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Meeting ID: 765 773 9945
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Meeting ID: 765 773 9945
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Kimberly Palladino (University of Wisconsin-Madison)12/8/19, 9:00 AM
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Jim Hirschauer12/8/19, 9:15 AM
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Jodi Cooley12/8/19, 9:30 AM
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Dr BRENNA FLAUGHER (Fermilab)12/8/19, 9:45 AMBRN PlenariesPrecision measurements of cosmic expansion and the large-scale distribution of matter transform the universe into a laboratory for studying fundamental physics. Measurements of the “late universe,” through Stage-III dark energy experiments and the “early universe” through the Cosmic Microwave Background (CMB) reveal a universe that is best described by the Lambda CDM concordance cosmological...Go to contribution page
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Sarah Demers (Yale University)12/8/19, 10:00 AM
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Amy Conolly12/8/19, 10:15 AM
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Junqi XIE (Argonne National Laboratory)12/8/19, 11:40 AM
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Tim Kovachy12/8/19, 11:52 AM
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Dr Hugh Lippincott (UCSB)12/8/19, 12:04 PMBRN Plenaries
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Prof. Tulika Bose (University of Wisconsin-Madison)12/8/19, 12:16 PM
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Carl Haber12/8/19, 1:30 PM
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Roger Rusack12/8/19, 1:45 PMBRN Plenaries
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Mitch Newcomer12/8/19, 2:00 PM
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Mr austin mcdonald (University of Texas at Arlington)12/9/19, 4:30 PMAward plenariesTalkA robust observation of neutrinoless double beta decay is currently the most sensitive method to determine the Majorana nature of the neutrino. The detection of the single barium ion produced as a result of the double beta decay of xenon 136 would enable a new class of ultra-low background neutrinoless double beta decay experiments. However, despite 19 years of R&D, a credible method to...Go to contribution page
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Mr Tanner Kaptanoglu (University of Pennsylvania)12/9/19, 4:45 PMAward plenariesTalkWe introduce a new device, ‘the dichroicon’, that is capable of providing information on photon wavelength in a large-scale neutrino detector. In a Cherenkov detector, photon wavelength carries information about the propagation time from source vertex to photon sensor. Measuring the difference in time between many long-wavelength and short-wavelength photons that lie along a Cherenkov ring...Go to contribution page
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Mr xinran li (Princeton University)12/9/19, 5:00 PMAward plenaries
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Ana Amelia Machado, Ettore Segreto12/9/19, 5:15 PMThe idea of the ARAPUCA was proposed in 2015 with the goal of satisfying the need for a device with a good detection efficiency (at the level of few percent) over a large area (tenths of a squre meter or more), for large scale liquid argon experiments. The great novelty introduced by this device is represented by its capability of trapping photons inside a cavity with highly reflective...Go to contribution page
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Dr hanguo wang (UCLA)12/9/19, 5:35 PMAward plenariesIn this presentation, I will first review briefly the early liquid noble gas R&D work within the ICARUS framework at CERN since 1989. Then I will report a few technical areas related to liquid noble TPC requirement, such as TPC field uniformity, high voltage, cryogenics and purification. I then will summarize the current work aiming at a zero instrumental background detector DarkSide-20k. A...Go to contribution page
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Dr Jingke Xu (Lawrence Livermore National Laboratory), Jonathan Asaadi (Syracuse), Jonathan Asaadi (University of Texas Arlington)12/10/19, 1:30 PM
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Isobel Ojalvo (University Wisconsin Madison), Verena Ingrid Martinez Outschoorn (University of Massachusetts Amherst)12/10/19, 1:45 PM
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Prof. Karl Berggren (MIT), Dr juan estrada (fermilab)12/10/19, 2:00 PM
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Andrey Elagin (University of Chicago), Junqi XIE (Argonne National Laboratory), paul oconnor (Brookhaven National Laboratory)12/10/19, 2:15 PM
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Sally Seidel (University of New Mexico)12/10/19, 2:30 PM
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Kimberly Palladino (University of Wisconsin-Madison)12/10/19, 2:45 PM
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12/10/19, 3:00 PM