2021 Annual Workshop
The second Centre Annual Workshop will be held on Monday 29th November - Wednesday 1st December 2021. This year’s Workshop will be an online event, held via Zoom (and the posters session in Gather) with in person gatherings at the nodes.
Code of Conduct
In registering for this event, you have agreed to abide by the Centre’s Code of Conduct. Please ensure that you are familiar with the Code of Conduct, including the Centre Values which are detailed in the full document. An extract of the requirements regarding conduct in meetings is below (click to expand the section).
Zoom details
Join from PC, Mac, iOS or Android: Join our Cloud HD Video Meeting
Password: 334997
Some meeting etiquette and procedure…
if you are not currently presenting, speaking to the meeting, and are not the Session Chair, please make sure your microphone is muted.
perhaps if you are to address the meeting (e.g. during question time), please state your name and maybe also institution, to give some context, and so we all know who you are!
it is up to presenters to use Zoom’s Screenshare on their own computers to display their presentation files to the workshop (unless an alternative has been arranged in advance). Please make sure that you know how to use Screenshare before it’s your turn to present. (The linked files are for backups in case something goes significantly awry, as well as for archiving.)
Uploading presentations
If you are unable to upload your presentation to the Centre’s Confluence site, please email your presentation file directly to padric.mcgee@adelaide.edu.au
Note: if you have a presentation that you do not want to upload to this page (which is a public page), they can be uploaded here instead: 2021 Annual Meeting - (Private) ARC CoE for Dark Matter Particle Physics - Confluence (atlassian.net)
If you do have login access to the Centre’s Confluence site, please login as usual and follow these steps:
click on the Edit icon (the pencil icon at the top-right corner of the page (note that you may need to scroll up the page for it to be visible);
scroll down the page until you find your assigned timeslot in the Agenda (below);
click in the “File” box for your timeslot;
click on the “Files and images” icon at the top of this browser window (6th from right near the centre of the window);
click “Upload a file” to upload the file from your computer;
once it has uploaded, it will be highlighted in blue with a tick mark in the top-right corner;
click “Insert a file” to place the file link at the location where your cursor was in the third step in this process;
click “Publish” in the top-right corner of this browser window in order to save and publish your edit to the page.
NOTE: if there are multiple file links in one timeslot, not all of them may be visible at once. If so, hover your cursor over that timeslot in the Agenda, and one or more arrows should appear; you can use these left and right arrows to scroll through the multiple file links.
Agenda
NOTE: the tables for the Agenda may be wider than your browser window. In this case, at the very end of the Agenda table for each day, there should be a horizontal scroll bar which will allow you to scroll across to the rest of the table. This horizontal scroll bar will be visible only when you are viewing the very end of each day’s Agenda.
Note: times are given in AEDT. Adelaide is 0.5 hours behind; Perth is 3 hours behind.
Monday 29th November
Time (AEDT) | Topic / talk title | Presenter | File | Link to recording |
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10:15-10:20 | Please join the meeting 10-15 minutes prior to its start time. | The meeting proper will commence at 10:30 sharp. | This is to allow for any unexpected problems, etc. |
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10:30
| Welcome and Introduction | Elisabetta Barberio (Director) |
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Session 1 | Session Chair | Raymond Volkas |
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10:45-12:25 | Research Theme Session - Direct Detection |
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10:45-11:00 | Gusts in the Headwind: Uncertainties in Direct Dark Matter Detection | Grace Lawrence |
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11:00-11:10 | SABRE Status Report | Gary Hill |
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11:10-11:20 | SABRE Prospective and Physics Reach part 1 | William Melbourne |
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11:20-11:35 | SABRE Prospective and Physics Reach part 2 | Madeleine Zurowski | (see above) |
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11:35-11:50 | Cygnus: Status and Future Plans | Lachlan McKie |
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11:50:12:05 | ORGAN: Results and Future Plans | Aaron Quiskamp |
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12:05-12:15 | WISP & Snowmass: How to be part of the International Conversation | Mike Tobar |
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12:15-12:25 | WIMP: Future Experimental Landscape | Peter Cox/Elisabetta Barberio |
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12:25-13:15 | Break |
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Session 2 | Session Chair | Anthony Thomas |
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13:15-13:45 | Research Theme Session - LHC |
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13:15 (6 mins) | Introduction | Geoff Taylor |
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13:21 (12 mins) | Physics analyses with the ATLAS experiment | Harish Potti |
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13:33 (12 mins) | The Australian ITk programme | James Webb |
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13:45-14:15 | Research Theme Session - Metrology |
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| Metrology: Overview | Ferdos Dastgiri |
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| Radioimpurities in Detector Materials: Potassium-40 | Zuzana Slavkovska |
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| Lead-210: A Radioimpurity In Particle Detectors For Dark Matter Studies | Michaela Froehlich |
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Session 3 | Session Chair | Phillip Urquijo |
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14:15 (30 mins) | Outreach Activity | Jackie Bondell |
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14:45 (40 mins) | ED&I Session | Cedric Simenel and Phillip Urquijo (Portfolio Leaders) |
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15:25 (15 mins) | Media & Communications Session | Fleur Morrison |
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15:40-16:00 | Break |
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16:00 | Close |
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Tuesday 30th November
Time (AEDT) | Topic / talk title | Presenter | File | Link to recording |
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10:15-10:20 | Please join the meeting 10-15 minutes prior to its start time. | The meeting proper will commence at 10:30 sharp. | This is to allow for any unexpected problems, etc. |
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Session 4 | Session Chair | Andrew Stuchbery |
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10:30 (45 mins) | Keynote presentation - Low-mass DM detection | Noah Kurinsky, Staff Scientist, SLAC National Accelerator Laboratory Noah got his PhD from Stanford in 2018 working on the SuperCDMS experiment, using new detector concepts to probe sub-GeV dark matter. From 2018-2021, Noah was a Lederman Fellow at Fermilab, where he spearheaded efforts to combine concepts from quantum information science and particle physics to open new windows into the study of dark matter. He joined SLAC in 2021, starting a new lab focused on meV-GeV mass dark matter detection with quantum sensors. Noah is a member of the SuperCDMS collaboration, a founding member of the BREAD axion search experiment, and leads R&D programs into novel qubit architectures and advanced techniques for phonon and photon sensing in low-background environments. |
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11:15-12:45 | Research Theme Session - Theory |
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11:15 (20 mins) | Cosmological simulations: beyond the Standard Model | Robert Mostoghiu |
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11:35 (20 mins) | Constraints on the dark photon from deep inelastic scattering | Xuan-Gong Wang |
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11:55 (20 mins) | Saving the axion from gravity: the 'companion axion' and its phenomenology | Zac Picker |
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12:15 (15 mins) | Exploring the cosmological dark matter coincidence with infrared fixed points | Alex Ritter |
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12:30 (15 mins) | A new stellar constraint on axion-like particles | Fred Hiskens |
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12:45-13:25 | Break |
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Session 5 | Session Chair | Ben McAllister |
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13:25 (20 mins) | Awards Ceremony | Elisabetta Barberio/Justin Zobel | selection Criteria
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13:45 (1 hour) | Code of Conduct Deployment / Emotional Intelligence Module Launch | Mark Dean |
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14:45 (15 mins) | ECR Update | Lindsey Bignell, Zuzana Slavkovska, William Melbourne |
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15:00-15:20 | Break |
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15:20 (1 hour) | Poster Session | Various - see attached list See the attached document that contains instructions on using Gather and the link to access Gather during the annual annual meeting and poster session. Poster presenters and Centre members who wish to view the posters in Gather must have access to their own laptop/computer with camera and microphone. |
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16:20 | Close |
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Wednesday 1st December
Time (AEDT) | Topic / talk title | Presenter | File | Link to recording |
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10:00-10:15 | Please join the meeting 10-15 minutes prior to its start time. | The meeting proper will commence at 10:15 sharp. | This is to allow for any unexpected problems, etc. |
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| EQUS / CDM Combined Session |
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10:15 (45 mins) | Keynote Presentation: To see 85% of the World in a Grain of Sand: Search for wave-like dark matter in the ADMX Run 1C dataset | Dr Chelsea Bartram Chelsea is an experimentalist at heart, with a goal of finding dark matter and revealing physics beyond the Standard Model. Her research interests lie at the intersection of particle physics, fundamental symmetries, dark matter, and quantum electronics. She is a leader in the Axion Dark Matter eXperiment (ADMX) located at CENPA, a nuclear physics lab at the University of Washington. Her research pulls from disparate fields such as microwave technology, low temperature physics and high magnetic fields. It even has overlap with the world of amateur radio–a hobby which prompted an interest in science many years ago. She has had the privilege of working in numerous research groups, touching on fundamental symmetries and neutrino physics. As a graduate student, she built a tabletop experiment to search for CPT-violation in positronium at UNC Chapel Hill. Chelsea finds nothing so empowering as building an experiment that tells you something about the real world and she strives to teach others to do the same. |
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11:00 (20 mins) | Finding Dark Matter with Superfluid Helium Astrophysical phenomena in dilute superfluids | Glen Harris Tyler Neely |
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11:20 (20 mins) | Towards Cryogenic Particle Detection | Catriona Thomson |
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11:40 (20 mins) | Bloch-Redfield or Lindblad equations for modelling a current biased RCJ single photon detector | Graeme Flower |
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| Return to CDM Session | Join our Cloud HD Video Meeting Password: 334997 |
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12:00 (20 mins) | Other Aspects of Low Mass Direct Detection | Matthew Dolan |
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12:20-13:00 | Break |
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Session 6 | Session Chair | Nicole Bell |
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13:00 (15 mins) | Advisory Board Chair | Professor Aidan Byrne |
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13:15 (1 hour) | Innovation Activity | Christine Thong | QR code → short feedback survey (2 mins) |
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14:15 (15 mins) | SUPL C Chair | Sue Barrell |
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14:30 (15 mins) | Director’s Conclusions / Visions for the Future | Elisabetta Barberio |
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14:45-15:05 | Break |
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15:05-15:35 | Node Activity - each node has the option to run a social activity or finish the day early. |
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15:35 | Close |
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