: PDF (65 kB) Magnetic-Field Influence on Radiative Axion Decay into Photons of the Same Polarization N. V. Mikheev, A. Ya. Parkhomenko, and L. A. Vassilevskaya pp. 1046-1049 Full Text: PDF (68 kB) On Charm Production at High Energies L. V. Volkova and G. T. Zatsepin pp. 1050-1052 Full Text: PDF (46 kB) About the Character of the "Knee" at E ~= 3 × 1015 eV in the Energy Spectrum and the Mass Composition of Primary Cosmic Rays in the Energy Range 1015–1017 eV Yu. F. Novosel'tsev pp. 1053-1057 Full Text: PDF (71 kB) PHYSICS BEYOND THE STANDARD MODEL The Link between Neutrino Masses and Proton Decay in Supersymmetric Unification J. C. Pati pp. 1058-1077 Full Text: PDF (264 kB) Neutrino Masses Originating from SUSY R-Parity-Violating Terms with U(1) Flavor Symmetry O. Haug, J. D. Vergados, A. Faessler, and S. G. Kovalenko pp. 1078-1082 Full Text: PDF (77 kB) Neutrino Oscillations from Supersymmetry without R-Parity—Its Implications on the Flavor Structure of the Theory O. C. W. Kong pp. 1083-1087 Full Text: PDF (76 kB) Search for Quantum Spacetime Foam D. V. Nanopoulos pp. 1088-1096 Full Text: PDF (128 kB) Possible Spontaneous Breaking of Lorentz and CPT Symmetry D. Colladay pp. 1097-1102 Full Text: PDF (81 kB) NEUTRINO PHYSICS AT ACCELERATORS Perspectives for Neutrino Physics at CERN A. Guglielmi pp. 1103-1109 Full Text: PDF (128 kB)Archived web conten

    Limits on the high-energy gamma and neutrino fluxes from the SGR 1806-20 giant flare of 27 December 2004 with the AMANDA-II detector.

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    On 27 December 2004, a giant gamma flare from the Soft Gamma-Ray Repeater 1806-20 saturated many satellite gamma-ray detectors, being the brightest transient event ever observed in the Galaxy. AMANDA-II was used to search for down-going muons indicative of high-energy gammas and/or neutrinos from this object. The data revealed no significant signal, so upper limits (at 90% C.L.) on the normalization constant were set: 0.05(0.5) TeV-1 m;{-2} s;{-1} for gamma=-1.47 (-2) in the gamma flux and 0.4(6.1) TeV-1 m;{-2} s;{-1} for gamma=-1.47 (-2) in the high-energy neutrino flux

    Measurement of sound speed vs. depth in South Pole ice for neutrino astronomy

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    We have measured the speed of both pressure waves and shear waves as a function of depth between 80 and 500 m depth in South Pole ice with better than 1% precision. The measurements were made using the South Pole Acoustic Test Setup (SPATS), an array of transmitters and sensors deployed in the ice at the South Pole in order to measure the acoustic properties relevant to acoustic detection of astrophysical neutrinos. The transmitters and sensors use piezoceramics operating at ∼5-25 kHz. Between 200 m and 500 m depth, the measured profile is consistent with zero variation of the sound speed with depth, resulting in zero refraction, for both pressure and shear waves. We also performed a complementary study featuring an explosive signal propagating vertically from 50 to 2250 m depth, from which we determined a value for the pressure wave speed consistent with that determined for shallower depths, higher frequencies, and horizontal propagation with the SPATS sensors. The sound speed profile presented here can be used to achieve good acoustic source position and emission time reconstruction in general, and neutrino direction and energy reconstruction in particular. The reconstructed quantities could also help separate neutrino signals from background. © 2010 Elsevier B.V. All rights reserved.0SCOPUS: ar.jinfo:eu-repo/semantics/publishe

    Physics of Atomic Nuclei V. 68, I. 07

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    Physics of Atomic Nuclei -- July 2005 Volume 68, Issue 7, pp. 1079-1262 NUCLEI Experiment Alpha-Cluster States in 18O V. Z. Goldberg, K.-M. Källman, T. Lönnroth, P. Manngård, and B. B. Skorodumov pp. 1079-1086 Full Text: PDF (292 kB) Jpi = 0– Levels in 156Gd and 158Gd E. P. Grigoriev pp. 1087-1095 Full Text: PDF (216 kB) Cold-Neutron Storage Owing to Diffusion Reflection S. S. Arzumanov, L. N. Bondarenko, P. Geltenbort, V. I. Morozov, and Yu. N. Panin pp. 1096-1100 Full Text: PDF (215 kB) Analysis of the Phase Tunneling Time for Cold Neutrons through a Neutron Interference Filter A. K. Zaichenko and V. S. Olkhovsky pp. 1101-1103 Full Text: PDF (106 kB) Dynamic Reflection and Refraction of Neutrons at the Boundaries of Matter Characterized by a Variable Magnetic Induction A. V. Kozlov and A. I. Frank pp. 1104-1119 Full Text: PDF (311 kB) Theory Puzzle of the 6Li Quadrupole Moment: Steps toward Solving It L. D. Blokhintsev, V. I. Kukulin, and V. N. Pomerantsev pp. 1120-1132 Full Text: PDF (295 kB) Magic Numbers of Ultraheavy Nuclei V. Yu. Denisov pp. 1133-1137 Full Text: PDF (230 kB) Effect of Synchrotron Radiation on Nuclear Beta Decay I. V. Kopytin and K. N. Karelin pp. 1138-1146 Full Text: PDF (242 kB) Nature of Coulomb Shifts of Nuclear Scattering Resonances N. Zh. Takibayev pp. 1147-1152 Full Text: PDF (152 kB) The Examination of the 12C + 24Mg Elastic Scattering around the Coulomb Barrier I. Boztosun, Y. Dagdemir, and O. Bayrak pp. 1153-1159 Full Text: PDF (227 kB) ELEMENTARY PARTICLES AND FIELDS Experiment A Study of the Nuclear-Medium Influence on Transverse Momentum of Hadrons Produced in Deep-Inelastic Neutrino Scattering N. M. Agababyan, V. V. Ammosov, M. Atayan, N. Grigoryan, H. Gulkanyan, A. A. Ivanilov, Zh. Karamyan, and V. A. Korotkov pp. 1160-1170 Full Text: PDF (303 kB) Backscattered Flux Generated by Protons with Energy above 1 TeV in a Lead Absorber D. M. Podorozhnyi, I. D. Rapoport, and A. N. Turundaevsky pp. 1171-1175 Full Text: PDF (141 kB) Albedo in the ATIC Experiment: Measurements and Simulations N. V. Sokolskaya, J. H. Adams, Jr., H. S. Ahn, K. E. Batkov, G. L. Bashindzhagyan, J. Z. Wang, J. P. Wefel, J. Wu, O. Ganel, T. G. Guzik, R. M. Gunasingha, V. I. Zatsepin, J. Isbert, K. C. Kim, M. Christl, E. N. Kouznetsov, M. I. Panasyuk, A. D. Panov, E. S. Seo, A. R. Fazely, J. Chang, and W. K. H. Schmidt pp. 1176-1182 Full Text: PDF (199 kB) Theory Some Features of the Production of Heavy-Quark-Containing Baryons in Electron-Positron Collisions S. P. Baranov and V. L. Slad pp. 1183-1189 Full Text: PDF (237 kB) Is It Still Interesting to Search for Lepton-Flavor Violation in Rare Kaon Decays? L. G. Landsberg pp. 1190-1210 Full Text: PDF (388 kB) Pion Electromagnetic Form Factor in QCD Sum Rules V. V. Braguta and A. I. Onishchenko pp. 1211-1217 Full Text: PDF (167 kB) On the Stability of a Self-Similar Spherical Bubble of a Scalar Higgs Field in de Sitter Space N. A. Voronov, A. L. Dyshko, and N. B. Konyukhova pp. 1218-1226 Full Text: PDF (226 kB) Quasilinearization Method: Nonperturbative Approach to Physical Problems V. B. Mandelzweig pp. 1227-1258 Full Text: PDF (505 kB) LETTERS TO THE EDITOR Quadrupole Moments and Transition Probabilities B(E2) for Light Nuclei in the Orthogonal-Scheme Basis with Symmetric Representations of the O(A – 1) Group K. J. Yankauskas and A. K. Petrauskas pp. 1259-1260 Full Text: PDF (92 kB) FUTURE PUBLICATIONS Future Publications pp. 1261-1262 Full Text: PDF (74 kB)Archived web conten

    Health education and the control of intestinal worm infections in China : a new vision

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    The transmission of soil-transmitted helminths (STHs) is associated with poverty, poor hygiene behaviour, lack of clean water and inadequate waste disposal and sanitation. Periodic administration of benzimidazole drugs is the mainstay for global STH control but it does not prevent re-infection, and is unlikely to interrupt transmission as a stand-alone intervention.; We reported recently on the development and successful testing in Hunan province, PR China, of a health education package to prevent STH infections in Han Chinese primary school students. We have recently commenced a new trial of the package in the ethnically diverse Xishuangbanna autonomous prefecture in Yunnan province and the approach is also being tested in West Africa, with further expansion into the Philippines in 2015.; The work in China illustrates well the direct impact that health education can have in improving knowledge and awareness, and in changing hygiene behaviour. Further, it can provide insight into the public health outcomes of a multi-component integrated control program, where health education prevents re-infection and periodic drug treatment reduces prevalence and morbidity

    First year performance of the IceCube neutrino telescope

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    The first sensors of the IceCube neutrino observatory were deployed at the South Pole during the austral summer of 2004-2005 and have been producing data since February 2005. One string of 60 sensors buried in the ice and a surface array of eight ice Cherenkov tanks took data until December 2005 when deployment of the next set of strings and tanks began. We have analyzed these data, demonstrating that the performance of the system meets or exceeds design requirements. Times are determined across the whole array to a relative precision of better than 3 ns, allowing reconstruction of muon tracks and light bursts in the ice, of air-showers in the surface array and of events seen in coincidence by surface and deep-ice detectors separated by up to 2.5 km. (c) 2006 Elsevier B.V. All rights reserved

    Association between footwear use and neglected tropical diseases : a systematic review and meta-analysis

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    BACKGROUND: The control of neglected tropical diseases (NTDs) has primarily focused on preventive chemotherapy and case management. Less attention has been placed on the role of ensuring access to adequate water, sanitation, and hygiene and personal preventive measures in reducing exposure to infection. Our aim was to assess whether footwear use was associated with a lower risk of selected NTDs. METHODOLOGY: We conducted a systematic review and meta-analysis to assess the association between footwear use and infection or disease for those NTDs for which the route of transmission or occurrence may be through the feet. We included Buruli ulcer, cutaneous larva migrans (CLM), leptospirosis, mycetoma, myiasis, podoconiosis, snakebite, tungiasis, and soil-transmitted helminth (STH) infections, particularly hookworm infection and strongyloidiasis. We searched Medline, Embase, Cochrane, Web of Science, CINAHL Plus, and Popline databases, contacted experts, and hand-searched reference lists for eligible studies. The search was conducted in English without language, publication status, or date restrictions up to January 2014. Studies were eligible for inclusion if they reported a measure of the association between footwear use and the risk of each NTD. Publication bias was assessed using funnel plots. Descriptive study characteristics and methodological quality of the included studies were summarized. For each study outcome, both outcome and exposure data were abstracted and crude and adjusted effect estimates presented. Individual and summary odds ratio (OR) estimates and corresponding 95% confidence intervals (CIs) were calculated as a measure of intervention effect, using random effects meta-analyses. PRINCIPAL FINDINGS: Among the 427 studies screened, 53 met our inclusion criteria. Footwear use was significantly associated with a lower odds of infection of Buruli ulcer (OR = 0.15; 95% CI: 0.08-0.29), CLM (OR = 0.24; 95% CI: 0.06-0.96), tungiasis (OR = 0.42; 95% CI 0.26-0.70), hookworm infection (OR = 0.48; 95% CI: 0.37-0.61), any STH infection (OR = 0.57; 95% CI: 0.39-0.84), strongyloidiasis (OR = 0.56; 95% CI: 0.38-0.83), and leptospirosis (OR = 0.59; 95% CI: 0.37-0.94). No significant association between footwear use and podoconiosis (OR = 0.63; 95% CI: 0.38-1.05) was found and no data were available for mycetoma, myiasis, and snakebite. The main limitations were evidence of heterogeneity and poor study quality inherent to the observational studies included. CONCLUSIONS/SIGNIFICANCE: Our results show that footwear use was associated with a lower odds of several different NTDs. Access to footwear should be prioritized alongside existing NTD interventions to ensure a lasting reduction of multiple NTDs and to accelerate their control and elimination

    Sensitivity of the IceCube detector to astrophysical sources of high energy muon neutrinos

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    We present results of a Monte Carlo study of the sensitivity of the planned IceCube detector to predicted fluxes of muon neutrinos at TeV to PeV energies. A complete simulation of the detector and data analysis is used to study the detector's capability to search for muon neutrinos from potential sources such as active galaxies and gamma-ray bursts (GRBs). We study the effective area and the angular resolution of the detector as a function of muon energy and angle of incidence. We present detailed calculations of the sensitivity of the detector to both diffuse and pointlike neutrino fluxes, including an assessment of the sensitivity to neutrinos detected in coincidence with GRB observations. After three years of data taking, IceCube will be able to detect a point-source flux of Eν2× dNν/dEν=7×10-9 cm-2s-1 GeV at a 5σ significance, or, in the absence of a signal, place a 90% c.l. limit at a level of Eν2×dNν/dEν= 2×10-9 cm-2 s-1 GeV. A diffuse E-2 flux would be detectable at a minimum strength of Eν2×dNν/dEν =10-8 cm-2-1 sr-1 GeV. A GRB model following the formulation of Waxman and Bahcall would result in a 5σ effect after the observation of 200 bursts in coincidence with satellite observations of the gamma rays. © 2003 Elsevier B.V. All rights reserved.0SCOPUS: ar.jinfo:eu-repo/semantics/publishe
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