Search Results - "Leason, E"

QUEST-DMC superfluid 3He detector for sub-GeV dark matter by Autti, S., Casey, A., Eng, N., Darvishi, N., Franchini, P., Haley, R. P., Heikkinen, P. J., Jennings, A., Kemp, A., Leason, E., Levitin, L. V., Monroe, J., March-Russel, J., Noble, M. T., Prance, J. R., Rojas, X., Salmon, T., Saunders, J., Smith, R., Thompson, M. D., Tsepelin, V., West, S. M., Whitehead, L., Zavjalov, V. V., Zmeev, D. E.

“…The focus of dark matter searches to date has been on Weakly Interacting Massive Particles (WIMPs) in the GeV/ c 2 -TeV/ c 2 mass range. The direct, indirect…”
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QUEST-DMC superfluid $$^3$$He detector for sub-GeV dark matter by Autti, S., Casey, A., Eng, N., Darvishi, N., Franchini, P., Haley, R. P., Heikkinen, P. J., Jennings, A., Kemp, A., Leason, E., Levitin, L. V., Monroe, J., March-Russel, J., Noble, M. T., Prance, J. R., Rojas, X., Salmon, T., Saunders, J., Smith, R., Thompson, M. D., Tsepelin, V., West, S. M., Whitehead, L., Zavjalov, V. V., Zmeev, D. E.

“…Abstract The focus of dark matter searches to date has been on Weakly Interacting Massive Particles (WIMPs) in the GeV/ $$c^2$$ c 2 -TeV/ $$c^2$$ c 2 mass…”
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QUEST-DMC: Background Modelling and Resulting Heat Deposit for a Superfluid Helium-3 Bolometer by Autti, S., Casey, A., Eng, N., Darvishi, N., Franchini, P., Haley, R. P., Heikkinen, P. J., Kemp, A., Leason, E., Levitin, L. V., Monroe, J., March-Russel, J., Noble, M. T., Prance, J. R., Rojas, X., Salmon, T., Saunders, J., Smith, R., Thompson, M. D., Tsepelin, V., West, S. M., Whitehead, L., Zhang, K., Zmeev, D. E.

“…We report the results of radioactivity assays and heat leak calculations for a range of common cryogenic materials, considered for use in the QUEST-DMC…”
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QUEST-DMC superfluid $$^3$$ 3 He detector for sub-GeV dark matter by QUEST-DMC collaboration, S. Autti, A. Casey, N. Eng, N. Darvishi, P. Franchini, R. P. Haley, P. J. Heikkinen, A. Jennings, A. Kemp, E. Leason, L. V. Levitin, J. Monroe, J. March-Russel, M. T. Noble, J. R. Prance, X. Rojas, T. Salmon, J. Saunders, R. Smith, M. D. Thompson, V. Tsepelin, S. M. West, L. Whitehead, V. V. Zavjalov, D. E. Zmeev

“…Abstract The focus of dark matter searches to date has been on Weakly Interacting Massive Particles (WIMPs) in the GeV/ $$c^2$$ c 2 -TeV/ $$c^2$$ c 2 mass…”
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The LUX-ZEPLIN (LZ) experiment by Akerlof, C. W., Akimov, D. Yu, Alquahtani, A., Armstrong, J. E., Arthurs, M., Bang, J., Bauer, P., Baxter, A., Belle, J., Beltrame, P., Birrittella, B., Boast, K. E., Boxer, B., Bramante, R., Breidenbach, M., Buckley, J. H., Bugaev, V. V., Burdin, S., Carels, C., Cascella, M., Cherwinka, J. J., Chiller, A. A., Conley, R. A., Cottle, A., Coughlen, R., Craddock, W. W., Currie, A., Cutter, J. E., Edwards, B. N., Emmet, W. T., Faham, C. H., Fayer, S., Fogarty Florang, I. M., Francis, V. B., Fruth, T., Ghag, C., Gibson, E., Gokhale, S., Gonda, T. G., Greenwood, S., Hans, S., Hasselkus, C., Hertel, S. A., Hoff, M. D., Huang, D. Q., Jacobsen, R. G., Jeffery, S. N., Ji, W., Kamaha, A., Kocher, C. D., Koyuncu, M., Krebs, H. J., Larsen, N. A., Lee, H. S., Li, J., Lindote, A., Lynch, C., Manenti, L., Markley, D. J., Mei, D. -M., Molash, D., Morad, J. A., Murphy, A. St. J., Naim, D., Nedlik, C., O’Dell, J., Oh, H., O’Neill, F. G., Pagenkopf, D., Penning, B. P., Powell, S., Rose, H. J., Rucinski, R., Rutherford, G., Sabarots, L., Schnee, R. W., Seymour, D., Shaw, S., Skarpaas, K., Skulski, W., Sosnovtsev, V. V., Stark, M. R., Stern, N., Sumner, T. J., Sundarnath, K., Tennyson, B. P., Timalsina, M., To, W. H., Uvarov, S., Verbus, J. R., Walker, K., Watson, J. R., Weatherly, S., White, D. T., Wilson, K., Witherell, M. S., Xiang, X., Xiao, Q., Young, I., Zhang, C.

“…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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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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QUEST-DMC: Background Modelling and Resulting Heat Deposit for a Superfluid Helium-3 Bolometer by Autti, S, Casey, A, Eng, N, Darvishi, N, Franchini, P, Haley, R. P, Heikkinen, P. J, Kemp, A, Leason, E, Levitin, L. V, Monroe, J, March-Russel, J, Noble, M. T, Prance, J. R, Rojas, X, Salmon, T, Saunders, J, Smith, R, Thompson, M. D, Tsepelin, V, West, S. M, Whitehead, L, Zhang, K, Zmeev, D. E

“…Journal of Low Temperature Physics, Special Issue: Quantum Fluids and Solids (QFS2023) We report the results of radioactivity assays and heat leak calculations…”
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QUEST-DMC superfluid $^3$He detector for sub-GeV dark matter by Autti, S, Casey, A, Eng, N, Darvishi, N, Franchini, P, Haley, R. P, Heikkinen, P. J, Jennings, A, Kemp, A, Leason, E, Levitin, L. V, Monroe, J, March-Russel, J, Noble, M. T, Prance, J. R, Rojas, X, Salmon, T, Saunders, J, Smith, R, Thompson, M. D, Tsepelin, V, West, S. M, Whitehead, L, Zavjalov, V. V, Zmeev, D. E

“…Eur. Phys. J. C (2024) 84:248 The focus of dark matter searches to date has been on Weakly Interacting Massive Particles (WIMPs) in the GeV/$c^2$-TeV/$c^2$…”
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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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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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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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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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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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Constraints on Effective Field Theory Couplings Using 311.2 days of LUX Data by 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, 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, Xiang, X, Xu, J, Zhang, C

“…Phys. Rev. D 104, 062005 (2021) We report here the results of an Effective Field Theory (EFT) WIMP search analysis using LUX data. We build upon previous LUX…”
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Projected sensitivities of the LUX-ZEPLIN (LZ) experiment to new physics via low-energy electron recoils by Amarasinghe, C. S, Anderson, T. J, Angelides, N, Armstrong, J. E, Balajthy, J, Bargemann, J. W, Baxter, A, Beltrame, P, Bernstein, A, Biekert, A, Blockinger, G. M, Boxer, B, Brew, C. A. J, Brás, P, Burdin, S, Buuck, M, Cabrita, R, Carmona-Benitez, M. C, Cascella, M, Chan, C, Chott, N. I, Cottle, A, Cox, G, Creaner, O, de Viveiros, L, Dobson, J. E. Y, Eriksen, S. R, Fearon, N. M, Flaecher, H, Gibson, E, Gwilliam, C. B, Hall, C. R, Hardy, C. A, Horn, M, Ignarra, C. M, James, R. S, Ji, W, Kazkaz, K, Khaitan, D, Khurana, I, Kodroff, D, Kravitz, S, Kreczko, L, Leason, E. A, Leonard, D. S, Lesko, K. T, Levy, C, Li, J, Liao, J, Liu, X, Lorenzon, W, Manalaysay, A, Marangou, N, McCarthy, M. E, McLaughlin, J, Miller, E. H, Monzani, M. E, Morad, J. A, Mendoza, J. D. Morales, Naim, D, Nedlik, C, Nelson, H. N, Nguyen, 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

“…LUX-ZEPLIN (LZ) is a dark matter detector expected to obtain world-leading sensitivity to weakly interacting massive particles (WIMPs) interacting via nuclear…”
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Enhancing the sensitivity of the LUX-ZEPLIN (LZ) dark matter experiment to low energy signals by Akerib, D. S, Ames, A, Anderson, T. J, Araújo, H. M, Armstrong, J. E, Arthurs, M, Bai, X, Balashov, S, Bang, J, Bauer, D, Baxter, A, Beltrame, P, Bernard, E. P, Bernstein, A, Biekert, A, Biesiadzinski, T. P, Birch, H. J, Blockinger, G. M, Boxer, B, Brew, C. A. J, Buuck, M, Cabrita, R, Cascella, M, Chan, C, Chott, N. I, Cole, A, Cox, G, Cutter, J. E, Dobson, J. E. Y, Druszkiewicz, E, Flaecher, H, Fruth, T, Genovesi, J, Ghag, C, Gokhale, S, Haselschwardt, S. J, Huang, D. Q, Ignarra, C. M, James, R. S, Ji, W, Kaboth, A. C, Kazkaz, K, Khaitan, D, Khazov, A, Kodroff, D, Korolkova, E. V, Kraus, H, Kudryavtsev, V. A, Levy, C, Li, J, Lin, J, Paredes, B. López, Lorenzon, W, Majewski, P. A, Manalaysay, A, Mannino, R. L, McKinsey, D. N, Mizrachi, E, Morad, J. A, Mendoza, J. D. Morales, Morrison, E, Mount, B. J, Naim, D, Nedlik, C, Nikoleyczik, J. A, Oliver-Mallory, K. C, Pal, S, Palmer, J, Pease, E. K, Penning, B, Pereira, G, Reichenbacher, J, Richards, A, Riffard, Q, Rischbieter, G. R. C, Sazzad, A. B. M. R, Scovell, P. R, Shutt, T. A, Silk, J. J, Silva, C, Solovov, V. N, Sorensen, P, Stancu, I, Stifter, K, Sumner, T. J, Swanson, N, Szydagis, M, Taylor, W. C, Taylor, R, Terman, P. A, Tiedt, D. R, Timalsina, M, To, W. H, Tripathi, M, Wang, B, White, R. G, Williams, M, Woodward, D, Xiang, X, Xu, J

“…Two-phase xenon detectors, such as that at the core of the forthcoming LZ dark matter experiment, use photomultiplier tubes to sense the primary (S1) and…”
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