Monday, November 21, 2022
4:10PM - 4:23PM
|
|
T11.00001: Convectively-driven internal gravity waves in a massive star
Evan H Anders, Daniel Lecoanet, Keaton J Burns, Jeff S Oishi, Geoffrey Vasil, Benjamin P Brown
|
Monday, November 21, 2022
4:23PM - 4:36PM
|
|
T11.00002: Automatic spectral methods for non-radial structure and stability problems
Keaton J Burns, Daniel Lecoanet, Geoffrey Vasil, Benjamin P Brown, Jeff S Oishi
|
Monday, November 21, 2022
4:36PM - 4:49PM
|
|
T11.00003: Propagation of a Thermohaline Mixing Front in 3D DNS and 1D Models
Imogen G Cresswell, Adrian E Fraser, Evan H Anders, Benjamin P Brown
|
Monday, November 21, 2022
4:49PM - 5:02PM
|
|
T11.00004: Layer formation in a stably-stratified fluid cooled from above. Towards an analog for Jupiter and other gas giants
Rafael Fuentes, Andrew Cumming, Evan H Anders
|
Monday, November 21, 2022
5:02PM - 5:15PM
|
|
T11.00005: A `dark-energy-free` turbulence similarity solution for an infinite homogeneous expanding universe using Einstein's Averaged Field Equations
William K George, Gunnar Johansson
|
Monday, November 21, 2022
5:15PM - 5:28PM
|
|
T11.00006: The Stability of Prendergast Magnetic Fields
Emma Kaufman, Daniel Lecoanet, Evan H Anders
|
Monday, November 21, 2022
5:28PM - 5:41PM
|
|
T11.00007: Inferring Stellar Magnetic Fields with Magnetic - Internal Gravity Wave Interactions
Daniel Lecoanet, Ian Freeman, Dominic Bowman, Timothy Van Reeth
|
Monday, November 21, 2022
5:41PM - 5:54PM
|
|
T11.00008: Hydrodynamic stability constraints on the three-dimensional structure of planetary vortices
Aidi Zhang, Philip S Marcus
|
Monday, November 21, 2022
5:54PM - 6:07PM
Not Participating
|
|
T11.00009: The influence of density ratio on instabilities present in supernova remnants.
Samuel Petter, Quinton Dzurny, Gokul Pathikonda, Benjamin Musci, Devesh Ranjan
|
Monday, November 21, 2022
6:07PM - 6:20PM
|
|
T11.00010: Internal Heating, why Convective Driving Models Matter for Astrophysics
Whitney T Powers, Evan H Anders, Benjamin P Brown
|
Monday, November 21, 2022
6:20PM - 6:33PM
|
|
T11.00011: Predicting the dark matter particle mass, size, and other properties from the mass and energy cascade and two-thirds law in dark matter flow
Zhijie Xu
|
