Search Results - "Hjemfelt, C."

Projected WIMP sensitivity of the LUX-ZEPLIN (LZ) dark matter experiment by Akerib, D. S, Araújo, H. M, Arthurs, M, Bailey, A. J, Balajthy, J, Bauer, D, Belle, J, Benson, T, Bernard, E. P, Biesiadzinski, T. P, Boast, K. E, Boxer, B, Brás, P, Carels, C, Carlsmith, D. L, Carlson, B, Carmona-Benitez, M. C, Chan, C, Cottle, A, Currie, A, Dahl, C. E, Druszkiewicz, E, Fayer, S, Fiorucci, S, Fruth, T, Gaitskell, R. J, Ghag, C, Gilchriese, M. G. D, van der Grinten, M. G. D, Hanzel, K, Haselschwardt, S. J, Hjemfelt, C, Huang, D. Q, Ignarra, C. M, Ji, W, Kamdin, K, Khaitan, D, Kim, Y. D, Kocher, C. D, Korolkova, E. V, Krebs, H. J, Krikler, B, Kudryavtsev, V. A, Kyre, S, Lenardo, B. G, Li, J, Liao, F. -T, Lindote, A, Linehan, R, Lippincott, W. H, Liu, X, Lopes, M. I, Paredes, B. López, Lorenzon, W, Majewski, P, Manalaysay, A, McKinsey, D. N, Monzani, M. E, Morad, J. A, Mount, B. J, Murphy, A. St. J, Nikoleyczik, J, Olevitch, M. A, Palladino, K. J, Patton, S. J, Penning, B, Piepke, A, Preece, R. M, Ratcliff, B. N, Reichenbacher, J, Rhyne, C. A, Rodrigues, J. P, Saba, J. S, Sarychev, M, Schnee, R. W, Scovell, P. R, Shaw, S, Shutt, T. A, Silk, J. J, Silva, C, Solmaz, M, Solovov, V. N, Stark, M. R, Stiegler, T. M, Taylor, W. C, Taylor, D. J, Terman, P. A, Timalsina, M, To, W. H, Tomás, A, Tope, T. E, Tripathi, M, Utku, U, Vacheret, A, Webb, R. C, Whitis, T. J, Woodward, D, Worm, S. D, Yeh, M, Young, I

“…Phys. Rev. D 101, 052002 (2020) LUX-ZEPLIN (LZ) is a next generation dark matter direct detection experiment that will operate 4850 feet underground at the…”
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Identification of Radiopure Titanium for the LZ Dark Matter Experiment and Future Rare Event Searches by Akerib, D. S, Akerlof, C. W, Akimov, D. Yu, Araújo, H. M, Arnquist, I. J, Bai, X, Bailey, A. J, Balashov, S, Belle, J, Beltrame, P, Benson, T, Bernard, E. P, Boast, K. E, Bolozdynya, A, Bramante, R, Brás, P, Burdin, S, Busenitz, J. K, Carlsmith, D. L, Carmona-Benitez, M. C, Cherwinka, J. J, Chiller, A. A, Cottle, A, Coughlen, R, Currie, A, Dahl, C. E, Davison, T. J. R, Dobi, A, Emmet, W. T, Fiorucci, S, Fruth, T, Gantos, N. J, Ghag, C, Gomber, B, Hall, C. R, Haselschwardt, S. J, Hillbrand, S, Hoff, M. D, Holtom, E, Hoppe, E. W, Huang, D. Q, Hurteau, T. W, Kaboth, A, Konovalov, A. M, Koyuncu, M, Kyre, S, Lee, J, Lindote, A, Lippincott, W. H, Liu, X, Lopes, M. I, Paredes, B. Lopez, Majewski, P, Manenti, L, Markley, D. J, Martin, T. J, Marzioni, M. F, McConnell, C. T, McKinsey, D. N, Miller, E. H, Mock, J, Mount, B. J, Murphy, A. St. J, Nehrkorn, C, Nelson, H. N, Olevitch, M. A, Oliver-Mallory, K. C, Pease, E. K, Powell, S, Preece, R. M, Rodrigues, J. P, Rossiter, P, Saba, J. S, Sarychev, M, Schnee, R. W, Scovell, P. R, Shaw, S, Shutt, T. A, Silva, C, Skulski, W, Solovov, V. N, Szydagis, M, Taylor, D. J, Taylor, W. C, Temples, D, Thomas, K. J, Tiedt, D. R, Tomás, A, Tope, T. E, Tvrznikova, L, Va'vra, J, Vuosalo, C. O, Waldron, W. L, While, M, White, D. T, Wolfs, F. L. H, Woodward, D, 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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LUX-ZEPLIN (LZ) Technical Design Report by Huang, D. Q, Malling, D. C, Leonard, D. S, Cottle, A, Lippincott, W. H, Martin, T. J, Sarychev, M, Khaleeq, M, Olcina, I, Richards, A, Vacheret, A, Brás, P, Neves, F, Rodrigues, J. P, Silva, C, Cole, A, Dobi, A, Gantos, N. J, Gilchriese, M. G. D, Patton, S. J, Saba, J. S, Waldron, W. L, Kazkaz, K, Xu, J, Auyeung, H, Biesiadzinski, T. P, Breidenbach, M, Bramante, R, Fan, A, Hau, A, Linehan, R, Luitz, S, Ratcliff, B. N, To, W. H, Whitis, T. J, Wisniewski, W. J, Bai, X, Bunker, R, Coughlen, R, Leonard, R, Reichenbacher, J, Sundarnath, K, Keefner, J, Maupin, C, Khazov, A, Majewski, P, Nikkel, J. A, O'Dell, J, Preece, R. M, van der Grinten, M. G. D, Worm, S. D, Mock, J, Szydagis, M, Busenitz, J. K, Elnimr, M, Stancu, I, Kreczko, L, Krikler, B, Penning, B, Bernard, E. P, Gerhard, R. M, Hemer, D, Manalaysay, A. G, Morad, J. A, Uvarov, S, Kyre, S, Dobson, J. E. Y, Ghag, C, Shaw, S, Utku, U, Nilima, A, Burdin, S, Balajthy, J, Edberg, T. K, Silk, J. S, Arthurs, M, Carels, C, Lin, J, Scovell, P. R, Khaitan, D, Koyuncu, M, Skulski, W, Wolfs, F. L. H, Woodward, D, Chiller, A. A, Chiller, C, Wang, L, Wei, W. -Z, Zhang, C, Alsum, S. K, Benson, T, Carlsmith, D. L, Gregerson, G, Pagac, A, Palladino, K. J, Buckley, J. H, Bugaev, V. V, Olevitch, M. A, Emmet, W. T, Larsen, N. A

“…In this Technical Design Report (TDR) we describe the LZ detector to be built at the Sanford Underground Research Facility (SURF). The LZ dark matter…”
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