25–28 Mar 2020
UCLA
US/Pacific timezone

Scintillating Bubble Chambers for GeV WIMPs and reactor CEvNS

27 Mar 2020, 18:00
15m
PAB- 1-425 (UCLA)

PAB- 1-425

UCLA

UCLA Department of Physics and Astronomy 475 Portola Plaza, Los Angeles, CA 90095
Talk Non-directional direct dark matter detection Session 14

Speaker

Dr Rocco Coppejans (Northwestern University)

Description

The Scintillating Bubble Chamber (SBC) is a rapidly developing new technology for sub-keV nuclear recoil detection. Demonstrations in liquid xenon at the few-gram scale have confirmed that this technique combines the event-by-event energy resolution of a liquid-noble scintillation detector with the world-leading electron-recoil discrimination capability of the bubble chamber, and in fact maintains that discrimination capability at much lower thresholds than traditional Freon-based bubble chambers. The promise of unambiguous identification of sub-keV nuclear recoils in a scalable detector makes this an ideal technology for both GeV-mass WIMP searches and CEvNS detection at reactor sites. We will present progress from the SBC Collaboration towards the construction of a pair of 10-kg argon bubble chambers at Fermilab and SNOLAB, to test the low-threshold performance of this technique in a physics-scale device and to search for 0.7 - 7 GeV dark matter, respectively.

Authors

Dr Rocco Coppejans (Northwestern University) Prof. C Eric Dahl (Northwestern University)

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