47 research outputs found

    Constraints on neutrino oscillation parameters from the measurement of day-night solar neutrino fluxes at Super-Kamiokande

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    A search for day-night variations in the solar neutrino flux resulting from neutrino oscillations has been carried out using the 504 day sample of solar neutrino data obtained at Super-Kamiokande. The absence of a significant day-night variation has set an absolute flux independent exclusion region in the two neutrino oscillation parameter space.Comment: 11 pages, 3 figures, submitted to PRL, single-spacin

    The ATLAS Trigger/DAQ Authorlist, version 1.0

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    This is a reference document giving the ATLAS Trigger/DAQ author list, version 1.0 of 20 Nov 2008

    The ATLAS Trigger/DAQ Authorlist, version 2.0

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    This is the ATLAS Trigger/DAQ Authorlist, version 2.0, 31 July 200

    The ATLAS Trigger/DAQ Authorlist, version 3.0

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    This is the ATLAS Trigger/DAQ Authorlist, version 3.0, 11 September 200

    The ATLAS Trigger/DAQ Authorlist, version 3.1

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    This is the ATLAS Trigger/DAQ Authorlist, version 3.1, 17 September 200

    Role of Spin-Orbit Coupling and Hybridization Effects in the Electronic Structure of Ultrathin Bi Films

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    The electronic structure of Bi(001) ultrathin films (thickness >= 7 bilayers) on Si(111)-7x7 was studied by angle-resolved photoemission spectroscopy and first-principles calculations. In contrast with the semimetallic nature of bulk Bi, both the experiment and theory demonstrate the metallic character of the films with the Fermi surface formed by spin-orbit-split surface states (SSs) showing little thickness dependence. Below the Fermi level, we clearly detected quantum well states (QWSs) at the M ()overbarpoint,whichweresurprisinglyfoundtobenon−spin−orbitsplit;thefilmsare"electronicallysymmetric"despitetheobviousstructuralnonequivalenceofthetopandbottominterfaces.WefoundthattheSSshybridizewiththeQWSsnearM() over bar point, which were surprisingly found to be non-spin-orbit split; the films are "electronically symmetric" despite the obvious structural nonequivalence of the top and bottom interfaces. We found that the SSs hybridize with the QWSs near M () over bar and lose their spin-orbit-split character
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