Conveners
Collab Meeting: Monday Morning
- M. Patrick Decowski (Nikhef / University of Amsterdam)
Collab Meeting
- Chamkaur Ghag
Collab Meeting
- Teresa Marrodán Undagoitia
Collab Meeting
- Jonathan Hays (University of London (GB))
Collab Meeting
- Marco Selvi (INFN Bologna)
Collab Meeting
- Masaki Yamashita (Nagoya University)
Collab Meeting: L2 Breakout Time
- There are no conveners in this block
Collab Meeting
- Thomas Brunner (McGill University)
Collab Meeting
- Kathrin Valerius
Collab Meeting
- Alexandre Lindote
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Björn Penning, Laura Baudis29/06/2026, 10:00Presentation
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Daniel Akerib, Henrique Araujo, Prof. Marc Schumann (University of Freiburg (DE))29/06/2026, 10:10
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Ran Budnik29/06/2026, 10:40Presentation
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Dr Alexandre Lindote, Teresa Marrodán Undagoitia29/06/2026, 10:50Presentation
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Henrique Araujo, Kevin Lesko29/06/2026, 11:00Presentation
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Hugh Lippincott (UCSB)29/06/2026, 13:30Presentation
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Theresa Fruth (University of Sydney)29/06/2026, 14:15Presentation
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Brian Mong (SLAC), Thomas Brunner (McGill University)29/06/2026, 14:45Presentation
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Prof. Kimberly Palladino (University of Oxford), Laura Baudis29/06/2026, 15:15Presentation
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Daniel Tovey (University of Sheffield (GB)), Tom Shutt, Prof. Uwe Gerd Oberlack (Johannes Gutenberg University Mainz)29/06/2026, 16:00Presentation
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29/06/2026, 16:20
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29/06/2026, 17:00Presentation
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29/06/2026, 17:30Presentation
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30/06/2026, 08:30Presentation
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30/06/2026, 09:00
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Prof. Kimberly Palladino (University of Oxford), Prof. Marc Schumann (University of Freiburg (DE)), Tom Shutt30/06/2026, 09:30Presentation
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Pietro Di Gangi, Sergey Burdin (University of Liverpool (GB))30/06/2026, 10:00Presentation
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30/06/2026, 11:00Presentation
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30/06/2026, 11:30
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30/06/2026, 12:00Presentation
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Brian Mong (SLAC)30/06/2026, 14:00Presentation
I will describe the 222Rn backgrounds in XLZD, try to come up with a bottom up estimate as I see it. I will also like to talk about Rn assay techniques.
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Lutz Althüser (University of Münster)30/06/2026, 14:20Presentation
Next generation liquid noble gas detectors for the search of weakly interacting massive particles (WIMPs), such as XLZD, aim to increase their sensitivity down to the neutrino fog. This ambitious goal can only be achieved by further reducing the detector backgrounds dominated by LXe intrinsic isotopes of $^{85}$Kr and $^{222}$Rn to a factor ten below the unshieldable solar and atmospheric...
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Naman Walia30/06/2026, 14:40Presentation
The construction of next generation low-background detectors requires, material that balances radiopurity with superior mechanical properties. While electroformed copper is currently known to have the best radiopurity levels, however it is constrained by slow depositions rate, limited structural strength and complex manufacturing requirements. The talk introduces chemical vapour deposition...
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Frédéric Girard (McGill University)30/06/2026, 15:00Presentation
The ReStoX concept is, in itself, simple: a pressure vessel with cryopumping capability, able to safely recover and store high-pressure xenon at room temperature. Beyond this concept lie complex, site-dependent engineering challenges that influence the design with aspects such as laboratory accessibility, on-site vs. off-site construction, cooling power requirements, operational complexity and...
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Alex Jones (STFC-UKRI)30/06/2026, 15:20Presentation
An overview of the existing XLZD@Boulby schedule and how it might be adjusted to suit a site agnostic installation timeline in advance of the XLZD Concept Design Review (CDR). The current schedule covers key components from the Work Breakdown Structure (WBS) from completion of the XLZD CDR through to commissioning of the XLZD detector, identifying potential critical paths, and estimating lead...
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Nadav Hargittai (Weizmann Institute of Science)30/06/2026, 15:40Presentation
The two research communities of Neutrinoless Double Beta Decay ($0\nu2\beta$) and dark matter Weakly Interacting Massive Particle (WIMP) searches have had a large technological overlap in their use of the Liquid Xenon (LXe) Time Projection Chamber (TPC). As detectors get larger and more complex, the possibility of combining their efforts into one mutually beneficial experiment becomes...
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30/06/2026, 16:30
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01/07/2026, 08:30
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01/07/2026, 08:55
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01/07/2026, 09:20
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01/07/2026, 09:45
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Adam Softley-Brown (University of Sheffield), Jelle Aalbers (University of Amsterdam / Nikhef)01/07/2026, 10:10
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01/07/2026, 11:00Presentation
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01/07/2026, 11:30Presentation
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01/07/2026, 12:00Presentation
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Daniel Tovey (University of Sheffield (GB)), Tom Shutt, Prof. Uwe Gerd Oberlack (Johannes Gutenberg University Mainz)01/07/2026, 14:00
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Henrique Araujo01/07/2026, 15:00Presentation
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Erica Caden (SNOLAB), Nicolas Angelides (University of Zurich)01/07/2026, 15:30
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Björn Penning, Laura Baudis01/07/2026, 16:00Presentation
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Huan ZhangPoster
LUX-ZEPLIN (LZ) and the next generation XLZD experiments are designed to search for dark matter using two-phase xenon time projection chambers. Apart from searching for Weakly Interacting Massive Particles (WIMPs), LZ is also looking for axion-like particles (ALPs), solar neutrino, mirror dark matter, and hidden photons. XLZD has already published or been researching on its projections to...
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Adam Softley-Brown (University of Sheffield), Jelle Aalbers (University of Amsterdam / Nikhef)