Our charge is to review future plans experimentation in particle dark matter experiments. We will not focus much on the theoretical motivations for experiments; instead, we will try to evaluate the current sensitivities and limitations, and try to project sensitivities in the near future.
We will encourage robust interaction and discussion, so times other than the 8:30am start time may slip. Speakers should plan to leave 10 minutes for discussion. The talks should focus on the speaker's own projects and their experimental limitations and projections.
The room will have an overhead projector, and should have a laptop controlled
projector. To be safe, I advise speakers to bring transparencies.
| Time | Speaker | Institution | Topic | ||
|---|---|---|---|---|---|
| 8:00am | Darin Kinion | UC Berkeley | Super Low Noise RF Amplifier via a SQUID | kinion1@llnl.gov | |
| 8:30am | Leslie Rosenberg | MIT | The Future of Axion Detection | ljr@mitlns.mit.edu | |
| 9:00am | Laura Baudis | Stanford | Genius | lbaudis@Stanford.EDU | ppt |
| 9:30am | Rick Gaitskell | UCL/Brown | CryoArray: 1 tonne discriminating Dark Matter Detector | rick@gaitskell.com | ppt |
| 10:55am | James White | Texas A & M | Dark Matter Detection in Liquid and Solid Noble Gases | white@physics.tamu.edu | |
| 11:25am | Elena Aprile | Columbia | LXe in Astrophysics and Applications to Dark Matter | age@astro.columbia.edu | |
| 11:55am | Neil Spooner | Sheffield | Overview of Boulby Liquid Xenon Program | N.Spooner@sheffield.ac.uk | ppt |
| 12:10pm | Hanguo Wang | UCLA | Zeplin II-Status / Zeplin IV | wangh@physics.ucla.edu | ppt |
| 12:40pm | Tim Sumner | Imperial College | Zeplin-III | t.sumner@ic.ac.uk | ppt |
| 1:10pm | All | Adjourn |