Search Results - "Tiedt, D.R."

Radiogenic and muon-induced backgrounds in the LUX dark matter detector by Akerib, D.S., Araújo, H.M., Bai, X., Bailey, A.J., Balajthy, J., Bernard, E., Bernstein, A., Bradley, A., Byram, D., Cahn, S.B., Carmona-Benitez, M.C., Chan, C., Chapman, J.J., Chiller, A.A., Chiller, C., Coffey, T., Currie, A., de Viveiros, L., Dobi, A., Dobson, J., Druszkiewicz, E., Edwards, B., Faham, C.H., Fiorucci, S., Flores, C., Gaitskell, R.J., Gehman, V.M., Ghag, C., Gibson, K.R., Gilchriese, M.G.D., Hall, C., Hertel, S.A., Horn, M., Huang, D.Q., Ihm, M., Jacobsen, R.G., Kazkaz, K., Knoche, R., Larsen, N.A., Lee, C., Lindote, A., Lopes, M.I., Malling, D.C., Mannino, R., McKinsey, D.N., Mei, D.-M., Mock, J., Moongweluwan, M., Morad, J., Murphy, A.St.J., Nehrkorn, C., Nelson, H., Neves, F., Ott, R.A., Pangilinan, M., Parker, P.D., Pease, E.K., Pech, K., Phelps, P., Reichhart, L., Shutt, T., Silva, C., Solovov, V.N., Sorensen, P., O’Sullivan, K., Sumner, T.J., Szydagis, M., Taylor, D., Tennyson, B., Tiedt, D.R., Tripathi, M., Uvarov, S., Verbus, J.R., Walsh, N., Webb, R., White, J.T., Witherell, M.S., Wolfs, F.L.H., Woods, M., Zhang, C.

“…The Large Underground Xenon (LUX) dark matter experiment aims to detect rare low-energy interactions from Weakly Interacting Massive Particles (WIMPs). The…”
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LUX trigger efficiency by Akerib, D.S., Alsum, S., Araújo, H.M., Bai, X., Balajthy, J., Beltrame, P., Bernard, E.P., Bernstein, A., Biesiadzinski, T.P., Boulton, E.M., B. Boxer, Brás, P., S. Burdin, Byram, D., Carmona-Benitez, M.C., Chan, C., Cutter, J.E., Davison, T.J.R., Druszkiewicz, E., Fallon, S.R., Fan, A., Fiorucci, S., Gaitskell, R.J., Genovesi, J., Ghag, C., Gilchriese, M.G.D., E. Grace, C. Gwilliam, Hall, C.R., Haselschwardt, S.J., Hertel, S.A., Hogan, D.P., Horn, M., Huang, D.Q., Ignarra, C.M., Jacobsen, R.G., Ji, W., Kamdin, K., Kazkaz, K., Khaitan, D., Knoche, R., E.V. Korolkova, S. Kravitz, V.A. Kudryavtsev, Lenardo, B.G., Lesko, K.T., Liao, J., J. Lin, Lindote, A., Lopes, M.I., Manalaysay, A., Mannino, R.L., Marangou, N., Marzioni, M.F., McKinsey, D.N., Mei, D.-M., Moongweluwan, M., Morad, J.A., Murphy, A.St.J., Nehrkorn, C., Nelson, H.N., Neves, F., Oliver-Mallory, K.C., Palladino, K.J., Pease, E.K., G. Rischbieter, Rhyne, C., P. Rossiter, Shaw, S., Shutt, T.A., Silva, C., Solmaz, M., Solovov, V.N., Sorensen, P., Sumner, T.J., Szydagis, M., Taylor, D.J., Taylor, W.C., Tennyson, B.P., Terman, P.A., Tiedt, D.R., To, W.H., Tripathi, M., Tvrznikova, L., Utku, U., Uvarov, S., Velan, V., Verbus, J.R., Webb, R.C., White, J.T., Whitis, T.J., Witherell, M.S., Wolfs, F.L.H., D. Woodward, Xu, J., Yazdani, K., Zhang, C.

“…The Large Underground Xenon experiment (LUX) searches for dark matter using a dual-phase xenon detector. LUX uses a custom-developed trigger system for event…”
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Results from the LUX dark matter experiment by Horn, Markus, Akerib, D.S, Araújo, H.M., Bai, X., Bailey, A.J., Balajthy, J., Bernard, E., Bernstein, A., Bradley, A., Byram, D., Cahn, S.B., Carmona-Benitez, M.C., Chan, C., Chapman, J.J., Chiller, A.A., Chiller, C., Currie, A., de Viveiros, L., Dobi, A., Dobson, J., Druszkiewicz, E., Edwards, B., Faham, C.H., Fiorucci, S., Flores, C., Gaitskell, R.J., Gehman, V.M., Ghag, C., Gibson, K.R., Gilchriese, M.G.D., Hall, C., Hanhardt, M., Haselschwardt, S., Hertel, S.A., Huang, D.Q., Ihm, M., Jacobsen, R.G., Kazkaz, K., Knoche, R., Larsen, N.A., Lee, C., Lenardo, B., Lesko, K.T., Lindote, A., Lopes, M.I., Malling, D.C., Mannino, R., McKinsey, D.N., Mei, D.-M., Mock, J., Moongweluwan, M., Morad, J., Murphy, A.St.J., Nehrkorn, C., Nelson, H., Neves, F., Ott, R.A., Pangilinan, M., Parker, P.D., Pease, E.K., Pech, K., Phelps, P., Reichhart, L., Shutt, T., Silva, C., Solovov, V.N., Sorensen, P., O׳Sullivan, K., Sumner, T.J., Szydagis, M., Taylor, D., Tennyson, B., Tiedt, D.R., Tripathi, M., Uvarov, S., Verbus, J.R., Walsh, N., Webb, R., White, J.T., Witherell, M.S., Wolfs, F.L.H., Woods, M., Zhang, C.

“…The LUX (Large Underground Xenon) experiment aims at the direct detection of dark matter particles via their collisions with xenon nuclei. The 370kg two-phase…”
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First Results of the LUX Dark Matter Experiment by Carmona-Benitez, M.C., Akerib, D.S., Araújo, H.M., Bai, X., Bailey, A.J., Balajthy, J., Beltrame, P., Bernard, E., Bernstein, A., Bradley, A., Byram, D., Cahn, S.B., Chan, C., Chapman, J.J., Chiller, A.A., Chiller, C., Currie, A., de Viveiros, L., Dobi, A., Dobson, J., Druszkiewicz, E., Edwards, B., Faham, C.H., Fiorucci, S., Flores, C., Gaitskell, R.J., Gehman, V.M., Ghag, C., Gibson, K.R., Gilchriese, M.G.D., Hall, C., Hanhardt, M., Haselschwardt, S., Hertel, S.A., Horn, M., Huang, D.Q., Ihm, M., Jacobsen, R.G., Kazkaz, K., Knoche, R., Larsen, N.A., Lee, C., Lenardo, B., Lesko, K.T., Lindote, A., Lopes, M.I., Malling, D.C., Manalaysay, A., Mannino, R., McKinsey, D.N., Mei, D.-M., Mock, J., Moongweluwan, M., Morad, J., Murphy, A.St.J., Nehrkorn, C., Nelson, H., Neves, F., Ott, R.A., Pangilinan, M., Parker, P.D., Pease, E.K., Pech, K., Phelps, P., Reichhart, L., Shutt, T., Silva, C., Solovov, V.N., Sorensen, P., O'Sullivan, K., Sumner, T.J., Szydagis, M., Taylor, D., Tennyson, B., Tiedt, D.R., Tripathi, M., Tvrznikova, L., Uvarov, S., Verbus, J.R., Walsh, N., Webb, R., White, J.T., Witherell, M.S., Wolfs, F.L.H., Woods, M., Zhang, C.

“…LUX (Large Underground Xenon) is a dark matter direct detection experiment deployed at the 4850' level of the Sanford Underground Research Facility (SURF) in…”
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