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Insertion of STC into TRT at the Department of Physics, Oxford
Credit: CERN

Dr. Kimberly Palladino

Associate Professor

Sub department

  • Particle Physics

Research groups

  • LUX-ZEPLIN
kimberly.palladino@physics.ox.ac.uk
Telephone: 273301
Denys Wilkinson Building, room 622
  • About
  • Publications

Signal yields, energy resolution, and recombination fluctuations in liquid xenon

(2016)

Authors:

DS Akerib, S Alsum, HM Araújo, X Bai, AJ Bailey, J Balajthy, P Beltrame, EP Bernard, A Bernstein, TP Biesiadzinski, EM Boulton, R Bramante, P Brás, D Byram, SB Cahn, MC Carmona-Benitez, C Chan, AA Chiller, C Chiller, A Currie, JE Cutter, TJR Davison, A Dobi, JEY Dobson, E Druszkiewicz, BN Edwards, CH Faham, S Fiorucci, RJ Gaitskell, VM Gehman, C Ghag, KR Gibson, MGD Gilchriese, CR Hall, M Hanhardt, SJ Haselschwardt, SA Hertel, DP Hogan, M Horn, DQ Huang, CM Ignarra, M Ihm, RG Jacobsen, W Ji, K Kamdin, K Kazkaz, D Khaitan, R Knoche, NA Larsen, C Lee, BG Lenardo, KT Lesko, A Lindote, MI Lopes, A Manalaysay, RL Mannino, MF Marzioni, DN McKinsey, D-M Mei, J Mock, M Moongweluwan, JA Morad, A St J Murphy, C Nehrkorn, HN Nelson, F Neves, K O'Sullivan, KC Oliver-Mallory, KJ Palladino, EK Pease, P Phelps, L Reichhart, C Rhyne, S Shaw, TA Shutt, C Silva, M Solmaz, VN Solovov, P Sorensen, S Stephenson, TJ Sumner, M Szydagis, DJ Taylor, WC Taylor, BP Tennyson, PA Terman, DR Tiedt, WH To, M Tripathi, L Tvrznikova, S Uvarov, JR Verbus, RC Webb, JT White, TJ Whitis, MS Witherell, FLH Wolfs, J Xu, K Yazdani, SK Young, C Zhang
More details from the publisher

Results from a search for dark matter in the complete LUX exposure

(2016)

Authors:

DS Akerib, S Alsum, HM Araújo, X Bai, AJ Bailey, J Balajthy, P Beltrame, EP Bernard, A Bernstein, TP Biesiadzinski, EM Boulton, R Bramante, P Brás, D Byram, SB Cahn, MC Carmona-Benitez, C Chan, AA Chiller, C Chiller, A Currie, JE Cutter, TJR Davison, A Dobi, JEY Dobson, E Druszkiewicz, BN Edwards, CH Faham, S Fiorucci, RJ Gaitskell, VM Gehman, C Ghag, KR Gibson, MGD Gilchriese, CR Hall, M Hanhardt, SJ Haselschwardt, SA Hertel, DP Hogan, M Horn, DQ Huang, CM Ignarra, M Ihm, RG Jacobsen, W Ji, K Kamdin, K Kazkaz, D Khaitan, R Knoche, NA Larsen, C Lee, BG Lenardo, KT Lesko, A Lindote, MI Lopes, A Manalaysay, RL Mannino, MF Marzioni, DN McKinsey, DM Mei, J Mock, M Moongweluwan, JA Morad, A St J Murphy, C Nehrkorn, HN Nelson, F Neves, K O`Sullivan, KC Oliver-Mallory, KJ Palladino, EK Pease, P Phelps, L Reichhart, C Rhyne, S Shaw, TA Shutt, C Silva, M Solmaz, VN Solovov, P Sorensen, S Stephenson, TJ Sumner, M Szydagis, DJ Taylor, WC Taylor, BP Tennyson, PA Terman, DR Tiedt, WH To, M Tripathi, L Tvrznikova, S Uvarov, JR Verbus, RC Webb, JT White, TJ Whitis, MS Witherell, FLH Wolfs, J Xu, K Yazdani, SK Young, C Zhang
More details from the publisher

Low-energy (0.7-74 keV) nuclear recoil calibration of the LUX dark matter experiment using D-D neutron scattering kinematics

ArXiv 1608.05381 (2016)

Authors:

LUX Collaboration, DS Akerib, S Alsum, HM Araújo, X Bai, AJ Bailey, J Balajthy, P Beltrame, EP Bernard, A Bernstein, TP Biesiadzinski, EM Boulton, A Bradley, R Bramante, P Brás, D Byram, SB Cahn, MC Carmona-Benitez, C Chan, JJ Chapman, AA Chiller, C Chiller, A Currie, JE Cutter, TJR Davison, L de Viveiros, A Dobi, JEY Dobson, E Druszkiewicz, BN Edwards, CH Faham, S Fiorucci, RJ Gaitskell, VM Gehman, C Ghag, KR Gibson, MGD Gilchriese, CR Hall, M Hanhardt, SJ Haselschwardt, SA Hertel, DP Hogan, M Horn, DQ Huang, CM Ignarra, M Ihm, RG Jacobsen, W Ji, K Kamdin, K Kazkaz, D Khaitan, R Knoche, NA Larsen, C Lee, BG Lenardo, KT Lesko, A Lindote, MI Lopes, DC Malling, A Manalaysay, RL Mannino, MF Marzioni, DN McKinsey, DM Mei, J Mock, M Moongweluwan, JA Morad, A St J Murphy, C Nehrkorn, HN Nelson, F Neves, K O'Sullivan, KC Oliver-Mallory, KJ Palladino, M Pangilinan, EK Pease, P Phelps, L Reichhart, CA Rhyne, S Shaw, TA Shutt, C Silva, M Solmaz, VN Solovov, P Sorensen, S Stephenson, TJ Sumner, M Szydagis, DJ Taylor, WC Taylor, BP Tennyson, PA Terman, DR Tiedt, WH To, M Tripathi, L Tvrznikova, S Uvarov, JR Verbus, RC Webb, JT White, TJ Whitis, MS Witherell, FLH Wolfs, J Xu, K Yazdani, SK Young, C Zhang

Abstract:

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 $\textit{in situ}$ in the LUX detector using a collimated beam of mono-energetic 2.45 MeV neutrons produced by a deuterium-deuterium (D-D) fusion source. The nuclear recoil energy from the first neutron scatter in the TPC was reconstructed using the measured scattering angle defined by double-scatter neutron events within the active xenon volume. We measured the absolute charge ($Q_{y}$) and light ($L_{y}$) yields at an average electric field of 180 V/cm for nuclear recoil energies spanning 0.7 to 74 keV and 1.1 to 74 keV, respectively. This calibration of the nuclear recoil signal yields will permit the further refinement of liquid xenon nuclear recoil signal models and, importantly for dark matter searches, clearly demonstrates measured ionization and scintillation signals in this medium at recoil energies down to $\mathcal{O}$(1 keV).
Details from ArXiV

Characteristics of Four Upward-Pointing Cosmic-Ray-like Events Observed with ANITA

Physical Review Letters American Physical Society (APS) 117:7 (2016) 071101

Authors:

PW Gorham, J Nam, A Romero-Wolf, S Hoover, P Allison, O Banerjee, JJ Beatty, K Belov, DZ Besson, WR Binns, V Bugaev, P Cao, C Chen, P Chen, JM Clem, A Connolly, B Dailey, C Deaconu, L Cremonesi, PF Dowkontt, MA DuVernois, RC Field, BD Fox, D Goldstein, J Gordon, C Hast, CL Hebert, B Hill, K Hughes, R Hupe, MH Israel, A Javaid, J Kowalski, J Lam, JG Learned, KM Liewer, TC Liu, JT Link, E Lusczek, S Matsuno, BC Mercurio, C Miki, P Miočinović, M Mottram, K Mulrey, CJ Naudet, J Ng, RJ Nichol, K Palladino, BF Rauch, K Reil, J Roberts, M Rosen, B Rotter, J Russell, L Ruckman, D Saltzberg, D Seckel, H Schoorlemmer, S Stafford, J Stockham, M Stockham, B Strutt, K Tatem, GS Varner, AG Vieregg, D Walz, SA Wissel, F Wu
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Details from ArXiV

Chromatographic separation of radioactive noble gases from xenon

(2016)

Authors:

LUX Collaboration, DS Akerib, HM Araújo, X Bai, AJ Bailey, J Balajthy, P Beltrame, EP Bernard, A Bernstein, TP Biesiadzinski, EM Boulton, R Bramante, SB Cahn, MC Carmona-Benitez, C Chan, AA Chiller, C Chiller, T Coffey, A Currie, JE Cutter, TJR Davison, A Dobi, JEY Dobson, E Druszkiewicz, BN Edwards, CH Faham, S Fiorucci, RJ Gaitskell, VM Gehman, C Ghag, KR Gibson, MGD Gilchriese, CR Hall, M Hanhardt, SJ Haselschwardt, SA Hertel, DP Hogan, M Horn, DQ Huang, CM Ignarra, M Ihm, RG Jacobsen, W Ji, K Kamdin, K Kazkaz, D Khaitan, R Knoche, NA Larsen, C Lee, BG Lenardo, KT Lesko, A Lindote, MI Lopes, A Manalaysay, RL Mannino, MF Marzioni, DN McKinsey, D-M Mei, J Mock, M Moongweluwan, JA Morad, A St J Murphy, C Nehrkorn, HN Nelson, F Neves, K O'Sullivan, KC Oliver-Mallory, KJ Palladino, EK Pease, K Pech, P Phelps, L Reichhart, C Rhyne, S Shaw, TA Shutt, C Silva, VN Solovov, P Sorensen, S Stephenson, TJ Sumner, M Szydagis, DJ Taylor, W Taylor, BP Tennyson, PA Terman, DR Tiedt, WH To, M Tripathi, L Tvrznikova, S Uvarov, JR Verbus, RC Webb, JT White, TJ Whitis, MS Witherell, FLH Wolfs, K Yazdani, SK Young, C Zhang
More details from the publisher

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