Search Results - "Faham, C H"

First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment by Aalbers, J, Akerib, D S, Akerlof, C W, Al Musalhi, A K, Alder, F, Alqahtani, A, Alsum, S K, Amarasinghe, C S, Ames, A, Anderson, T J, Angelides, N, Araújo, H M, Armstrong, J E, Arthurs, M, Azadi, S, Bailey, A J, Baker, A, Balajthy, J, Balashov, S, Bang, J, Bargemann, J W, Barry, M J, Barthel, J, Bauer, D, Baxter, A, Beattie, K, Belle, J, Beltrame, P, Bensinger, J, Benson, T, Bernard, E P, Bhatti, A, Biekert, A, Biesiadzinski, T P, Birch, H J, Birrittella, B, Blockinger, G M, Boast, K E, Boxer, B, Bramante, R, Brew, C A J, Brás, P, Buckley, J H, Bugaev, V V, Burdin, S, Busenitz, J K, Buuck, M, Cabrita, R, Carels, C, Carlsmith, D L, Carlson, B, Carmona-Benitez, M C, Cascella, M, Chan, C, Chawla, A, Chen, H, Cherwinka, J J, Chott, N I, Cole, A, Coleman, J, Converse, M V, Cottle, A, Cox, G, Craddock, W W, Creaner, O, Curran, D, Currie, A, Cutter, J E, Dahl, C E, David, A, Davis, J, Davison, T J R, Delgaudio, J, Dey, S, de Viveiros, L, Dobi, A, Dobson, J E Y, Druszkiewicz, E, Dushkin, A, Edberg, T K, Edwards, W R, Elnimr, M M, Emmet, W T, Eriksen, S R, Faham, C H, Fan, A, Fayer, S, Fearon, N M, Fiorucci, S, Flaecher, H, Ford, P, Francis, V B, Fraser, E D, Fruth, T, Gaitskell, R J, Gantos, N J, Garcia, D, Geffre, A, Gehman, V M, Genovesi, J

“…The LUX-ZEPLIN experiment is a dark matter detector centered on a dual-phase xenon time projection chamber operating at the Sanford Underground Research…”
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Results from a Search for Dark Matter in the Complete LUX Exposure by Akerib, D S, Alsum, S, Araújo, H M, Bai, X, Bailey, A J, Balajthy, J, Beltrame, P, Bernard, E P, Bernstein, A, Biesiadzinski, T P, Boulton, E M, Bramante, R, Brás, P, Byram, D, Cahn, S B, Carmona-Benitez, M C, Chan, C, Chiller, A A, Chiller, C, Currie, A, Cutter, J E, Davison, T J R, Dobi, A, Dobson, J E Y, Druszkiewicz, E, Edwards, B N, Faham, C H, Fiorucci, S, Gaitskell, R J, Gehman, V M, Ghag, C, Gibson, K R, Gilchriese, M G D, Hall, C R, Hanhardt, M, Haselschwardt, S J, Hertel, S A, Hogan, D P, Horn, M, Huang, D Q, Ignarra, C M, Ihm, M, Jacobsen, R G, Ji, W, Kamdin, K, Kazkaz, K, Khaitan, D, Knoche, R, Larsen, N A, Lee, C, Lenardo, B G, Lesko, K T, Lindote, A, Lopes, M I, Manalaysay, A, Mannino, R L, Marzioni, M F, McKinsey, D N, Mei, D-M, Mock, J, Moongweluwan, M, Morad, J A, Murphy, A St J, Nehrkorn, C, Nelson, H N, Neves, F, O'Sullivan, K, Oliver-Mallory, K C, Palladino, K J, Pease, E K, Phelps, P, Reichhart, L, Rhyne, C, Shaw, S, Shutt, T A, Silva, C, Solmaz, M, Solovov, V N, Sorensen, P, Stephenson, S, 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, Uvarov, S, Verbus, J R, Webb, R C, White, J T, Whitis, T J, Witherell, M S, Wolfs, F L H, Xu, J, Yazdani, K, Young, S K

“…We report constraints on spin-independent weakly interacting massive particle (WIMP)-nucleon scattering using a 3.35×10^{4}  kg day exposure of the Large…”
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Improved Limits on Scattering of Weakly Interacting Massive Particles from Reanalysis of 2013 LUX Data by Akerib, D S, Araújo, H M, Bai, X, Bailey, A J, Balajthy, J, Beltrame, P, Bernard, E P, Bernstein, A, Biesiadzinski, T P, Boulton, E M, Bradley, A, Bramante, R, Cahn, S B, Carmona-Benitez, M C, Chan, C, Chapman, J J, Chiller, A A, Chiller, C, Currie, A, Cutter, J E, Davison, T J R, de Viveiros, L, Dobi, A, Dobson, J E Y, Druszkiewicz, E, Edwards, B N, Faham, C H, Fiorucci, S, Gaitskell, R J, Gehman, V M, Ghag, C, Gibson, K R, Gilchriese, M G D, Hall, C R, Hanhardt, M, Haselschwardt, S J, Hertel, S A, Hogan, D P, Horn, M, Huang, D Q, Ignarra, C M, Ihm, M, Jacobsen, R G, Ji, W, Kazkaz, K, Khaitan, D, Knoche, R, Larsen, N A, Lee, C, Lenardo, B G, Lesko, K T, Lindote, A, Lopes, M I, Malling, D C, Manalaysay, A, Mannino, R L, Marzioni, M F, McKinsey, D N, Mei, D-M, Mock, J, Moongweluwan, M, Morad, J A, Murphy, A St J, Nehrkorn, C, Nelson, H N, Neves, F, O'Sullivan, K, Oliver-Mallory, K C, Ott, R A, Palladino, K J, Pangilinan, M, Pease, E K, Phelps, P, Reichhart, L, Rhyne, C, Shaw, S, Shutt, T A, Silva, C, Solovov, V N, Sorensen, P, Stephenson, S, Sumner, T J, Szydagis, M, Taylor, D J, Taylor, W, Tennyson, B P, Terman, P A, Tiedt, D R, To, W H, Tripathi, M, Tvrznikova, L, Uvarov, S, Verbus, J R, Webb, R C, White, J T, Whitis, T J, Witherell, M S, Wolfs, F L H, Yazdani, K, Young, S K

“…We present constraints on weakly interacting massive particles (WIMP)-nucleus scattering from the 2013 data of the Large Underground Xenon dark matter…”
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First results from the LUX dark matter experiment at the Sanford underground research facility by Akerib, D S, Araújo, H M, Bai, X, Bailey, A J, Balajthy, J, Bedikian, S, Bernard, E, Bernstein, A, Bolozdynya, A, Bradley, A, Byram, D, Cahn, S B, Carmona-Benitez, M C, Chan, C, Chapman, J J, Chiller, A A, Chiller, C, Clark, K, Coffey, T, Currie, A, Curioni, A, Dazeley, S, de Viveiros, L, Dobi, A, Dobson, J, Dragowsky, E M, 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, Hertel, S A, Horn, M, Huang, D Q, Ihm, M, Jacobsen, R G, Kastens, L, Kazkaz, K, Knoche, R, Kyre, S, Lander, R, Larsen, N A, Lee, C, Leonard, D S, Lesko, K T, Lindote, A, Lopes, M I, Lyashenko, A, Malling, D C, Mannino, R, McKinsey, D N, Mei, D-M, Mock, J, Moongweluwan, M, Morad, J, Morii, M, Murphy, A St J, Nehrkorn, C, Nelson, H, Neves, F, Nikkel, J A, Ott, R A, Pangilinan, M, Parker, P D, Pease, E K, Pech, K, Phelps, P, Reichhart, L, Shutt, T, Silva, C, Skulski, W, Sofka, C J, Solovov, V N, Sorensen, P, Stiegler, T, O'Sullivan, K, Sumner, T J, Svoboda, R, Sweany, M, Szydagis, M, Taylor, D, Tennyson, B, Tiedt, D R, Tripathi, M, Uvarov, S, Verbus, J R, Walsh, N, Webb, R, White, J T, White, D, Witherell, M S, Wlasenko, M, Wolfs, F L H

“…The Large Underground Xenon (LUX) experiment is a dual-phase xenon time-projection chamber operating at the Sanford Underground Research Facility (Lead, South…”
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First Searches for Axions and Axionlike Particles with the LUX Experiment by Akerib, D S, Alsum, S, Aquino, C, Araújo, H M, Bai, X, Bailey, A J, Balajthy, J, Beltrame, P, Bernard, E P, Bernstein, A, Biesiadzinski, T P, Boulton, E M, Brás, P, Byram, D, Cahn, S B, Carmona-Benitez, M C, Chan, C, Chiller, A A, Chiller, C, Currie, A, Cutter, J E, Davison, T J R, Dobi, A, Dobson, J E Y, Druszkiewicz, E, Edwards, B N, Faham, C H, Fallon, S R, Fiorucci, S, Gaitskell, R J, Gehman, V M, Ghag, C, Gibson, K R, Gilchriese, M G D, Hall, C R, Hanhardt, M, 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, Larsen, N A, Lee, C, Lenardo, B G, Lesko, K T, Lindote, A, Lopes, M I, Manalaysay, A, Mannino, R L, Marzioni, M F, McKinsey, D N, Mei, D-M, Mock, J, Moongweluwan, M, Morad, J A, Murphy, A St J, Nehrkorn, C, Nelson, H N, Neves, F, O'Sullivan, K, Oliver-Mallory, K C, Palladino, K J, Pease, E K, Reichhart, L, Rhyne, C, Shaw, S, Shutt, T A, Silva, C, Solmaz, M, Solovov, V N, Sorensen, P, Stephenson, S, 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, Uvarov, S, Velan, V, Verbus, J R, Webb, R C, White, J T, Whitis, T J, Witherell, M S, Wolfs, F L H, Xu, J, Yazdani, K, Young, S K

“…The first searches for axions and axionlike particles with the Large Underground Xenon experiment are presented. Under the assumption of an axioelectric…”
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Results on the Spin-Dependent Scattering of Weakly Interacting Massive Particles on Nucleons from the Run 3 Data of the LUX Experiment by Akerib, D S, Araújo, H M, Bai, X, Bailey, A J, Balajthy, J, Beltrame, P, Bernard, E P, Bernstein, A, Biesiadzinski, T P, Boulton, E M, Bradley, A, Bramante, R, Cahn, S B, Carmona-Benitez, M C, Chan, C, Chapman, J J, Chiller, A A, Chiller, C, Currie, A, Cutter, J E, Davison, T J R, de Viveiros, L, Dobi, A, Dobson, J E Y, Druszkiewicz, E, Edwards, B N, Faham, C H, Fiorucci, S, Gaitskell, R J, Gehman, V M, Ghag, C, Gibson, K R, Gilchriese, M G D, Hall, C R, Hanhardt, M, Haselschwardt, S J, Hertel, S A, Hogan, D P, Horn, M, Huang, D Q, Ignarra, C M, Ihm, M, Jacobsen, R G, Ji, W, Kazkaz, K, Khaitan, D, Knoche, R, Larsen, N A, Lee, C, Lenardo, B G, Lesko, K T, Lindote, A, Lopes, M I, Malling, D C, Manalaysay, A, Mannino, R L, Marzioni, M F, McKinsey, D N, Mei, D-M, Mock, J, Moongweluwan, M, Morad, J A, Murphy, A St J, Nehrkorn, C, Nelson, H N, Neves, F, O'Sullivan, K, Oliver-Mallory, K C, Ott, R A, Palladino, K J, Pangilinan, M, Pease, E K, Phelps, P, Reichhart, L, Rhyne, C, Shaw, S, Shutt, T A, Silva, C, Solovov, V N, Sorensen, P, Stephenson, S, Sumner, T J, Szydagis, M, Taylor, D J, Taylor, W, Tennyson, B P, Terman, P A, Tiedt, D R, To, W H, Tripathi, M, Tvrznikova, L, Uvarov, S, Verbus, J R, Webb, R C, White, J T, Whitis, T J, Witherell, M S, Wolfs, F L H, Yazdani, K, Young, S K

“…We present experimental constraints on the spin-dependent WIMP (weakly interacting massive particle)-nucleon elastic cross sections from LUX data acquired in…”
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The LUX-ZEPLIN (LZ) radioactivity and cleanliness control programs by Alquahtani, A., Anderson, T. J., Armstrong, J. E., Bai, X., Baxter, A., Bernard, E. P., Bernstein, A., Bhatti, A., Boast, K. E., Bramante, R., Branson, S., Bugaev, V. V., Burdin, S., Cabrita, R., Carels, C., Carlsmith, D. L., Carmona-Benitez, M. C., Chan, C., Cherwinka, J. J., Chott, N. I., Curran, D., Currie, A., Dahl, C. E., Decheine, N., Dobi, A., Druszkiewicz, E., Flaecher, H., Fruth, T., Gantos, N. J., Gehman, V. M., Hasselkus, C., Hertel, S. A., Huang, D. Q., Jahangir, O., Jeffery, S. N., Johnson, J., Kamaha, A., Khaleeq, M., Khurana, I., Kim, Y. D., Korolkova, E. V., Kras, J., Kudryavtsev, V. A., Lambert, A. R., Larsen, N. A., Leason, E. A., Li, J., Liu, R., Lopes, M. I., Lyle, J. M., Lynch, C., MarrLaundrie, P., Martin, T. J., McKinsey, D. N., Mizrachi, E., Molash, D., Neves, F., Nikkel, J. A., Nilima, A., Olcina, I., Olevitch, M. A., Pagenkopf, D., Pal, S., Palladino, K. J., Pereira, C., Piepke, A., Pierson, S., Powell, S., Reichenbacher, J., Sabarots, L., Sazzad, A. B. M. R., Shutt, G. W., Silk, J. J., Silva, C., Skulski, W., Smith, A. R., Smith, R. E., Solovov, V. N., Sosnovtsev, V. V., Stancu, I., Stifter, K., Studley, R., Sutcliffe, P., Taylor, W. C., Taylor, R., Temples, D., Thomson, J. A., Tomás, A., Verbus, J. R., Vietanen, T., Walcott, S., Wang, W., Migneault, J., White, R. G., Wilson, K., Witherell, M. S., Wolfs, F. L. H., Xu, J., Yeh, M., Zarzhitsky, P.

“…LUX-ZEPLIN (LZ) is a second-generation direct dark matter experiment with spin-independent WIMP-nucleon scattering sensitivity above 1.4 × 10 - 48 cm 2 for a…”
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Limits on Spin-Dependent WIMP-Nucleon Cross Section Obtained from the Complete LUX Exposure by Akerib, D S, Alsum, S, Araújo, H M, Bai, X, Bailey, A J, Balajthy, J, Beltrame, P, Bernard, E P, Bernstein, A, Biesiadzinski, T P, Boulton, E M, Brás, P, Byram, D, Cahn, S B, Carmona-Benitez, M C, Chan, C, Chiller, A A, Chiller, C, Currie, A, Cutter, J E, Davison, T J R, Dobi, A, Dobson, J E Y, Druszkiewicz, E, Edwards, B N, Faham, C H, Fallon, S R, Fiorucci, S, Gaitskell, R J, Gehman, V M, Ghag, C, Gilchriese, M G D, Hall, C R, Hanhardt, M, 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, Larsen, N A, Lee, C, Lenardo, B G, Lesko, K T, Lindote, A, Lopes, M I, Manalaysay, A, Mannino, R L, Marzioni, M F, McKinsey, D N, Mei, D-M, Mock, J, Moongweluwan, M, Morad, J A, Murphy, A St J, Nehrkorn, C, Nelson, H N, Neves, F, O'Sullivan, K, Oliver-Mallory, K C, Palladino, K J, Pease, E K, Reichhart, L, Rhyne, C, Shaw, S, Shutt, T A, Silva, C, Solmaz, M, Solovov, V N, Sorensen, P, Stephenson, S, 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, Uvarov, S, Velan, V, Verbus, J R, Webb, R C, White, J T, Whitis, T J, Witherell, M S, Wolfs, F L H, Xu, J, Yazdani, K, Young, S K, Zhang, C

“…We present experimental constraints on the spin-dependent WIMP-nucleon elastic cross sections from the total 129.5  kg yr exposure acquired by the Large…”
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Erratum to: The LUX-ZEPLIN (LZ) radioactivity and cleanliness control programs by Alquahtani, A., Anderson, T. J., Armstrong, J. E., Bai, X., Baxter, A., Bernard, E. P., Bernstein, A., Bhatti, A., Boast, K. E., Bramante, R., Branson, S., Bugaev, V. V., Burdin, S., Cabrita, R., Carels, C., Carlsmith, D. L., Carmona-Benitez, M. C., Chan, C., Cherwinka, J. J., Chott, N. I., Curran, D., Currie, A., Dahl, C. E., Decheine, N., Dobi, A., Druszkiewicz, E., Flaecher, H., Fruth, T., Gantos, N. J., Gehman, V. M., Hasselkus, C., Hertel, S. A., Huang, D. Q., Jahangir, O., Jeffery, S. N., Johnson, J., Kamaha, A., Khaleeq, M., Khurana, I., Kim, Y. D., Korolkova, E. V., Kras, J., Kudryavtsev, V. A., Lambert, A. R., Larsen, N. A., Leason, E. A., Li, J., Liu, R., Lopes, M. I., Lyle, J. M., Lynch, C., MarrLaundrie, P., Martin, T. J., McKinsey, D. N., Mizrachi, E., Molash, D., Neves, F., Nikkel, J. A., Nilima, A., Olcina, I., Olevitch, M. A., Pagenkopf, D., Pal, S., Palladino, K. J., Pereira, C., Piepke, A., Pierson, S., Powell, S., Reichenbacher, J., Sabarots, L., Sazzad, A. B. M. R., Shutt, G. W., Silk, J. J., Silva, C., Skulski, W., Smith, A. R., Smith, R. E., Solovov, V. N., Sosnovtsev, V. V., Stancu, I., Stifter, K., Studley, R., Sutcliffe, P., Taylor, W. C., Taylor, R., Temples, D., Thomson, J. A., Tomás, A., Verbus, J. R., Vietanen, T., Walcott, S., Wang, W., Migneault, J., White, R. G., Wilson, K., Witherell, M. S., Wolfs, F. L. H., Xu, J., Yeh, M., Zarzhitsky, P.

“…LUX-ZEPLIN (LZ) is a second-generation direct dark matter experiment with spin-independent WIMP-nucleon scattering sensitivity above 1.4 × 10-48 cm2 for a WIMP…”
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Chromatographic separation of radioactive noble gases from xenon by Akerib, D.S., Araújo, H.M., Bai, X., Bailey, A.J., Balajthy, J., Beltrame, P., Bernard, E.P., Bernstein, A., Biesiadzinski, T.P., Boulton, E.M., Bramante, R., Cahn, S.B., Carmona-Benitez, M.C., Chan, C., Chiller, A.A., Chiller, C., Coffey, T., Currie, A., Cutter, J.E., Davison, T.J.R., Dobi, A., Dobson, J.E.Y., Druszkiewicz, E., Edwards, B.N., Faham, C.H., Fiorucci, S., Gaitskell, R.J., Gehman, V.M., Ghag, C., Gibson, K.R., Gilchriese, M.G.D., Hall, C.R., Hanhardt, M., Haselschwardt, S.J., Hertel, S.A., Hogan, D.P., Horn, M., Huang, D.Q., Ignarra, C.M., Ihm, M., Jacobsen, R.G., Ji, W., Kamdin, K., Kazkaz, K., Khaitan, D., Knoche, R., Larsen, N.A., Lee, C., Lenardo, B.G., Lesko, K.T., Lindote, A., Lopes, M.I., Manalaysay, A., Mannino, R.L., Marzioni, M.F., McKinsey, D.N., Mei, D.-M., Mock, J., Moongweluwan, M., Morad, J.A., Murphy, A.St.J., Nehrkorn, C., Nelson, H.N., Neves, F., O’Sullivan, K., Oliver-Mallory, K.C., Palladino, K.J., Pease, E.K., Pech, K., Phelps, P., Reichhart, L., Rhyne, C., Shaw, S., Shutt, T.A., Silva, C., Solovov, V.N., Sorensen, P., Stephenson, S., Sumner, T.J., Szydagis, M., Taylor, D.J., Taylor, W., Tennyson, B.P., Terman, P.A., Tiedt, D.R., To, W.H., Tripathi, M., Tvrznikova, L., Uvarov, S., Verbus, J.R., Webb, R.C., White, J.T., Whitis, T.J., Witherell, M.S., Wolfs, F.L.H., Yazdani, K., Young, S.K., Zhang, C.

“…The Large Underground Xenon (LUX) experiment operates at the Sanford Underground Research Facility to detect nuclear recoils from the hypothetical Weakly…”
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Technical results from the surface run of the LUX dark matter experiment by Akerib, D.S., Bai, X., Bernard, E., Bernstein, A., Bradley, A., Byram, D., Cahn, S.B., Carmona-Benitez, M.C., Chapman, J.J., Coffey, T., Dobi, A., Dragowsky, E., Druszkiewicz, E., Edwards, B., Faham, C.H., Fiorucci, S., Gaitskell, R.J., Gibson, K.R., Gilchriese, M., Hall, C., Hanhardt, M., Ihm, M., Jacobsen, R.G., Kastens, L., Kazkaz, K., Knoche, R., Larsen, N., Lee, C., Lesko, K.T., Lindote, A., Lopes, M.I., Lyashenko, A., Malling, D.C., Mannino, R., McKinsey, D.N., Mei, D., Mock, J., Moongweluwan, M., Morii, M., Nelson, H., Neves, F., Nikkel, J.A., Pangilinan, M., Pech, K., Phelps, P., Rodionov, A., Shutt, T., Silva, C., Skulski, W., Solovov, V.N., Sorensen, P., Stiegler, T., Sweany, M., Szydagis, M., Taylor, D., Tripathi, M., Uvarov, S., Verbus, J.R., de Viveiros, L., Walsh, N., Webb, R., White, J.T., Wlasenko, M., Wolfs, F.L.H., Woods, M., Zhang, C.

“…We present the results of the three-month above-ground commissioning run of the Large Underground Xenon (LUX) experiment at the Sanford Underground Research…”
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FPGA-based trigger system for the LUX dark matter experiment by Akerib, D.S., Araújo, H.M., Bai, X., Bailey, A.J., Balajthy, J., Beltrame, P., Bernard, E.P., Bernstein, A., Biesiadzinski, T.P., Boulton, E.M., Bradley, A., Bramante, R., Cahn, S.B., Carmona-Benitez, M.C., Chan, C., Chapman, J.J., Chiller, A.A., Chiller, C., Currie, A., Cutter, J.E., Davison, T.J.R., de Viveiros, L., Dobi, A., Dobson, J.E.Y., Druszkiewicz, E., Edwards, B.N., Faham, C.H., Fiorucci, S., Gaitskell, R.J., Gehman, V.M., Ghag, C., Gibson, K.R., Gilchriese, M.G.D., Hall, C.R., Hanhardt, M., Haselschwardt, S.J., Hertel, S.A., Hogan, D.P., Horn, M., Huang, D.Q., Ignarra, C.M., Ihm, M., Jacobsen, R.G., Ji, W., Kazkaz, K., Khaitan, D., Knoche, R., Larsen, N.A., Lee, C., Lenardo, B.G., Lesko, K.T., Lindote, A., Lopes, M.I., Malling, D.C., Manalaysay, A.G., Mannino, R.L., McKinsey, D.N., Mei, D.-M., Mock, J., Moongweluwan, M., Morad, J.A., Murphy, A.St.J., Nehrkorn, C., Nelson, H.N., Neves, F., O׳Sullivan, K., Oliver-Mallory, K.C., Ott, R.A., Palladino, K.J., Pangilinan, M., Pease, E.K., Phelps, P., Reichhart, L., Rhyne, C., Shaw, S., Shutt, T.A., Silva, C., Skulski, W., Solovov, V.N., Sorensen, P., Stephenson, S., Sumner, T.J., Szydagis, M., Taylor, D.J., Taylor, W., Tennyson, B.P., Terman, P.A., Tiedt, D.R., To, W.H., Tripathi, M., Tvrznikova, L., Uvarov, S., Verbus, J.R., Webb, R.C., White, J.T., Whitis, T.J., Wolfs, F.L.H., Yin, J., Young, S.K., Zhang, C.

“…LUX is a two-phase (liquid/gas) xenon time projection chamber designed to detect nuclear recoils resulting from interactions with dark matter particles…”
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Data acquisition and readout system for the LUX dark matter experiment by Akerib, D.S., Bai, X., Bedikian, S., Bernard, E., Bernstein, A., Bradley, A., Cahn, S.B., Carmona-Benitez, M.C., Carr, D., Chapman, J.J., Clark, K., Classen, T., Coffey, T., Curioni, A., Dazeley, S., de Viveiros, L., Dragowsky, M., Druszkiewicz, E., Faham, C.H., Fiorucci, S., Gaitskell, R.J., Gibson, K.R., Hall, C., Hanhardt, M., Holbrook, B., Ihm, M., Jacobsen, R.G., Kastens, L., Kazkaz, K., Lander, R., Larsen, N., Lee, C., Leonard, D., Lesko, K., Lyashenko, A., Malling, D.C., Mannino, R., McKinsey, D.N., Mei, D., Mock, J., Morii, M., Nelson, H., Nikkel, J.A., Pangilinan, M., Phelps, P., Shutt, T., Skulski, W., Sorensen, P., Spaans, J., Stiegler, T., Svoboda, R., Sweany, M., Szydagis, M., Thomson, J., Tripathi, M., Verbus, J.R., Walsh, N., Webb, R., White, J.T., Wlasenko, M., Wolfs, F.L.H., Woods, M., Zhang, C.

“…LUX is a two-phase (liquid/gas) xenon time projection chamber designed to detect nuclear recoils from interactions with dark matter particles. Signals from the…”
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The LUX-ZEPLIN (LZ) experiment by Akimov, D.Yu, Angelides, N., Araújo, H.M., Armstrong, J.E., Balashov, S., Baxter, A., Belle, J., Bhatti, A., Birrittella, B., Boulton, E.M., Branson, S., Bugaev, V.V., Campbell, J.S., Chiller, A.A., Colling, D., Coughlen, R., Curran, D., da Cunha, J.P., Dardin, S., Davison, T.J.R., de Viveiros, L., Dobson, J.E.Y., Edberg, T.K., Elnimr, M.M., Fruth, T., Gaitskell, R.J., Garcia, D., Geffre, A., Ghag, C., Gibson, E., Gilchriese, M.G.D., Hans, S., Harrison, A., Holtom, E., Ignarra, C.M., Irving, M.N., Johnson, M., Jones, W.G., Kim, W.T., Kocher, C.D., Kravitz, S.W., Kumpan, A.V., Kyre, S., Lee, H.S., Lee, C., Lenardo, B.G., Leonard, R., Lesko, K.T., Liu, Y., Liao, J., Lin, J., Linehan, R., Liu, R., Loniewski, C., Lucero, D., Lynch, C., Manenti, L., McKinsey, D.N., McLaughlin, J., Mei, D.-M., Meng, Y., Naim, D., Nehrkorn, C., Nelson, H.N., Nikkel, J.A., Nilima, A., Oliver-Mallory, K.C., Pagenkopf, D., Palmaccio, V.M., Palmer, J., Pangilinan, M., Penning, B.P., Pereira, G., Peterson, I.B., Piepke, A., Pierson, S., Powell, S., Ratcliff, B.N., Rosero, R., Rynders, D., Sarychev, M., Severson, M., Silva, C., Smith, R.J., Stephenson, S., Studley, R., Sundarnath, K., Szydagis, M., Terman, P.A., Thomas, K.J., Tiedt, D.R., Tronstad, D.R., Tull, C.E., Walcott, S., Wang, L., Wei, W.-Z., Witherell, M.S., Xiang, X., Xiao, Q., Yeh, M.

“…We describe the design and assembly of the LUX-ZEPLIN experiment, a direct detection search for cosmic WIMP dark matter particles. The centerpiece of the…”
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The Large Underground Xenon (LUX) experiment by Akerib, D.S., Bai, X., Bedikian, S., Bernard, E., Bernstein, A., Bolozdynya, A., Bradley, A., Byram, D., Cahn, S.B., Camp, C., Carmona-Benitez, M.C., Carr, D., Chapman, J.J., Chiller, A., Chiller, C., Clark, K., Classen, T., Coffey, T., Curioni, A., Dahl, E., Dazeley, S., de Viveiros, L., Dobi, A., Dragowsky, E., Druszkiewicz, E., Edwards, B., Faham, C.H., Fiorucci, S., Gaitskell, R.J., Gibson, K.R., Gilchriese, M., Hall, C., Hanhardt, M., Holbrook, B., Ihm, M., Jacobsen, R.G., Kastens, L., Kazkaz, K., Knoche, R., Kyre, S., Kwong, J., Lander, R., Larsen, N.A., Lee, C., Leonard, D.S., Lesko, K.T., Lindote, A., Lopes, M.I., Lyashenko, A., Malling, D.C., Mannino, R., Marquez, Z., McKinsey, D.N., Mei, D.-M., Mock, J., Moongweluwan, M., Morii, M., Nelson, H., Neves, F., Nikkel, J.A., Pangilinan, M., Parker, P.D., Pease, E.K., Pech, K., Phelps, P., Rodionov, A., Roberts, P., Shei, A., Shutt, T., Silva, C., Skulski, W., Solovov, V.N., Sofka, C.J., Sorensen, P., Spaans, J., Stiegler, T., Stolp, D., Svoboda, R., Sweany, M., Szydagis, M., Taylor, D., Thomson, J., Tripathi, M., Uvarov, S., Verbus, J.R., Walsh, N., Webb, R., White, D., White, J.T., Whitis, T.J., Wlasenko, M., Wolfs, F.L.H., Woods, M., Zhang, C.

“…The Large Underground Xenon (LUX) collaboration has designed and constructed a dual-phase xenon detector, in order to conduct a search for Weakly Interacting…”
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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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Proposed low-energy absolute calibration of nuclear recoils in a dual-phase noble element TPC using D-D neutron scattering kinematics by Verbus, J.R., Rhyne, C.A., Malling, D.C., Genecov, M., Ghosh, S., Moskowitz, A.G., Chan, S., Chapman, J.J., de Viveiros, L., Faham, C.H., Fiorucci, S., Huang, D.Q., Pangilinan, M., Taylor, W.C., Gaitskell, R.J.

“…We propose a new technique for the calibration of nuclear recoils in large noble element dual-phase time projection chambers used to search for WIMP dark…”
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Extending light WIMP searches to single scintillation photons in LUX by Akerib, D. S, Alsum, S, Araújo, H. M, Bai, X, Balajthy, J, Baxter, A, Beltrame, P, Bernard, E. P, Bernstein, A, Biesiadzinski, T. P, Boulton, E. M, Boxer, B, Brás, P, Burdin, S, Byram, D, Cahn, S. B, Carmona-Benitez, M. C, Chan, C, Chiller, A. A, Currie, A, Cutter, J. E, de Viveiros, L, Dobi, A, Dobson, J. E. Y, Druszkiewicz, E, Fallon, S. R, Fiorucci, S, Gaitskell, R. J, Gehman, V. M, Ghag, C, Gibson, K. R, Gilchriese, M. G. D, Grace, E, Gwilliam, C, Hanhardt, M, Hertel, S. A, Hogan, D. P, Huang, D. Q, Ignarra, C. M, Jacobsen, R. G, Jahangir, O, Ji, W, Kamdin, K, Kazka, K, Khaitan, D, Korolkova, E. V, Kravitz, S, Kudryavtsev, V. A, Larsen, N. A, Lee, C, Lenardo, B. G, Lesko, K. T, Lin, J, Lindote, A, Lopes, M. I, López-Paredes, B, Manalaysay, A, Mannino, R. L, Marangou, N, Marzioni, M. F, Mei, D. M, Mock, J, Morad, J. A, Murphy, A. St. J, Nehrkorn, C, Neves, F, Nilima, A, O'Sullivan, K, Oliver-Mallory, K. C, Palladino, K. J, Pease, E. K, Reichhart, L, Riffard, Q, Rischbieter, G. R. C, Rossiter, P, Shaw, S, Silva, C, Solmaz, M, Solovov, V. N, Sorensen, P, Sumner, T. J, Szydagis, M, Taylor, D. J, Taylor, R, Tennyson, B. P, Terman, P. A, To, W. H, Tripathi, M, Tvrznikova, L, Utku, U, Uvarov, S, Vacheret, A, Velan, V, Verbus, J. R, White, J. T, Whitis, T. J, Woodward, D, Xu, J, Young, S. K, Zhang, C

“…Phys. Rev. D 101, 042001 (2020) We present a novel analysis technique for liquid xenon time projection chambers that allows for a lower threshold by relying on…”
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Measurements of wavelength-dependent double photoelectron emission from single photons in VUV-sensitive photomultiplier tubes by Faham, C. H, Gehman, V. M, Currie, A, Dobi, A, Sorensen, P, Gaitskell, R. J

“…Journal of Instrumentation 10 (2015) P09010 Measurements of double photoelectron emission (DPE) probabilities as a function of wavelength are reported for…”
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Identification of radiopure titanium for the LZ dark matter experiment and future rare event searches by Akerib, D.S., Arnquist, I.J., Bai, X., Belle, J., Beltrame, P., Bernard, E.P., Biesiadzinski, T.P., Boast, K.E., Bolozdynya, A., Boxer, B., Bramante, R., Brás, P., Buckley, J.H., Busenitz, J.K., Carlson, B., Cherwinka, J.J., Chiller, A.A., Chiller, C., Craddock, W.W., Dahl, C.E., Davison, T.J.R., Dobson, J.E.Y., Druszkiewicz, E., Edwards, W.R., Emmet, W.T., Faham, C.H., Gaitskell, R.J., Gehman, V.M., Gerhard, R.M., Ghag, C., Gilchriese, M.G.D., Gomber, B., Haselschwardt, S.J., Hertel, S.A., Hillbrand, S., Hjemfelt, C., Hoppe, E.W., Hor, J.Y-K., Huang, D.Q., Hurteau, T.W., Ignarra, C.M., Kamdin, K., Khaitan, D., Khromov, A.V., Konovalov, A.M., Kudryavtsev, V.A., Kyre, S., Lee, C., Lesko, K.T., Lippincott, W.H., Lopez Paredes, B., Lorenzon, W., Manalaysay, A., Mei, D.-M., Miller, E.H., Mizrachi, E., Mock, J., Monzani, M.E., O’Dell, J., O’Sullivan, K., Oliver-Mallory, K.C., Palladino, K.J., Piepke, A., Preece, R.M., Pushkin, K., Ratcliff, B.N., Reichenbacher, J., Richards, A., Rodrigues, J.P., Rosero, R., Schnee, R.W., Schubnell, M., Skarpaas, K., Solovov, V.N., Sorensen, P., Stancu, I., Stark, M.R., Stephenson, S., Stiegler, T.M., Stifter, K., Sumner, T.J., Taylor, W.C., Temples, D., Thomas, K.J., To, W.H., Tripathi, M., Va’vra, J., van der Grinten, M.G.D., Verbus, J.R., Vuosalo, C.O., Waldron, W.L., Wang, R., Watson, R., Webb, R.C., Wei, W.-Z., While, M., Wolfs, F.L.H., Worm, S., Yeh, M., Yin, J.

“…The LUX-ZEPLIN (LZ) experiment will search for dark matter particle interactions with a detector containing a total of 10 tonnes of liquid xenon within a…”
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