Yes that’s a USC Rosary 📿 he’s holding.
Yes that’s a USC Rosary 📿 he’s holding.
From folks in the writing program helping students communicate, listen, speak, and write… to physicists working on superconducting qubits, it was an amazing celebration of excellence in the liberal arts @usc.edu
From folks in the writing program helping students communicate, listen, speak, and write… to physicists working on superconducting qubits, it was an amazing celebration of excellence in the liberal arts @usc.edu
arxiv.org/abs/2506.08508
arxiv.org/abs/2506.08508
www.eventbrite.com/e/math-and-d...
www.eventbrite.com/e/math-and-d...
uci.edu/climate-coll...
uci.edu/climate-coll...
This NSF-funded facility will enable rapid sample analysis to inform climate change and air quality research. 🌎🌳☀️
This NSF-funded facility will enable rapid sample analysis to inform climate change and air quality research. 🌎🌳☀️
** Implications for testing #darkmatter models using dark matter structures in the vicinity of the Sun.
arxiv.org/abs/2503.10766
** Implications for testing #darkmatter models using dark matter structures in the vicinity of the Sun.
arxiv.org/abs/2503.10766
-> We are able to produce enough thin disks at the Milky Way scale
-> Do NOT produce enough thin galaxies at lower masses.
-> We are able to produce enough thin disks at the Milky Way scale
-> Do NOT produce enough thin galaxies at lower masses.
-> Massive galaxies form their stars in disks.
-> Middle size galaxies form stars in elongated pickle-like configurations.
-> Low-mass galaxies form stars in spheroids.
-> Massive galaxies form their stars in disks.
-> Middle size galaxies form stars in elongated pickle-like configurations.
-> Low-mass galaxies form stars in spheroids.
arxiv.org/abs/2503.05612
arxiv.org/abs/2503.05612
-> We are able to produce enough thin disks at the Milky Way scale
-> Do NOT produce enough thin galaxies at lower masses.
** Low-mass disk issue could be a significant problem for FIRE+LCDM simulations. Need more higher resolution runs to make sure.
-> We are able to produce enough thin disks at the Milky Way scale
-> Do NOT produce enough thin galaxies at lower masses.
** Low-mass disk issue could be a significant problem for FIRE+LCDM simulations. Need more higher resolution runs to make sure.
-> Massive galaxies form their stars in disks.
-> Middle size galaxies form stars in elongated pickle-like configurations.
-> Low-mass galaxies form stars in spheroids.
-> Massive galaxies form their stars in disks.
-> Middle size galaxies form stars in elongated pickle-like configurations.
-> Low-mass galaxies form stars in spheroids.
Asst Prof Sue Sim - Early Career Research
Prof Alessandra Pantano - Teaching
Asst Prof Christopher Miles - Early Career Teaching
Asst Prof Sue Sim - Early Career Research
Prof Alessandra Pantano - Teaching
Asst Prof Christopher Miles - Early Career Teaching
lnkd.in/guVq9w9E
lnkd.in/guVq9w9E