Search Results - "Cutter, J. E."

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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Measurement of the gamma ray background in the Davis cavern at the Sanford Underground Research Facility by Akerlof, C.W., Angelides, N., Araújo, H.M., Armstrong, J.E., Arthurs, M., Bai, X., Baxter, A., Biekert, A., Biesiadzinski, T.P., Boast, K.E., Boxer, B., Buckley, J.H., Busenitz, J.K., Carels, C., Carmona-Benitez, M.C., Chan, C., Cottle, A., Dahl, C.E., Edberg, T.K., Fiorucci, S., Flaecher, H., Gaitskell, R.J., Ghag, C., Gilchriese, M.G.D., Hall, C.R., Harrison, J., Haselschwardt, S.J., Hertel, S.A., Horn, M., Ignarra, C.M., Jahangir, O., Johnson, J., Khazov, A., Kim, W.T., Kocher, C.D., Korley, L., Korolkova, E.V., Kraus, H., Kravitz, S.W., Kreczko, L., Krikler, B., Kudryavtsev, V.A., Leason, E.A., Lee, J., Leonard, D.S., Lesko, K.T., Levy, C., Li, J., Liao, J., Liao, F.-T., Lin, J., Lindote, A., Lippincott, W.H., Liu, R., Liu, X., López Paredes, B., Lorenzon, W., Luitz, S., Majewski, P.A., Manenti, L., Marangou, N., Meng, Y., Miller, E.H., Morad, J.A., Mount, B.J., Naim, D., Nedlik, C., Nelson, H.N., Neves, F., Nilima, A., Oliver-Mallory, K.C., Palladino, K.J., Pease, E.K., Penning, B.P., Pereira, G., Pushkin, K., Reichenbacher, J., Rischbieter, G.R.C., Rossiter, P., Rutherford, G., Sazzad, A.B.M.R., Seymour, D., Shaw, S., Solmaz, M., Solovov, V.N., Sorensen, P., Stancu, I., Stevens, A., Stifter, K., Szydagis, M., Taylor, W.C., Taylor, R., Tomás, A., Tripathi, M., Tvrznikova, L., Uvarov, S., Vacheret, A., Watson, J.R., Whitis, T.J., Yin, J.

“…Deep underground environments are ideal for low background searches due to the attenuation of cosmic rays by passage through the earth. However, they are…”
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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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Simulations of events for the LUX-ZEPLIN (LZ) dark matter experiment by Alsum, S.K., Angelides, N., Araújo, H.M., Arthurs, M., Bai, X., Balajthy, J., Balashov, S., Baxter, A., Bernard, E.P., Birch, H.J., Boast, K.E., Boxer, B., Buckley, J.H., Bugaev, V.V., Busenitz, J.K., Cabrita, R., Carels, C., Carmona-Benitez, M.C., Cole, A., Cottle, A., Cutter, J.E., Viveiros, L. de, Druszkiewicz, E., Fan, A., Fayer, S., Fruth, T., Ghag, C., Gibson, E., Gokhale, S., van der Grinten, M.G.D., Harrison, A., Hertel, S.A., Hor, J.Y-K., Huang, D.Q., Ignarra, C.M., Ji, W., Kaboth, A.C., Kazkaz, K., Kocher, C.D., Korley, L., Korolkova, E.V., Kras, J., Kraus, H., Kravitz, S., Kudryavtsev, V.A., Leason, E.A., Lee, J., Lesko, K.T., Levy, C., Li, J., Liao, J., Liao, F.-T., Lin, J., Liu, R., Loniewski, C., Lopes, M.I., Lorenzon, W., Luitz, S., Manalaysay, A., Manenti, L., McLaughlin, J., Meng, Y., Miller, E.H., Mizrachi, E., Morad, J.A., Morrison, E., Nehrkorn, C., Nilima, A., Oliver-Mallory, K.C., Parveen, N., Piepke, A., Pushkin, K., Richards, A., Rutherford, G., Sazzad, A.B.M.R., Schnee, R.W., Seymour, D., Shaw, S., Silk, J.J., Smith, R., Stancu, I., Stevens, A., Stifter, K., Swanson, N., Tan, M., Taylor, R., Temples, D.J., Tiedt, D.R., Timalsina, M., Tripathi, M., Tvrznikova, L., Vaitkus, A., Wang, J.J., Wang, W., Webb, R.C., Whitis, T.J., Woodward, D., Xiang, X., Yeh, M., Zarzhitsky, P.

“…The LUX-ZEPLIN dark matter search aims to achieve a sensitivity to the WIMP-nucleon spin-independent cross-section down to (1–2)×10−12 pb at a WIMP mass of 40 …”
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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.

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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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The LUX-ZEPLIN (LZ) radioactivity and cleanliness control programs by Akerlof, C. W., Arthurs, M., Bang, J., Bauer, P., Bernstein, A., Bhatti, A., Biesiadzinski, T. P., Boast, K. E., Bolozdynya, A. I., Boulton, E. M., Boxer, B., Breidenbach, M., Cabrita, R., Carmona-Benitez, M. C., Cole, A., Coleman, J., Curran, D., Davis, J., Decheine, N., Dobson, J. Y., Flaecher, H., Gomber, B., Greenall, A., Gregerson, G., Hasselkus, C., Haselschwardt, S. J., Hillbrand, S., Hoff, M. D., Horn, M., Hurteau, T. W., Ignarra, C. M., Jahangir, O., Jeffery, S. N., Ji, W., Keefner, J., Khaitan, D., Khromov, A. V., Kodroff, D., Konovalov, A. M., Korley, L., Kras, J., Kravitz, S. W., Kyre, S., Laundrie, A., Lesko, K. T., Lin, J., Lindote, A., Lippincott, W. H., Loniewski, C., Paredes, B. López, Lynch, C., Malling, D. C., Manenti, L., Marangou, N., Mei, D. -M., Morad, J. A., Naylor, A., Nehrkorn, C., Neves, F., O’Dell, J., Oxborough, L., Pagac, A., Pagenkopf, D., Palmer, J., Parveen, N., Pease, E. K., Pereira, G., Preece, R. M., Richards, A., Riffard, Q., Rossiter, P., Rucinski, R., Sabarots, L., Schnee, R. W., Schubnell, M., Shutt, T. A., Smith, A. R., Solmaz, M., Stern, N., Stifter, K., Swanson, N., Taylor, D. J., Temples, D., Terman, P. A., Timalsina, M., To, W. H., Tope, T. E., Tvrznikova, L., Utes, M., Va’vra, J., Verbus, J. R., Vietanen, T., Wang, Y., Migneault, J., Weatherly, S., Wei, W. -Z., While, M., White, R. G., Witherell, M. S., Young, I.

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The LUX-ZEPLIN (LZ) radioactivity and cleanliness control programs by Akerlof, C. W., Arthurs, M., Bang, J., Bauer, P., Bernstein, A., Bhatti, A., Biesiadzinski, T. P., Boast, K. E., Bolozdynya, A. I., Boulton, E. M., Boxer, B., Breidenbach, M., Cabrita, R., Carmona-Benitez, M. C., Cole, A., Coleman, J., Curran, D., Davis, J., Decheine, N., Dobson, J. Y., Flaecher, H., Gomber, B., Greenall, A., Gregerson, G., Hasselkus, C., Haselschwardt, S. J., Hillbrand, S., Hoff, M. D., Horn, M., Hurteau, T. W., Ignarra, C. M., Jahangir, O., Jeffery, S. N., Ji, W., Keefner, J., Khaitan, D., Khromov, A. V., Kodroff, D., Konovalov, A. M., Korley, L., Kras, J., Kravitz, S. W., Kyre, S., Laundrie, A., Lesko, K. T., Lin, J., Lindote, A., Lippincott, W. H., Loniewski, C., Paredes, B. López, Lynch, C., Malling, D. C., Manenti, L., Marangou, N., Mei, D. -M., Morad, J. A., Naylor, A., Nehrkorn, C., Neves, F., O’Dell, J., Oxborough, L., Pagac, A., Pagenkopf, D., Palmer, J., Parveen, N., Pease, E. K., Pereira, G., Preece, R. M., Richards, A., Riffard, Q., Rossiter, P., Rucinski, R., Sabarots, L., Schnee, R. W., Schubnell, M., Shutt, T. A., Smith, A. R., Solmaz, M., Stern, N., Stifter, K., Swanson, N., Taylor, D. J., Temples, D., Terman, P. A., Timalsina, M., To, W. H., Tope, T. E., Tvrznikova, L., Utes, M., Va’vra, J., Verbus, J. R., Vietanen, T., Wang, Y., Migneault, J., Weatherly, S., Wei, W. -Z., While, M., White, R. G., Witherell, M. S., Young, I.

“…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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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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Results of a Search for Sub-GeV Dark Matter Using 2013 LUX Data 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., Boxer, B., Brás, P., Burdin, S., 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., Gwilliam, C., Hall, C. R., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Jacobsen, R. G., Jahangir, O., Ji, W., Kamdin, K., Kazkaz, K., Khaitan, D., Knoche, R., Korolkova, E. V., Kravitz, S., Kudryavtsev, V. A., Lenardo, B. G., Lesko, K. T., Liao, J., Lin, J., 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., Naylor, A., Nehrkorn, C., Nelson, H. N., Neves, F., Oliver-Mallory, K. C., Palladino, K. J., Pease, E. K., Riffard, Q., Rischbieter, G. R. C., Rhyne, C., Rossiter, P., 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., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L. H., Woodward, D., Xu, J., Yazdani, K., Zhang, C.

“…The scattering of dark matter (DM) particles with sub-GeV masses off nuclei is difficult to detect using liquid xenon-based DM search instruments because the…”
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Results of a Search for Sub-GeV Dark Matter Using 2013 LUX Data 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., Boxer, B., Brás, P., Burdin, S., 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., Gwilliam, C., Hall, C. R., Haselschwardt, S. J., Hertel, S. A., Hogan, D. P., Horn, M., Huang, D. Q., Ignarra, C. M., Jacobsen, R. G., Jahangir, O., Ji, W., Kamdin, K., Kazkaz, K., Khaitan, D., Knoche, R., Korolkova, E. V., Kravitz, S., Kudryavtsev, V. A., Lenardo, B. G., Lesko, K. T., Liao, J., Lin, J., 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., Naylor, A., Nehrkorn, C., Nelson, H. N., Neves, F., Oliver-Mallory, K. C., Palladino, K. J., Pease, E. K., Riffard, Q., Rischbieter, G. R. C., Rhyne, C., Rossiter, P., 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., Webb, R. C., White, J. T., Whitis, T. J., Witherell, M. S., Wolfs, F. L. H., Woodward, D., Xu, J., Yazdani, K., Zhang, C., LUX Collaboration

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Simulations of events for the LUX-ZEPLIN (LZ) dark matter experiment by Akerlof, C. W., Armstrong, J. E., Arthurs, M., Bai, X., Balashov, S., Bang, J., Baxter, A., Bensinger, J., Bernard, E. P., Bhatti, A., Biekert, A., Boast, K. E., Boxer, B., Brás, P., Burdin, S., Carels, C., Cascella, M., Chott, N. I., Cole, A., Cottle, A., Dahl, C. E., Druszkiewicz, E., Fayer, S., Fiorucci, S., Flaecher, H., Gaitskell, R. J., Ghag, C., Hertel, S. A., Hor, J. Y-K., Horn, M., Huang, D. Q., Ignarra, C. M., Ji, W., Kaboth, A. C., Kazkaz, K., Khazov, A., Khurana, I., Kocher, C. D., Korley, L., Kreczko, L., Krikler, B., Kudryavtsev, V. A., Lee, J., Levy, C., Li, J., Liao, J., Liao, F. -T., Lin, J., Lindote, A., Linehan, R., Lippincott, W. H., Loniewski, C., Lopes, M. I., López Paredes, B., Lorenzon, W., Luitz, S., Manalaysay, A., Marangou, N., Marzioni, M. F., McKinsey, D. N., Meng, Y., Miller, E. H., Morad, J. A., Murphy, A. St.J., Naim, D., Naylor, A., Nedlik, C., Nehrkorn, C., Neves, F., Nilima, A., Parveen, N., Penning, B., Pereira, G., Piepke, A., Pushkin, K., Riffard, Q., Rischbieter, G. R.C., Rossiter, P., Rutherford, G., Schnee, R. W., Schubnell, M., Scovell, P. R., Seymour, D., Shaw, S., Shutt, T. A., Silk, J. J., Silva, C., Sorensen, P., Stancu, I., Szydagis, M., Tan, M., Taylor, W. C., Taylor, R., Tiedt, D. R., Tomás, A., Tripathi, M., Turner, W., Utku, U., Webb, R. C., White, R. G.

“…The LUX-ZEPLIN dark matter search aims to achieve a sensitivity to the WIMP-nucleon spin-independent cross-section down to (1-2) $\times$ $10^{-12}$ pb at a…”
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Simulations of events for the LUX-ZEPLIN (LZ) dark matter experiment by Akerlof, C. W., Armstrong, J. E., Arthurs, M., Bai, X., Balashov, S., Bang, J., Baxter, A., Bensinger, J., Bernard, E. P., Bhatti, A., Biekert, A., Boast, K. E., Boxer, B., Brás, P., Burdin, S., Carels, C., Cascella, M., Chott, N. I., Cole, A., Cottle, A., Dahl, C. E., Druszkiewicz, E., Fayer, S., Fiorucci, S., Flaecher, H., Gaitskell, R. J., Ghag, C., Hertel, S. A., Hor, J. Y-K., Horn, M., Huang, D. Q., Ignarra, C. M., Ji, W., Kaboth, A. C., Kazkaz, K., Khazov, A., Khurana, I., Kocher, C. D., Korley, L., Kreczko, L., Krikler, B., Kudryavtsev, V. A., Lee, J., Levy, C., Li, J., Liao, J., Liao, F. -T., Lin, J., Lindote, A., Linehan, R., Lippincott, W. H., Loniewski, C., Lopes, M. I., López Paredes, B., Lorenzon, W., Luitz, S., Manalaysay, A., Marangou, N., Marzioni, M. F., McKinsey, D. N., Meng, Y., Miller, E. H., Morad, J. A., Murphy, A. St.J., Naim, D., Naylor, A., Nedlik, C., Nehrkorn, C., Neves, F., Nilima, A., Parveen, N., Penning, B., Pereira, G., Piepke, A., Pushkin, K., Riffard, Q., Rischbieter, G. R.C., Rossiter, P., Rutherford, G., Schnee, R. W., Schubnell, M., Scovell, P. R., Seymour, D., Shaw, S., Shutt, T. A., Silk, J. J., Silva, C., Sorensen, P., Stancu, I., Szydagis, M., Tan, M., Taylor, W. C., Taylor, R., Tiedt, D. R., Tomás, A., Tripathi, M., Turner, W., Utku, U., Webb, R. C., White, R. G.

“…The LUX-ZEPLIN dark matter search aims to achieve a sensitivity to the WIMP-nucleon spin-independent cross-section down to (1-2) $\times$ $10^{-12}$ pb at a…”
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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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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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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., Marzioni, M. F., McKinsey, D. N., Mei, D. -M., Mock, J., Moongweluwan, M., Morad, J. A., Murphy, A. St. J., 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., 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., Yin, J., Young, S. K., Zhang, C.

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A Review of NEST Models, and Their Application to Improvement of Particle Identification in Liquid Xenon Experiments by Szydagis, M, Balajthy, J, Block, G. A, Brodsky, J. P, Brown, E, Cutter, J. E, Farrell, S. J, Huang, J, Kozlova, E. S, Liebenthal, C. S, McKinsey, D. N, McMichael, K, Mooney, M, Mueller, J, Ni, K, Rischbieter, G. R. C, Tripathi, M, Tunnell, C. D, Velan, V, Wyman, M. D, Zhao, Z, Zhong, M

“…This paper discusses microphysical simulation of interactions in liquid xenon, the active detector medium in many leading rare-event physics searches, and…”
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First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment by Akerlof, C. W, Alder, F, Alqahtani, A, Bailey, A. J, Baker, A, Balajthy, J, Bang, J, Bargemann, J. W, Barry, M. J, Blockinger, G. M, Boast, K. E, Boxer, B, Bramante, R, Bugaev, V. V, Busenitz, J. K, Buuck, M, Carels, C, Cascella, M, Chott, N. I, Cole, A, Craddock, W. W, Creaner, O, Curran, D, Dahl, C. E, Delgaudio, J, de Viveiros, L, Dobson, J. E. Y, Emmet, W. T, Fiorucci, S, Flaecher, H, Francis, V. B, Geffre, A, Gibson, E, Gomber, B, Green, J, Hall, C. R, Hoff, M. D, Horn, M, Ignarra, C. M, Ji, W, Kamaha, A. C, Kasey, V, Kazkaz, K, Khaleeq, M, Khazov, A, Kocher, C. D, Kodroff, D, Kras, J, Kraus, H, Krikler, B, Leason, E. A, Leonard, R, Levy, C, Lippincott, W. H, Liu, R, Asamar, E. Lopez, Luitz, S, Mannino, R. L, Marangou, N, Marzioni, M. F, McCarthy, M. E, McKinsey, D. N, Miller, E. H, Mock, J. A, Monte, A, Mount, B. J, Naim, D, Nedlik, C, Nehrkorn, C, Nikoleyczik, J. A, Orpwood, J, Palmer, J, Pangilinan, M, Pereira, G, Piepke, A, Pushkin, K, Qie, Y, Ratcliff, B. N, Rodriguez, A, Rose, H. J, Scovell, P. R, Shutt, T, Smith, R, Sorensen, P, Soria, J, Stark, M. R, Stiegler, T. M, Stifter, K, Sumner, T. J, Temples, D. J, Tong, Z, Trask, M, Tripathi, M, Turner, W, Wang, A, Whitis, T. J, Williams, M, Wolfs, J. D, Xiao, Q, Yin, J

“…Phys. Rev. Lett. 131, 041002 (2023) The LUX-ZEPLIN experiment is a dark matter detector centered on a dual-phase xenon time projection chamber operating at the…”
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Fast and Flexible Analysis of Direct Dark Matter Search Data with Machine Learning by LUX Collaboration, Akerib, D. S, Alsum, S, Araújo, H. M, Bai, X, Balajthy, J, Bang, J, Baxter, A, Bernard, E. P, Bernstein, A, Biesiadzinski, T. P, Boulton, E. M, Boxer, B, Brás, P, Burdin, S, Byram, D, Carrara, N, Carmona-Benitez, M. C, Chan, C, Cutter, J. E, de Viveiros, L, Druszkiewicz, E, Ernst, J, Fan, A, Fiorucci, S, Gaitskell, R. J, Ghag, C, Gilchriese, M. G. D, Gwilliam, C, Hall, C. R, Haselschwardt, S. J, Hertel, S. A, Hogan, D. P, Horn, M, Huang, D. Q, Ignarra, C. M, Jacobsen, R. G, Jahangir, O, Ji, W, Kamdin, K, Kazkaz, K, Khaitan, D, Korolkova, E. V, Kravitz, S, Kudryavtsev, V. A, Leason, E, Lenardo, B. G, Lesko, K. T, Liao, J, Lin, J, Lindote, A, Lopes, M. I, Manalaysay, A, Mannino, R. L, Marangou, N, McKinsey, D. N, Mei, D. -M, Morad, J. A, Murphy, A. St. J, Naylor, A, Nehrkorn, C, Nelson, H. N, Neves, F, Nilima, A, Oliver-Mallory, K. C, Palladino, K. J, Rhyne, C, Riffard, Q, Rischbieter, G. R. C, Rossiter, P, Shaw, S, Shutt, T. A, Silva, C, Solmaz, M, Solovov, V. N, Sorensen, P, Sumner, T. J, Swanson, N, Szydagis, M, Taylor, D. J, Taylor, R, Taylor, W. C, Tennyson, B. P, Terman, P. A, Tiedt, D. R, To, W. H, Tvrznikova, L, Utku, U, Vacheret, A, Vaitkus, A, Velan, V, Webb, R. C, White, J. T, Whitis, T. J, Witherell, M. S, Wolfs, F. L. H, Woodward, D, Xian, X, Xu, J, Zhang, C

“…Phys. Rev. D 106 (2022), 072009 We present the results from combining machine learning with the profile likelihood fit procedure, using data from the Large…”
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Improved Dark Matter Search Sensitivity Resulting from LUX Low-Energy Nuclear Recoil Calibration by LUX Collaboration, Akerib, D. S, Alsum, S, Araújo, H. M, Bai, X, Balajthy, J, Bang, J, Baxter, A, Bernard, E. P, Bernstein, A, Biesiadzinski, T. P, Boulton, E. M, Boxer, B, Brás, P, Burdin, S, Byram, D, Carmona-Benitez, M. C, Chan, C, Cutter, J. E, de Viveiros, L, Druszkiewicz, E, Fan, A, Fiorucci, S, Gaitskell, R. J, Ghag, C, Gilchriese, M. G. D, Gwilliam, C, Hall, C. R, Haselschwardt, S. J, Hertel, S. A, Hogan, D. P, Horn, M, Huang, D. Q, Ignarra, C. M, Jacobsen, R. G, Jahangir, O, Ji, W, Kamdin, K, Kazkaz, K, Khaitan, D, Korolkova, E. V, Kravitz, S, Kudryavtsev, V. A, Leason, E, Lesko, K. T, Liao, J, Lin, J, Lindote, A, Lopes, M. I, Manalaysay, A, Mannino, R. L, Marangou, N, McKinsey, D. N, Mei, D. -M, Morad, J. A, Murphy, A. St. J, Naylor, A, Nehrkorn, C, Nelson, H. N, Neves, F, Nilima, A, Oliver-Mallory, K. C, Palladino, K. J, Rhyne, C, Riffard, Q, Rischbieter, G. R. C, Rossiter, P, Shaw, S, Shutt, T. A, Silva, C, Solmaz, M, Solovov, V. N, Sorensen, P, Sumner, T. J, Swanson, N, Szydagis, M, Taylor, D. J, Taylor, R, Taylor, W. C, Tennyson, B. P, Terman, P. A, Tiedt, D. R, To, W. H, Tvrznikova, L, Utku, U, Vacheret, A, Vaitkus, A, Velan, V, Webb, R. C, White, J. T, Whitis, T. J, Witherell, M. S, Wolfs, F. L. H, Woodward, D, Xiang, X, Xu, J, Zhang, C

“…Dual-phase xenon time projection chamber (TPC) detectors have demonstrated superior search sensitivities to dark matter over a wide range of particle masses…”
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