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Alex Martyniuk (University College London)10/02/2020, 08:30
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Biagio Di Micco (Universita' degli Studi di Roma Tre e Istituto Nazionale di Fisica Nucleare (INFN))10/02/2020, 09:30
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Eric Drechsler (Simon Fraser University (CA))10/02/2020, 09:45
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Antonio Vagnerini (Deutsches Elektronen-Synchrotron (DE))10/02/2020, 10:00
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Kenji Hamano (University of Victoria (CA))10/02/2020, 10:15
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Nicolo Vladi Biesuz10/02/2020, 11:00
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Matthew Feickert (Univ. Illinois at Urbana Champaign (US))10/02/2020, 11:15
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Alexei Safonov (Texas A & M University (US))10/02/2020, 11:30
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Kohsaku Tobioka10/02/2020, 17:30
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Baduyo Cheng (IHEP), Jonathan Long (Univ. Illinois at Urbana Champaign (US))10/02/2020, 18:30
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Jonathan Long (Univ. Illinois at Urbana Champaign (US))10/02/2020, 18:45
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Chris Hill (Ohio State University (US))10/02/2020, 19:00
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Carlo Dallapiccola (University of Massachusetts (US))10/02/2020, 19:15
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Jonas Till Roemer (Rheinisch Westfaelische Tech. Hoch. (DE))10/02/2020, 19:30
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Guy Henri Maurice Wormser (Centre National de la Recherche Scientifique (FR))11/02/2020, 08:30
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Samuel William Maddrell-Mander (University of Bristol (GB))11/02/2020, 09:30
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Carmen Giugliano (Universita e INFN, Ferrara (IT))11/02/2020, 09:45
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Alexei Sibidanov (Istituto Nazionale Fisica Nucleare (INFN)-Unknown-Unknown)11/02/2020, 10:00
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Piera Muzzetto (Universita e INFN, Cagliari (IT))11/02/2020, 10:15
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Gediminas Sarpis (University of Manchester (GB))11/02/2020, 10:45
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Mr Kookhyun Kang (Kyungpook National Universiy)11/02/2020, 11:00
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David Cinabro11/02/2020, 11:15
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Andreas Warburton (McGill University, (CA))11/02/2020, 11:30
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Daniele Manuzzi (Universita e INFN, Bologna (IT))11/02/2020, 11:45
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Avery Broderick11/02/2020, 20:00
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Patrick Huber12/02/2020, 08:30
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Chris Marshall (University of Rochester)12/02/2020, 09:30
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Xuefeng Ding12/02/2020, 09:45
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Olga Kyzylova (Drexel University)12/02/2020, 10:00
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Xuefeng Ding12/02/2020, 10:15
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Claudio Kopper (University of Alberta)12/02/2020, 10:45
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Rémy Le Breton (APC)12/02/2020, 11:00
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Dr Matej Pavin (TRIUMF)12/02/2020, 11:15
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Nikolina Ilic (Nikhef National institute for subatomic physics (NL))12/02/2020, 11:30
The Deep Underground Neutrino Experiment (DUNE) represents a bold step forward with a new detector technology and the ability to measure neutrinos using a broad-band neutrino beam. DUNE will consist of two massive detectors: one located at Fermilab in Illinois, and one located 1300 km away in South Dakota. DUNE offers a unique opportunity to measure the nature of the neutrino masses, quantify...
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Tingjun Yang (Fermi National Accelerator Lab. (US))12/02/2020, 11:45
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Philip Hamacher-Baumann (RWTH Aachen University)12/02/2020, 17:30
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Ashley Back (Queen Mary, University of London)12/02/2020, 17:45
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Sophie Berkman (Fermi National Accelerator Laboratory)12/02/2020, 18:00
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Dr José I. Crespo-Anadón (Columbia University)12/02/2020, 18:15
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Yifan Chen (Universitaet Bern (CH))12/02/2020, 18:30
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Christopher Chambers12/02/2020, 18:45
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Bradford Welliver (Lawrence Berkeley National Laboratory)12/02/2020, 19:00
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Morgan Clark12/02/2020, 19:15
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Oliver Schulz (MPI for Physics, Munich)13/02/2020, 08:30
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Gulden Othman (University Of North Carolina)13/02/2020, 08:45
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Ashley Back (Queen Mary, University of London)13/02/2020, 09:00
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Jan D. Behrens13/02/2020, 09:15
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Yonatan Kahn (University of Illinois at Urbana-Champaign)13/02/2020, 09:30
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Michael De Nuccio13/02/2020, 10:45
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Chelsea Bartram (Boston University)13/02/2020, 11:00
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Enze Zhang13/02/2020, 11:15
The SuperCDMS SNOLAB experiment is designed to be a next generation dark matter direct detection experiment, following SuperCDMS Soudan. The experiment is currently under construction. The main science goal is to improve the sensitivity for dark matter particles with masses ≤10 GeV by at least one order of magnitude in cross section over current results from the SuperCDMS Soudan experiment....
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Mr Deepak Tiwari (PICO, Université de Montréal)13/02/2020, 11:30
The PICO collaboration uses bubble chambers filled with superheated C3F8 as a target for dark matter detection. PICO-60, with a threshold of 2.45 keV, set the most stringent direct-detection constraint to date on the weakly interacting massive particle (WIMP)-proton spin-dependent cross section at 3.2 × 10−41cm2 for a 25 GeV WIMP [Phys. Rev. D100 022001 (2019)]. Its successor PICO-40L employs...
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Sean Daugherty13/02/2020, 17:45
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Marie-Cécile Piro (University of Alberta)13/02/2020, 18:00
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Ryan Thomas (University of Chicago)13/02/2020, 18:15
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Holger Müller13/02/2020, 18:30
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Alexander Mitov (University of Cambridge (GB))14/02/2020, 08:30
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Federica Fabbri (University of Glasgow (GB))14/02/2020, 09:30
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Pavol Bartos (Comenius University (SK))14/02/2020, 09:45
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Greg Landsberg14/02/2020, 10:30
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Julie Kirk (Science and Technology Facilities Council STFC (GB))14/02/2020, 10:50
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Tadeas Bilka14/02/2020, 11:05
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MING-CHUAN CHANG (FU JEN CATHOLIC UNIVERSITY)14/02/2020, 11:20
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Fergus Wilson (Science and Technology Facilities Council STFC (GB))14/02/2020, 11:35
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Larry McLerran (BNL)14/02/2020, 17:30
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Justin Edward Frantz (Ohio University (US))14/02/2020, 18:30
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Samer Ahmed (Helmholtz-Institut Mainz)14/02/2020, 18:45
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Richard Bonventre (Lawrence Berkeley National Laboratory)14/02/2020, 19:00
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Dr Simone Schuchmann (Johannes Gutenberg Universitaet Mainz (DE))14/02/2020, 19:15
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Kristof Schmieden (CERN)14/02/2020, 19:35
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Hafizh Prihtiadi (Bandung Institute of Technology)
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Yi Wang
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Jun Guo (Shanghai Jiao Tong University (CN))
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