Collaboration Meeting
Our supersonic project collaboration meeting will take place Monday, March 27th - Wednesday, March 29th.
Venue: UCLA's Physics and Astronomy building. The talks will take place in the 3rd-floor conference room, known as PAB 3-703. The breakfast and coffee breaks will take place on the 3rd-floor patio (or in the Astro-reading room if weather conditions are less than favorable).
Schedule
Monday, March 27
| Time | Event/speaker | Details |
| 9:30am | Breakfast and meetup | |
| 10am | Introductions | |
| 10:15am | Smadar Naoz | The supersonic project - an overall view |
| 10:30am | William Lake | SIGOs evolution and star formation |
| 11am | Yurina Nakazato | H2 cooling of gravitational collapse of SIGOs with high-resolution simulationsn |
| 11:30am | discussion: | the definition of a SIGO and its evolution |
| 12:00am | Lunch break | Westwood or on campus |
| 2:00pm | Blakesley Burkhart | Statistics of Turbulence and Star Formation |
| 2:30pm | Mike Grudić | STARFORGE |
| 3:00pm | coffee break + discussion | SIGOs star formation and the role of turbulence |
| 4:00pm | Breakout sessions - self-selective: | (1) technical questions on running codes break - helping session for running AREPO and/or STARFORGE if needed (2) strategic planning for the next ATP/NSF cycle |
Tuesday, March 28
| Time | Event/speaker | Details |
| 9:30am | Breakfast | |
| 10am | Claire Williams | DM GHOSts and their morphology/rotation |
| 10:30am | Shail Hegde | A Semi-Analytic Model for High-Redshift Star Formation |
| 11:00am | Federico Marinacci | Star formation and feedback/Zoom-in simulations |
| 11:30am | discussion | DM GHOSts - what are they? + star formation, and feedback in the presence of the stream velocity |
| 12:00am | Lunch break | Westwood or on campus |
| 2pm | Mark Vogelsberger | Alternative DM models |
| 2:30pm | Stephanie O'Neil | Exploring types of self-interacting dark matter in galaxy simulations, mainly Milky Way sized halos, maybe some dwarf galaxies |
| 3pm | coffee + discussion | Inclusion of alternative DM models |
| 4pm | Discussion | detectability (JWST) and other observational signatures |
Wednesday, March 29
| Time | Event/speaker | Details |
| 9:30am | Breakfast | |
| 10am | Discussion | The future of the collaboration, strategic planning for students conferences and networking |
| >=10:30am | Discussion | Proposal planning and writing session. Wrapup of the meeting |
