Search Results - "Nikoleyczik, J"

Nuclear recoil response of liquid xenon and its impact on solar 8B neutrino and dark matter searches by Xiang, X, Gaitskell, R. J, Liu, R, Bang, J, Xu, J, Lippincott, W. H, Aalbers, J, Dobson, J. E. Y, Szydagis, M, Rischbieter, G. R. C, Parveen, N, Huang, D. Q, Olcina, I, James, R. J, Nikoleyczik, J. A

“…Knowledge of the ionization and scintillation responses of liquid xenon (LXe) to nuclear recoils is crucial for LXe-based dark matter experiments. Current…”
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First Constraints on WIMP-Nucleon Effective Field Theory Couplings in an Extended Energy Region From LUX-ZEPLIN by LZ Collaboration, Aalbers, J, Alder, F, Amarasinghe, C. S, Ames, A, Angelides, N, Araújo, H. M, Armstrong, J. E, Bargemann, J. W, Baxter, A, Beattie, K, Biesiadzinski, T. P, Blockinger, G. M, Brew, C. A. J, Brás, P, Buuck, M, Carmona-Benitez, M. C, Chawla, A, Chen, H, Cherwinka, J. J, Chott, N. I, Converse, M. V, Dahl, C. E, Delgaudio, J, Dey, S, de Viveiros, L, Dobson, J. E. Y, Eriksen, S. R, Fearon, N. M, Flaecher, H, Fruth, T. M. A, Gaitskell, R. J, Geffre, A, Gibbons, R, Green, J, Han, S, Hartigan-O'Connor, E, Heuermann, G, Homenides, G. J, Huang, D. Q, Hunt, D, Jacquet, E, James, R. S, Johnson, J, Kaboth, A. C, Kamaha, A. C, Khurana, I, Kim, J, Kingston, J, Kodroff, D, Korley, L, Kravitz, S, Kreczko, L, Lee, J, Leonard, D. S, Linehan, R, Lippincott, W. H, Asamar, E. Lopez, Lorenzon, W, Maupin, C, McCarthy, M. E, McLaughlin, J, Mizrachi, E, Mendoza, J. D. Morales, Murdy, M, Nedlik, C, Nelson, H. N, Nguyen, A, Nikoleyczik, J. A, Orpwood, J, Pannifer, N, Patton, S. J, Pereira, G, Perry, E, Qie, Y, Rhyne, C. A, Riffard, Q, Rosero, R, Rushton, T, Santone, D, Schnee, R. W, Shaw, S, Silk, J. J, Silva, C, Sinev, G, Smith, R, Stevens, A, Stifter, K, Tovey, D. R, Velan, V, Wang, Y, Weeldreyer, L, Woodford, S, Woodward, D, Wright, C. J, Xia, Q, Xiang, X, Xu, J, Yeh, M, Zweig, E. A

“…Phys. Rev. D 109, 092003 (2024) Following the first science results of the LUX-ZEPLIN (LZ) experiment, a dual-phase xenon time projection chamber operating…”
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New constraints on ultraheavy dark matter from the LZ experiment by Aalbers, J, Anderson, T. J, Angelides, N, Arthurs, M, Baker, A, Balashov, S, Bang, J, Beattie, K, Benson, T, Bhatti, A, Biekert, A, Biesiadzinski, T. P, Birch, H. J, Boxer, B, Burdin, S, Carmona-Benitez, M. C, Cherwinka, J. J, Converse, M. V, Cottle, A, Cox, G, Curran, D, David, A, Delgaudio, J, Ding, C, Druszkiewicz, E, Fiorucci, S, Fraser, E. D, Gaitskell, R. J, Geffre, A, Genovesi, J, Ghag, C, van der Grinten, M. G. D, Hall, C. R, Hartigan-O'Connor, E, Hertel, S. A, Huang, D. Q, Ignarra, C. M, Jacquet, E, Kaboth, A. C, Khaitan, D, Korley, L, Korolkova, E. V, Kraus, H, Kudryavtsev, V. A, Levy, C, Lin, J, Lopes, M. I, Lorenzon, W, Lu, C, Luitz, S, Majewski, P. A, Manalaysay, A, Mannino, R. L, McCarthy, M. E, McDowell, G, McKinsey, D. N, McMonigle, R, Miller, E. H, Mount, B. J, Murdy, M, Nedlik, C, Nelson, H. N, Neves, F, Olcina, I, Palladino, K. J, Pannifer, N. J, Parveen, N, Patton, S. J, Penning, B, Perry, E, Piepke, A, Qie, Y, Riyat, H. S, Rushton, T, Rynders, D, Schnee, R. W, Shaw, S, Silk, J. J, Silva, C, Sinev, G, Smith, R, Sorensen, P, Soria, J, Stifter, K, Szydagis, M, Timalsina, M, Tovey, D. R, Trask, M, Turner, W, Vaitkus, A. C, Velan, V, Wang, Y, Weeldreyer, L, Whitis, T. J, Wisniewski, W. J, Woodford, S, Woodward, D, Wright, C. J, Xia, Q, Xu, J

“…Phys. Rev. D 109, 112010 (2024) Searches for dark matter with liquid xenon time projection chamber experiments have traditionally focused on the region of the…”
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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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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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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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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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Measurement of the gamma ray background in the Davis cavern at the Sanford Underground Research Facility by Akerib, D. S., Akerlof, C. W., Angelides, N., Araújo, H. M., Bai, X., Boast, K. E., Brás, P., Buckley, J. H., Bugaev, V. V., Carels, C., Carlsmith, D. L., Carmona-Benitez, M. C., Cascella, M., Chan, C., Cole, A., Cutter, J. E., Dobson, J. E. Y., Druszkiewicz, E., Fiorucci, S., Flaecher, H., Fruth, T., Ghag, C., Gokhale, S., van der Grinten, M. G. D., Hall, C. R., Haselschwardt, S. J., Hor, J. Y-K., Horn, M., Ignarra, C. M., Jahangir, O., Ji, W., Johnson, J., Kaboth, A. C., Kamdin, K., Korley, L., Korolkova, E. V., Kraus, H., Kravitz, S. W., Kreczko, L., Krikler, B., Kudryavtsev, V. A., Lesko, K. T., Levy, C., Liao, J., Lindote, A., Liu, R., Liu, X., López Paredes, B., Lorenzon, W., Luitz, S., Lyle, J. M., Manenti, L., Mannino, R. L., Marangou, N., Marzioni, M. F., McKinsey, D. N., McLaughlin, J., Meng, Y., Morad, J. A., Murphy, A. St. J., Naim, D., Naylor, A., Nedlik, C., Nikoleyczik, J., Nilima, A., Olcina, I., Oliver-Mallory, K. C., Pal, S., Palladino, K. J., Pereira, G., Piepke, A., Pushkin, K., Reichenbacher, J., Rhyne, C. A., Riffard, Q., Rosero, R., Rossiter, P., Sazzad, A. B. M. R., Schnee, R. W., Schubnell, M., Seymour, D., Shaw, S., Silk, J. J., Solmaz, M., Solovov, V. N., Sorensen, P., Stancu, I., Stiegler, T. M., Stifter, K., Szydagis, M., Taylor, R., Temples, D., Tiedt, D. R., Tomás, A., Tripathi, M., Tvrznikova, L., Vacheret, A., Webb, R. C., Wolfs, F. L. H., 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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Measurement of the gamma ray background in the Davis cavern at the Sanford Underground Research Facility by Akerib, D. S., Akerlof, C. W., Angelides, N., Araújo, H. M., Bai, X., Boast, K. E., Brás, P., Buckley, J. H., Bugaev, V. V., Carels, C., Carlsmith, D. L., Carmona-Benitez, M. C., Cascella, M., Chan, C., Cole, A., Cutter, J. E., Dobson, J. E. Y., Druszkiewicz, E., Fiorucci, S., Flaecher, H., Fruth, T., Ghag, C., Gokhale, S., van der Grinten, M. G. D., Hall, C. R., Haselschwardt, S. J., Hor, J. Y-K., Horn, M., Ignarra, C. M., Jahangir, O., Ji, W., Johnson, J., Kaboth, A. C., Kamdin, K., Korley, L., Korolkova, E. V., Kraus, H., Kravitz, S. W., Kreczko, L., Krikler, B., Kudryavtsev, V. A., Lesko, K. T., Levy, C., Liao, J., Lindote, A., Liu, R., Liu, X., López Paredes, B., Lorenzon, W., Luitz, S., Lyle, J. M., Manenti, L., Mannino, R. L., Marangou, N., Marzioni, M. F., McKinsey, D. N., McLaughlin, J., Meng, Y., Morad, J. A., Murphy, A. St. J., Naim, D., Naylor, A., Nedlik, C., Nikoleyczik, J., Nilima, A., Olcina, I., Oliver-Mallory, K. C., Pal, S., Palladino, K. J., Pereira, G., Piepke, A., Pushkin, K., Reichenbacher, J., Rhyne, C. A., Riffard, Q., Rosero, R., Rossiter, P., Sazzad, A. B. M. R., Schnee, R. W., Schubnell, M., Seymour, D., Shaw, S., Silk, J. J., Solmaz, M., Solovov, V. N., Sorensen, P., Stancu, I., Stiegler, T. M., Stifter, K., Szydagis, M., Taylor, R., Temples, D., Tiedt, D. R., Tomás, A., Tripathi, M., Tvrznikova, L., Vacheret, A., Webb, R. C., Wolfs, F. L. H., 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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The Design, Implementation, and Performance of the LZ Calibration Systems by Aalbers, J, Amarasinghe, C. S, Anderson, T. J, Angelides, N, Armstrong, J. E, Baker, A, Balashov, S, Bang, J, Bargemann, J. W, Beattie, K, Bhatti, A, Biekert, A, Biesiadzinski, T. P, Birch, H. J, Blockinger, G. M, Brás, P, Burdin, S, Carmona-Benitez, M. C, Chen, H, Cherwinka, J. J, Chin, Y. T, Chott, N. I, Converse, M. V, Dahl, C. E, Delgaudio, J, Dey, S, de Viveiros, L, Dobson, J. E. Y, Eriksen, S. R, Fan, A, Fearon, N. M, Fieldhouse, N, Fiorucci, S, Flaecher, H, Gibbons, R, Gokhale, S, van der Grinten, M. G. D, Haiston, J. J, Han, S, Haselschwardt, S. J, Hernandez, M. A, Hertel, S. A, Huang, D. Q, James, R. S, Khaitan, D, Khurana, I, Kingston, J, Kirk, R, Korley, L, Korolkova, E. V, Kraus, H, Kravitz, S, Kudryavtsev, V. A, Lesko, K. T, Levy, C, Lopes, M. I, Luitz, S, Majewski, P. A, McKinsey, D. N, Miller, E. H, Monte, A, Mount, B. J, Murdy, M, Murphy, A. St. J, Olcina, I, Oliver-Mallory, K. C, Pannifer, N. J, Parveen, N, Penning, B, Pershing, T, Riffard, Q, Rischbieter, G. R. C, Rosero, R, Rynders, D, Sazzad, A. B. M. R, Schnee, R. W, Smith, R, Sorensen, P, Stancu, I, Suerfu, B, Sumner, T. J, Taylor, W. C, Timalsina, M, Tovey, D. R, Trask, M, Tronstad, D. R, Vacheret, A, Vaitkus, A. C, Velan, V, Webb, R. C, Weeldreyer, L, Whitis, T. J, Williams, M, Wisniewski, W. J, Woodford, S, Wright, C. J, Xia, Q, Xiang, X, Xu, J, Yeh, M

“…JINST 19 P08027 (2024) LUX-ZEPLIN (LZ) is a tonne-scale experiment searching for direct dark matter interactions and other rare events. It is located at the…”
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Probing the Scalar WIMP-Pion Coupling with the first LUX-ZEPLIN data by Aalbers, J, Amarasinghe, C. S, Anderson, T. J, Angelides, N, Armstrong, J. E, Baker, A, Balashov, S, Bang, J, Bargemann, J. W, Beattie, K, Bhatti, A, Biekert, A, Biesiadzinski, T. P, Birch, H. J, Bishop, E. J, Blockinger, G. M, Brás, P, Burdin, S, Carmona-Benitez, M. C, Cherwinka, J. J, Chott, N. I, Converse, M. V, Dahl, C. E, Delgaudio, J, Dey, S, Dobson, J. E. Y, Eriksen, S. R, Fan, A, Fearon, N. M, Flaecher, H, Gibbons, R, Gokhale, S, Green, J, vanderGrinten, M. G. D, Haiston, J. J, Haselschwardt, S. J, Hernandez, M. A, Hertel, S. A, Horn, M, Huang, D. Q, Jacquet, E, James, R. S, Johnson, J, Kamaha, A. C, Khaitan, D, Korley, L, Korolkova, E. V, Kraus, H, Kudryavtsev, V. A, Leonard, D. S, Lesko, K. T, Lindote, A, Lopes, M. I, Maupin, C, McKinsey, D. N, McLaughlin, J, Miller, E. H, Monte, A, Monzani, M. E, Morrison, E, Mount, B. J, Murdy, M, Murphy, A. St. J, Naylor, A, Nguyen, A, Nikoleyczik, J. A, Oliver-Mallory, K. C, Palmer, J, Pereira, G, Pershing, T, Reichenbacher, J, Rhyne, C. A, Riffard, Q, Rischbieter, G. R. C, Rosero, R, Rynders, D, Sazzad, A. B. M. R, Shutt, T, Silva, C, Solovov, V. N, Sorensen, P, Stancu, I, Suerfu, B, Sumner, T. J, Taylor, W. C, Timalsina, M, Tong, Z, Tovey, D. R, Trask, M, Tripathi, M, Vacheret, A, Vaitkus, A. C, Wang, A, Wang, J. J, Webb, R. C, Whitis, T. J, Williams, M, Wisniewski, W. J, Wright, C. J, Xu, J

“…Commun Phys 7, 292 (2024) Weakly interacting massive particles (WIMPs) may interact with a virtual pion that is exchanged between nucleons. This interaction…”
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The Data Acquisition System of the LZ Dark Matter Detector: FADR by Aalbers, J, Amarasinghe, C. S, Angelides, N, Armstrong, J. E, Baker, A, Balashov, S, Bang, J, Bargemann, J. W, Bhatti, A, Biekert, A, Biesiadzinski, T. P, Birch, H. J, Brás, P, Buuck, M, Carmona-Benitez, M. C, Chawla, A, Chen, H, Cherwinka, J. J, Dahl, C. E, David, A, de Viveiros, L, Di Felice, L, Ding, C, Fraser, E. D, Fruth, T. M. A, Genovesi, J, Green, J, Hall, C. R, Han, S, Hartigan-O'Connor, E, Haselschwardt, S. J, Hertel, S. A, Heuermann, G, Homenides, G. J, Horn, M, Hunt, D, Jacquet, E, James, R. S, Johnson, J, Kaboth, A. C, Kamaha, A. C, Kannichankandy, M, Khaitan, D, Khazov, A, Kim, J, Kingston, J, Kodroff, D, Kraus, H, Kreczko, L, Lesko, K. T, Lindote, A, Lopes, M. I, Maupin, C, McKinsey, D. N, McLaughlin, J, Mclaughlin, J. B, Miller, E. H, Monte, A, Monzani, M. E, Moongweluwan, M, Mount, B. J, Murdy, M, Murphy, A. St. J, Olcina, I, Olevitch, M. A, Orpwood, J, Palladino, K. J, Pannifer, N. J, Patton, S. J, Perry, E, Qie, Y, Rhyne, C. A, Riyat, H. S, Rushton, T, Santone, D, Sarkis, R, Shutt, T, Silva, C, Sinev, G, Solovov, V. N, Stancu, I, Suerfu, B, Taylor, W. C, Tiedt, D. R, Timalsina, M, Tong, Z, Tranter, J, Trask, M, Tripathi, M, Tronstad, D. R, Velan, V, Wang, Y, Watson, J. R, Weeldreyer, L, Wisniewski, W. J, Wolfs, J. D, Woodford, S, Woodward, D, Xiang, X, Yin, J

“…The Data Acquisition System (DAQ) for the LUX-ZEPLIN (LZ) dark matter detector is described. The signals from 745 PMTs, distributed across three subsystems,…”
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Constraints On Covariant WIMP-Nucleon Effective Field Theory Interactions from the First Science Run of the LUX-ZEPLIN Experiment by Aalbers, J, Amarasinghe, C. S, Anderson, T. J, Angelides, N, Armstrong, J. E, Baker, A, Balashov, S, Bang, J, Bargemann, J. W, Beattie, K, Bhatti, A, Biekert, A, Biesiadzinski, T. P, Birch, H. J, Bishop, E. J, Blockinger, G. M, Brás, P, Burdin, S, Carmona-Benitez, M. C, Chen, H, Cherwinka, J. J, Chin, Y. T, Chott, N. I, Converse, M. V, Dahl, C. E, Delgaudio, J, Dey, S, de Viveiros, L, Dobson, J. E. Y, Eriksen, S. R, Fan, A, Fearon, N. M, Flaecher, H, Gibbons, R, Gokhale, S, Green, J, van der Grinten, M. G. D, Haselschwardt, S. J, Hernandez, M. A, Hertel, S. A, Horn, M, Huang, D. Q, Ignarra, C. M, James, R. S, Khaitan, D, Khurana, I, Korley, L, Korolkova, E. V, Kraus, H, Kudryavtsev, V. A, Lesko, K. T, Levy, C, Lopes, M. I, Luitz, S, Majewski, P. A, McKinsey, D. N, McLaughlin, J. B, Miller, E. H, Monte, A, Mount, B. J, Murdy, M, Murphy, A. St. J, Olcina, I, Oliver-Mallory, K. C, Pannifer, N. J, Parveen, N, Penning, B, Perry, E, Pershing, T, Riffard, Q, Rischbieter, G. R. C, Rosero, R, Rynders, D, Sazzad, A. B. M. R, Schnee, R. W, Smith, R, Sorensen, P, Stancu, I, Suerfu, B, Sumner, T. J, Taylor, W. C, Timalsina, M, Tovey, D. R, Trask, M, Tronstad, D. R, Vacheret, A, Vaitkus, A. C, Velan, V, Webb, R. C, Weeldreyer, L, Whitis, T. J, Williams, M, Wisniewski, W. J, Woodford, S, Wright, C. J, Xia, Q, Xiang, X, Xu, J, Yeh, M, Zweig, E. A

“…The first science run of the LUX-ZEPLIN (LZ) experiment, a dual-phase xenon time project chamber operating in the Sanford Underground Research Facility in…”
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A search for new physics in low-energy electron recoils from the first LZ exposure by Aalbers, J, Alder, F, Amarasinghe, C. S, Ames, A, Anderson, T. J, Angelides, N, Araújo, H. M, Armstrong, J. E, Bargemann, J. W, Baxter, A, Beattie, K, Blockinger, G. M, Brew, C. A. J, Brás, P, Buuck, M, Carmona-Benitez, M. C, Chan, C, Chawla, A, Chen, H, Cherwinka, J. J, Chott, N. I, Converse, M. V, Dahl, C. E, Delgaudio, J, Dey, S, de Viveiros, L, Dobson, J. E. Y, Eriksen, S. R, Fearon, N. M, Flaecher, H, Fruth, T. M. A, Gaitskell, R. J, Geffre, A, Gibbons, R, Green, J, Hall, C. R, Han, S, Hartigan-O'Connor, E, Hertel, S. A, Heuermann, G, Jahangir, O, Kaboth, A. C, Khurana, I, Kirk, R, Korley, L, Korolkova, E. V, Kraus, H, Kravitz, S, Krikler, B, Kudryavtsev, V. A, Leason, E. A, Lee, J, Leonard, D. S, Linehan, R, Lippincott, W. H, Liu, X, Asamar, E. Lopez, Luitz, S, Majewski, P. A, McKinsey, D. N, Mizrachi, E, Monte, A, Monzani, M. E, Mendoza, J. D. Morales, Morrison, E, Mount, B. J, Murphy, A. St. J, Naylor, A, Olcina, I, Oliver-Mallory, K. C, Pereira, G, Pershing, T, Rischbieter, G. R. C, Rosero, R, Rynders, D, Sazzad, A. B. M. R, Schnee, R. W, Solovov, V. N, Sorensen, P, Stancu, I, Suerfu, B, Sumner, T. J, Taylor, W. C, Temples, D. J, Timalsina, M, Tovey, D. R, Trask, M, Tronstad, D. R, Turner, W, Vacheret, A, Vaitkus, A. C, Wang, A, Wang, J. J, Webb, R. C, Whitis, T. J, Williams, M, Wisniewski, W. J, Woodward, D, Wright, C. J, Xu, J

“…Phys. Rev. D 108, 072006 (2023) The LUX-ZEPLIN (LZ) experiment is a dark matter detector centered on a dual-phase xenon time projection chamber. We report…”
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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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Background Determination for the LUX-ZEPLIN (LZ) Dark Matter Experiment by Aalbers, J, Alsum, S. K, Amarasinghe, C. S, Ames, A, Angelides, N, Araújo, H. M, Armstrong, J. E, Bang, J, Beattie, K, Biesiadzinski, T. P, Birch, H. J, Blockinger, G. M, Brás, P, Burdin, S, Cabrita, R, Carmona-Benitez, M. C, Chan, C, Chawla, A, Chen, H, Chott, N. I, Converse, M. V, Dahl, C. E, Dey, S, de Viveiros, L, Ding, C, Dobson, J. E. Y, Druszkiewicz, E, Fiorucci, S, Fraser, E. D, Gaitskell, R. J, Genovesi, J, Ghag, C, Gilchriese, M. G. D, Gwilliam, C. B, Hall, C. R, Han, S, Hartigan-O'Connor, E, Heuermann, G, Huang, D. Q, Jahangir, O, James, R. S, Johnson, J, Kaboth, A. C, Kamaha, A. C, Khurana, I, Kodroff, D, Kudryavtsev, V. A, Levy, C, Lin, J, Lorenzon, W, Marangou, N, McCarthy, M. E, McLaughlin, J, Miller, E. H, Mount, B. J, Murdy, M, Naim, D, Nedlik, C, Nelson, H. N, Nguyen, A, Nikoleyczik, J. A, Orpwood, J, Palladino, K. J, Parveen, N, Patton, S. J, Penning, B, Perry, E, Piepke, A, Poudel, S, Reichenbacher, J, Rhyne, C. A, Riffard, Q, Rosero, R, Rossiter, P, Santone, D, Sazzad, A. B. M. R, Shutt, T, Silva, C, Sinev, G, Solmaz, M, Solovov, V. N, Stancu, I, Stevens, A, Suerfu, B, Sumner, T. J, Taylor, R, Taylor, W. C, Temples, D. J, Tiedt, D. R, Tong, Z, Tovey, D. R, Utku, U, Wang, Y, Watson, J. R, Whitis, T. J, Woodford, S, Wright, C. J, Xia, Q, Xiang, X, Yeh, M

“…Phys. Rev. D 108, 012010 (2023) The LUX-ZEPLIN experiment recently reported limits on WIMP-nucleus interactions from its initial science run, down to…”
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Cosmogenic production of $^{37}$Ar in the context of the LUX-ZEPLIN experiment by Aalbers, J, Alsum, S. K, Amarasinghe, C. S, Ames, A, Angelides, N, Araújo, H. M, Armstrong, J. E, Balashov, S, Bang, J, Bernard, E. P, Bhatti, A, Biekert, A, Birch, H. J, Bodnia, E, Boxer, B, Brew, C. A. J, Busenitz, J. K, Cabrita, R, Carmona-Benitez, M. C, Cascella, M, Chawla, A, Chen, H, Chott, N. I, Cole, A, Converse, M. V, Cutter, J. E, de Viveiros, L, Druszkiewicz, E, Fayer, S, Fearon, N. M, Fraser, E. D, Gaitskell, R. J, Genovesi, J, Ghag, C, Gilchriese, M. G. D, van der Grinten, M. G. D, Gwilliam, C. B, Haselschwardt, S. J, Horn, M, Hunt, D, Ignarra, C. M, James, R. S, Ji, W, Johnson, J, Kamaha, A. C, Khaitan, D, Kodroff, D, Korley, L, Kravitz, S, Kreczko, L, Kudryavtsev, V. A, Leason, E. A, Levy, C, Linehan, R, Lippincott, W. H, Liu, X, Asamar, E. Lopez, Manenti, L, Marangou, N, McKinsey, D. N, McLaughlin, J, Mizrachi, E, Monzani, M. E, Morad, J. A, Mendoza, J. D. Morales, Naim, D, Naylor, A, Nikoleyczik, J. A, Nilima, A, Oliver-Mallory, K, Pal, S, Palmer, J, Patton, S. J, Pereira, G, Pershing, J, Porzio, D, Richards, A, Schnee, R. W, Shutt, T. A, Silk, J. J, Silva, C, Sinev, G, Smith, R, Solmaz, M, Soria, J, Stevens, A, Stifter, K, Swanson, N, Szydagis, M, Taylor, R, Temples, D. J, Timalsina, M, To, W. H, Tovey, D. R, Trask, M, Utku, U, Wang, B, Whitis, T. J, Woodward, D, Xia, Q

“…We estimate the amount of $^{37}$Ar produced in natural xenon via cosmic ray-induced spallation, an inevitable consequence of the transportation and storage of…”
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The LUX-ZEPLIN (LZ) radioactivity and cleanliness control programs by Akerib, D. S, Alquahtani, A, Alsum, S. K, Armstrong, J. E, Aviles, S, Bang, J, Bauer, D, Bauer, P, Belle, J, Bernard, E. P, Biekert, A, Birch, H. J, Bramante, R, Bugaev, V. V, Campbell, J. S, Carels, C, Carlsmith, D. L, Carlson, B, Cascella, M, Chiller, A. A, Chott, N. I, Cox, G, Currie, A, Druszkiewicz, E, Edberg, T. K, Emmet, W. T, Fayer, S, Flaecher, H, Francis, V. B, Gerhard, R. M, Ghag, C, Gilchriese, M. G. D, Gomber, B, Gonda, T. G, Greenall, A, van der Grinten, M. G. D, Hall, C. R, Harrington, T, Hasselkus, C, Haselschwardt, S. J, Hillbrand, S, Irving, M. N, Jahangir, O, Kasey, V, Kazkaz, K, Khaitan, D, Khaleeq, M, Khazov, A, Khurana, I, Kras, J, Kreczko, L, Krikler, B, Kyre, S, Lenardo, B. G, Leonard, D. S, Li, J, Liao, F. -T, Linehan, R, Lippincott, W. H, Liu, X, Lorenzon, W, Lyle, J. M, Majewski, P. A, Makkinje, J, Manenti, L, Marangou, N, Mizrachi, E, Mock, J, Naylor, A, Nedlik, C, Nehrkorn, C, Nelson, H. N, O'Dell, J, Oliver-Mallory, K. C, Pangilinan, M, Pereira, G, Pereira, C, Powell, S, Preece, R. M, Sabarots, L, Scovell, P. R, Skulski, W, Smith, R. E, So, J, Sorensen, P, Swanson, N, Timalsina, M, Tripathi, M, Tull, C. E, Verbus, J. R, Voirin, E, Waldron, W. L, Wang, W, Watson, J. R, Weatherly, S, White, J. T, White, D. T, Wisniewski, W. J, Xu, J, Zhang, C

“…The European Physical Journal C, Volume 80, Article number: 1044 (2020) LUX-ZEPLIN (LZ) is a second-generation direct dark matter experiment with…”
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Projected sensitivity of the LUX-ZEPLIN (LZ) experiment to the two-neutrino and neutrinoless double beta decays of $^{134}$Xe by Collaboration, Alsum, S. K, Amarasinghe, C. S, Ames, A, Araujo, H. M, Armstrong, J. E, Arthurs, M, Bai, X, Balashov, S, Bang, J, Beltrame, P, Bernard, E. P, Bhatti, A, Biekert, A, Biesiadzinski, T. P, Birch, H. J, Blockinger, G. M, Bodnia, E, Boxer, B, Bras, P, Busenitz, J. K, Carmona-Benitez, M. C, Cascella, M, Cole, A, Converse, M. V, Cottle, A, Dahl, C. E, Eriksen, S. R, Fan, A, Fayer, S, Fiorucci, S, Fraser, E. D, Fruth, T, Gokhale, S, van der Grinten, M. G. D, Huang, D. Q, Ignarra, C. M, James, R. S, Ji, W, Kaboth, A. C, Kamaha, A. C, Kazkaz, K, Khurana, I, Kodroff, D, Kudryavtsev, V. A, Levy, C, Liao, J, Lin, J, Lippincott, W. H, Asamar, E. Lopez, Paredes, B. Lopez, Manenti, L, Mannino, R. L, Marangou, N, McLaughlin, J, Miller, E. H, Mizrachi, E, Mendoza, J. D. Morales, Naim, D, Nedlik, C, Nelson, H. N, Nikoleyczik, J. A, Nilima, A, Oliver-Mallory, K. C, Pal, S, Palladino, K. J, Palmer, J, Patton, S, Parveen, N, Penning, B, Pereira, G, Piepke, A, Qie, Y, Riffard, Q, Rossiter, P, Sazzad, A. B. M. R, Schnee, R. W, Scovell, P. R, Shaw, S, Shutt, T. A, Silk, J. J, Silva, C, Smith, R, Sorensen, P, Soria, J, Stifter, K, Swanson, N, Terman, P. A, Timalsina, M, To, W. H, Tovey, D. R, Tripathi, M, Tronstad, D. R, Utku, U, Vaitkus, A, Wang, B, Wang, J. J, Watson, J. R, White, R. G, Wright, C. J

“…The projected sensitivity of the LUX-ZEPLIN (LZ) experiment to two-neutrino and neutrinoless double beta decay of $^{134}$Xe is presented. LZ is a 10-tonne…”
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