Zobrazeno 1 - 10
of 64
pro vyhledávání: '"Chapman, JJ"'
Autor:
Malling, DC, Akerib, DS, Araujo, HM, Bai, X, Bedikian, S, Bernard, E, Bernstein, A, Bradley, A, Cahn, SB, Carmona-Benitez, MC, Carr, D, Chapman, JJ, Clark, K, Classen, T, Coffey, T, Curioni, A, Currie, A, Dazeley, S, Viveiros, LD, Dragowsky, M, Druszkiewicz, E, Faham, CH, Fiorucci, S, Gaitskell, RJ, Gibson, KR, Hall, C, Hanhardt, M, Holbrook, B, Ihm, M, Jacobsen, RG, Kastens, L, Kazkaz, K, Lander, R, Larsen, N, Lee, C, Leonard, D, Lesko, K, Lindote, A, Lopes, MI, Lyashenko, A, Majewski, P, Mannino, R, McKinsey, DN, Mei, D-M, Mock, J, Morii, M, Murphy, ASJ, Nelson, H, Neves, F, Nikkel, JA, Pangilinan, M, Phelps, P, Reichhart, L, Shutt, T, Silva, C, Skulski, W, Solovov, V, Sorensen, P, Spaans, J, Stiegler, T, Sumner, TJ, Svoboda, R, Sweany, M, Szydagis, M, Thomson, J, Tripathi, M, Verbus, JR, Walsh, N, Webb, R, White, JT, Wlasenko, M, Wolfs, FLH, Woods, M, Zhang, C
Publikováno v:
Malling, DC; Akerib, DS; Araujo, HM; Bai, X; Bedikian, S; Bernard, E; et al.(2018). After LUX: The LZ Program. UC Berkeley: Retrieved from: http://www.escholarship.org/uc/item/40j7t8n6
The LZ program consists of two stages of direct dark matter searches using liquid Xe detectors. The first stage will be a 1.5-3 tonne detector, while the last stage will be a 20 tonne detector. Both devices will benefit tremendously from research and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::aa2102b1552aad8201caa036dc46c74a
http://www.escholarship.org/uc/item/40j7t8n6
http://www.escholarship.org/uc/item/40j7t8n6
Autor:
Szydagis, M, Akerib, DS, Araujo, HM, Bai, X, Bailey, AJ, Balajthy, J, Bernard, E, Bernstein, A, Bradley, A, Byram, D, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chapman, JJ, Chiller, AA, Chiller, C, Coffey, T, Currie, A, Viveiros, L de, Dobi, A, Dobson, J, Druszkiewicz, E, Edwards, B, Faham, CH, Fiorucci, S, Flores, C, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, C, Hertel, SA, Horn, M, Huang, DQ, Ihm, M, Jacobsen, RG, Kazkaz, K, Knoche, R, Larsen, NA, Lee, C, Lindote, A, Lopes, MI, Malling, DC, Mannino, R, McKinsey, DN, Mei, D-M, Mock, J, Moongweluwan, M, Morad, J, Murphy, A St J, Nehrkorn, C, Nelson, H, Neves, F, Ott, RA, Pangilinan, M, Parker, PD, Pease, EK, Pech, K, Phelps, P, Reichhart, L, Shutt, T, Silva, C, Solovov, VN, Sorensen, P, O'Sullivan, K, Sumner, T, Taylor, D, Tennyson, B, Tiedt, DR, Tripathi, M, Uvarov, S, Verbus, JR, Walsh, N, Webb, R, White, JT, Witherell, MS, Wolfs, FLH, Woods, M, Zhang, C
Publikováno v:
Szydagis, M; Akerib, DS; Araujo, HM; Bai, X; Bailey, AJ; Balajthy, J; et al.(2018). A Detailed Look at the First Results from the Large Underground Xenon (LUX) Dark Matter Experiment. UC Berkeley: Retrieved from: http://www.escholarship.org/uc/item/5j70x745
LUX, the world's largest dual-phase xenon time-projection chamber, with a fiducial target mass of 118 kg and 10,091 kg-days of exposure thus far, is currently the most sensitive direct dark matter search experiment. The initial null-result limit on t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9ef9f916cb78e29be1ed3dbef103c5a4
http://www.escholarship.org/uc/item/5j70x745
http://www.escholarship.org/uc/item/5j70x745
Autor:
Collaboration, LUX, Akerib, DS, Alsum, S, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Beltrame, P, Bernard, EP, Bernstein, A, Biesiadzinski, TP, Whitis, TJ, Witherell, MS, Wolfs, FLH, Xu, J, Yazdani, K, Young, SK, Zhang, C, Boulton, EM, Bradley, A, Bramante, R, Brás, P, Byram, D, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chapman, JJ, Chiller, AA, Chiller, C, Currie, A, Cutter, JE, Davison, TJR, Viveiros, LD, Dobi, A, Dobson, JEY, Druszkiewicz, E, Edwards, BN, Faham, CH, Fiorucci, S, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, CR, Hanhardt, M, Haselschwardt, SJ, Hertel, SA, Hogan, DP, Horn, M, Huang, DQ, Ignarra, CM, Ihm, M, Jacobsen, RG, Ji, W, Kamdin, K, Kazkaz, K, Khaitan, D, Knoche, R, Larsen, NA, Lee, C, Lenardo, BG, Lesko, KT, Lindote, A, Lopes, MI, Malling, DC, Manalaysay, A, Mannino, RL, Marzioni, MF, McKinsey, DN, Mei, DM, Mock, J, Moongweluwan, M, Morad, JA, Murphy, ASJ, Nehrkorn, C, Nelson, HN, Neves, F, O'Sullivan, K, Oliver-Mallory, KC, Palladino, KJ, Pangilinan, M, Pease, EK, Phelps, P, Reichhart, L, Rhyne, CA, Shaw, S, Shutt, TA, Silva, C, Solmaz, M, Solovov, VN, Sorensen, P, Stephenson, S, Sumner, TJ, Szydagis, M, Taylor, DJ, Taylor, WC, Tennyson, BP, Terman, PA, Tiedt, DR, To, WH, Tripathi, M, Tvrznikova, L, Uvarov, S, Verbus, JR, Webb, RC, White, JT
The Large Underground Xenon (LUX) experiment is a dual-phase liquid xenon time projection chamber (TPC) operating at the Sanford Underground Research Facility in Lead, South Dakota. A calibration of nuclear recoils in liquid xenon was performed $\tex
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______1032::67b365e6fb3530582546147a4d4fa720
http://hdl.handle.net/10044/1/71453
http://hdl.handle.net/10044/1/71453
Autor:
Akerib, DS, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Beltrame, P, Bernard, EP, Bernstein, A, Biesiadzinski, TP, Boulton, EM, Bradley, A, Bramante, R, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chapman, JJ, Chiller, AA, Chiller, C, Currie, A, Cutter, JE, Davison, TJR, de Viveiros, L, Dobi, A, Dobson, JEY, Druszkiewicz, E, Edwards, BN, Faham, CH, Fiorucci, S, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, CR, Hanhardt, M, Haselschwardt, SJ, Hertel, SA, Hogan, DP, Horn, M, Huang, DQ, Ignarra, CM, Ihm, M, Jacobsen, RG, Ji, W, Kazkaz, K, Khaitan, D, Knoche, R, Larsen, NA, Lee, C, Lenardo, BG, Lesko, KT, Lindote, A, Lopes, MI, Malling, DC, Manalaysay, AG, Mannino, RL, Marzioni, MF, McKinsey, DN, Mei, D-M, Mock, J, Moongweluwan, M, Morad, JA, Murphy, A St J, Nehrkorn, C, Nelson, HN, Neves, F, O׳Sullivan, K, Oliver-Mallory, KC, Ott, RA, Palladino, KJ, Pangilinan, M, Pease, EK, Phelps, P, Reichhart, L, Rhyne, C, Shaw, S, Shutt, TA, Silva, C, Skulski, W, Solovov, VN, Sorensen, P, Stephenson, S, Sumner, TJ, Szydagis, M, Taylor, DJ, Taylor, W, Tennyson, BP, Terman, PA, Tiedt, DR, To, WH, Tripathi, M, Tvrznikova, L, Uvarov, S, Verbus, JR, Webb, RC, White, JT, Whitis, TJ, Witherell, MS, Wolfs, FLH, Yin, J
LUX is a two-phase (liquid/gas) xenon time projection chamber designed to detect nuclear recoils resulting from interactions with dark matter particles. Signals from the detector are processed with an FPGA-based digital trigger system that analyzes t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::0ded47f9c2fdfc9a2aaae02e8dfe2a29
https://escholarship.org/uc/item/2w63c8cm
https://escholarship.org/uc/item/2w63c8cm
Autor:
Akerib, DS, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Beltrame, P, Bernard, EP, Bernstein, A, Biesiadzinski, TP, Boulton, EM, Bradley, A, Bramante, R, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chapman, JJ, Chiller, AA, Chiller, C, Currie, A, Cutter, JE, Davison, TJR, De Viveiros, L, Dobi, A, Dobson, JEY, Druszkiewicz, E, Edwards, BN, Faham, CH, Fiorucci, S, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, CR, Hanhardt, M, Haselschwardt, SJ, Hertel, SA, Hogan, DP, Horn, M, Huang, DQ, Ignarra, CM, Ihm, M, Jacobsen, RG, Ji, W, Kazkaz, K, Khaitan, D, Knoche, R, Larsen, NA, Lee, C, Lenardo, BG, Lesko, KT, Lindote, A, Lopes, MI, Malling, DC, Manalaysay, A, Mannino, RL, Marzioni, MF, McKinsey, DN, Mei, DM, Mock, J, Moongweluwan, M, Morad, JA, Murphy, ASJ, Nehrkorn, C, Nelson, HN, Neves, F, O'Sullivan, K, Oliver-Mallory, KC, Ott, RA, Palladino, KJ, Pangilinan, M, Pease, EK
Publikováno v:
Akerib, DS; Araújo, HM; Bai, X; Bailey, AJ; Balajthy, J; Beltrame, P; et al.(2016). Results on the Spin-Dependent Scattering of Weakly Interacting Massive Particles on Nucleons from the Run 3 Data of the LUX Experiment. Physical Review Letters, 116(16). doi: 10.1103/PhysRevLett.116.161302. UC Berkeley: Retrieved from: http://www.escholarship.org/uc/item/8c58c062
© 2016 American Physical Society. We present experimental constraints on the spin-dependent WIMP (weakly interacting massive particle)-nucleon elastic cross sections from LUX data acquired in 2013. LUX is a dual-phase xenon time projection chamber o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::9b6385989203c8bb27a577f3acd2d0ee
http://www.escholarship.org/uc/item/8c58c062
http://www.escholarship.org/uc/item/8c58c062
Autor:
Akerib, DS, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Beltrame, P, Bernard, EP, Bernstein, A, Biesiadzinski, TP, Boulton, EM, Bradley, A, Bramante, R, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chapman, JJ, Chiller, AA, Chiller, C, Currie, A, Cutter, JE, Davison, TJR, De Viveiros, L, Dobi, A, Dobson, JEY, Druszkiewicz, E, Edwards, BN, Faham, CH, Fiorucci, S, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, CR, Hanhardt, M, Haselschwardt, SJ, Hertel, SA, Hogan, DP, Horn, M, Huang, DQ, Ignarra, CM, Ihm, M, Jacobsen, RG, Ji, W, Kazkaz, K, Khaitan, D, Knoche, R, Larsen, NA, Lee, C, Lenardo, BG, Lesko, KT, Lindote, A, Lopes, MI, Malling, DC, Manalaysay, AG, Mannino, RL, Marzioni, MF, McKinsey, DN, Mei, DM, Mock, J, Moongweluwan, M, Morad, JA, Murphy, ASJ, Nehrkorn, C, Nelson, HN, Neves, F, O'Sullivan, K, Oliver-Mallory, KC, Ott, RA, Palladino, KJ, Pangilinan, M, Pease, EK, Phelps, P, Reichhart, L, Rhyne, C, Shaw, S, Shutt, TA, Silva, C, Solovov, VN
Publikováno v:
Akerib, DS; Araújo, HM; Bai, X; Bailey, AJ; Balajthy, J; Beltrame, P; et al.(2016). Tritium calibration of the LUX dark matter experiment. Physical Review D, 93(7). doi: 10.1103/PhysRevD.93.072009. UC Berkeley: Retrieved from: http://www.escholarship.org/uc/item/07n3t524
© 2016 American Physical Society. We present measurements of the electron-recoil (ER) response of the LUX dark matter detector based upon 170 000 highly pure and spatially uniform tritium decays. We reconstruct the tritium energy spectrum using the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::bab5af0eaceea01f218363445a0b2a7a
http://www.escholarship.org/uc/item/07n3t524
http://www.escholarship.org/uc/item/07n3t524
Autor:
Akerib, DS, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Beltrame, P, Bernard, EP, Bernstein, A, Biesiadzinski, TP, Boulton, EM, Bradley, A, Bramante, R, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chapman, JJ, Chiller, AA, Chiller, C, Currie, A, Cutter, JE, Davison, TJR, De Viveiros, L, Dobi, A, Dobson, JEY, Druszkiewicz, E, Edwards, BN, Faham, CH, Fiorucci, S, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, CR, Hanhardt, M, Haselschwardt, SJ, Hertel, SA, Hogan, DP, Horn, M, Huang, DQ, Ignarra, CM, Ihm, M, Jacobsen, RG, Ji, W, Kazkaz, K, Khaitan, D, Knoche, R, Larsen, NA, Lee, C, Lenardo, BG, Lesko, KT, Lindote, A, Lopes, MI, Malling, DC, Manalaysay, A, Mannino, RL, Marzioni, MF, McKinsey, DN, Mei, DM, Mock, J, Moongweluwan, M, Morad, JA, Murphy, ASJ, Nehrkorn, C, Nelson, HN, Neves, F, O'Sullivan, K, Oliver-Mallory, KC, Ott, RA, Palladino, KJ, Pangilinan, M, Pease, EK
Publikováno v:
Akerib, DS; Araújo, HM; Bai, X; Bailey, AJ; Balajthy, J; Beltrame, P; et al.(2016). Improved Limits on Scattering of Weakly Interacting Massive Particles from Reanalysis of 2013 LUX Data. Physical Review Letters, 116(16). doi: 10.1103/PhysRevLett.116.161301. UC Berkeley: Retrieved from: http://www.escholarship.org/uc/item/8tf1w5zx
© 2016 American Physical Society. We present constraints on weakly interacting massive particles (WIMP)-nucleus scattering from the 2013 data of the Large Underground Xenon dark matter experiment, including 1.4×104 kg day of search exposure. This n
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::a6ee64cf79aacf4601b19a5b984ca9d8
http://www.escholarship.org/uc/item/8tf1w5zx
http://www.escholarship.org/uc/item/8tf1w5zx
Autor:
Carmona-Benitez, MC, Collaboration, LUX, Akerib, DS, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Beltrame, P, Bernard, E, Bernstein, A, Bradley, A, Byram, D, Cahn, SB, Chan, C, Chapman, JJ, Chiller, AA, Chiller, C, Currie, A, de Viveiros, L, Dobi, A, Dobson, J, Druszkiewicz, E, Edwards, B, Faham, CH, Fiorucci, S, Flores, C, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, C, Hanhardt, M, Haselschwardt, S, Hertel, SA, Horn, M, Huang, DQ, Ihm, M, Jacobsen, RG, Kazkaz, K, Knoche, R, Larsen, NA, Lee, C, Lenardo, B, Lesko, KT, Lindote, A, Lopes, MI, Malling, DC, Manalaysay, A, Mannino, R, McKinsey, DN, Mei, D-M, Mock, J, Moongweluwan, M, Morad, J, Murphy, A St J, Nehrkorn, C, Nelson, H, Neves, F, Ott, RA, Pangilinan, M, Parker, PD, Pease, EK, Pech, K, Phelps, P, Reichhart, L, Shutt, T, Silva, C, Solovov, VN, Sorensen, P, O'Sullivan, K, Sumner, TJ, Szydagis, M, Taylor, D, Tennyson, B, Tiedt, DR, Tripathi, M, Tvrznikova, L, Uvarov, S, Verbus, JR, Walsh, N, Webb, R, White, JT, Witherell, MS, Wolfs, FLH, Woods, M, Zhang, C
LUX (Large Underground Xenon) is a dark matter direct detection experiment deployed at the 4850' level of the Sanford Underground Research Facility (SURF) in Lead, SD, operating a 370 kg dual-phase xenon TPC. Results of the first WIMP search run were
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::6bdf12112d9a33dcad0291b17f0cc72a
https://escholarship.org/uc/item/8591d7x2
https://escholarship.org/uc/item/8591d7x2
Autor:
Horn, Markus, Akerib, DS, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Bernard, E, Bernstein, A, Bradley, A, Byram, D, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chapman, JJ, Chiller, AA, Chiller, C, Currie, A, de Viveiros, L, Dobi, A, Dobson, J, Druszkiewicz, E, Edwards, B, Faham, CH, Fiorucci, S, Flores, C, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, C, Hanhardt, M, Haselschwardt, S, Hertel, SA, Huang, DQ, Ihm, M, Jacobsen, RG, Kazkaz, K, Knoche, R, Larsen, NA, Lee, C, Lenardo, B, Lesko, KT, Lindote, A, Lopes, MI, Malling, DC, Mannino, R, McKinsey, DN, Mei, D-M, Mock, J, Moongweluwan, M, Morad, J, Murphy, A St J, Nehrkorn, C, Nelson, H, Neves, F, Ott, RA, Pangilinan, M, Parker, PD, Pease, EK, Pech, K, Phelps, P, Reichhart, L, Shutt, T, Silva, C, Solovov, VN, Sorensen, P, O׳Sullivan, K, Sumner, TJ, Szydagis, M, Taylor, D, Tennyson, B, Tiedt, DR, Tripathi, M, Uvarov, S, Verbus, JR, Walsh, N, Webb, R, White, JT, Witherell, MS, Wolfs, FLH, Woods, M, Zhang, C, Collaboration, On behalf of the LUX
© 2014 Elsevier B.V. The LUX (Large Underground Xenon) experiment aims at the direct detection of dark matter particles via their collisions with xenon nuclei. The 370. kg two-phase liquid xenon time projection chamber measures simultaneously the sc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::c3260b25ea4e635d85eb65dd676423f2
https://escholarship.org/uc/item/05z2g64b
https://escholarship.org/uc/item/05z2g64b
Autor:
Akerib, DS, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Bernard, E, Bernstein, A, Bradley, A, Byram, D, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chapman, JJ, Chiller, AA, Chiller, C, Coffey, T, Currie, A, De Viveiros, L, Dobi, A, Dobson, J, Druszkiewicz, E, Edwards, B, Faham, CH, Fiorucci, S, Flores, C, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, C, Hertel, SA, Horn, M, Huang, DQ, Ihm, M, Jacobsen, RG, Kazkaz, K, Knoche, R, Larsen, NA, Lee, C, Lindote, A, Lopes, MI, Malling, DC, Mannino, R, McKinsey, DN, Mei, DM, Mock, J, Moongweluwan, M, Morad, J, Murphy, ASJ, Nehrkorn, C, Nelson, H, Neves, F, Ott, RA, Pangilinan, M, Parker, PD, Pease, EK, Pech, K, Phelps, P, Reichhart, L, Shutt, T, Silva, C, Solovov, VN, Sorensen, P, O'Sullivan, K, Sumner, TJ, Szydagis, M, Taylor, D, Tennyson, B, Tiedt, DR, Tripathi, M, Uvarov, S, Verbus, JR, Walsh, N, Webb, R, White, JT, Witherell, MS, Wolfs, FLH, Woods, M, Zhang, C
We present the status and prospects of the LUX experiment, which employs approximately 300 kg of two-phase xenon to search for WIMP dark matter interactions. The LUX detector was commissioned at the surface laboratory of the Sanford Underground Resea
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::b75f3e4de0ad04a637316d64ff0e6bf8
https://escholarship.org/uc/item/26s1s7hp
https://escholarship.org/uc/item/26s1s7hp