🔥The 9th Round of Easy Loan, Earn $40 Reward is in progress❗️ ⏰ Promotion Period: January 15th - Feburary 15th, 2025 👉 Register now and check more details at gate.io/campaigns/358

Huge congratulations to Prof. Daniel Baumann for receiving the prestigious Humboldt Research Award! 🥳🥳🥳 iop.uva.nl/content/news/2…

Please help to spreading the news! Institute of Physics National Institute for Subatomic Physics Nikhef Radboud University GRAPPA Centre Gianfranco Bertone Samaya Nissanke (she/her) 🕊️❤️ Kyle Cranmer Benjamin Wandelt Fabio Iocco Shirley Ho @R_Trotta

The abstract submission for the first European AI for fundamental physics conference (EuCAIFCon) is closing soon! (15 January)

Abstract submission closes today 23:59 CET.

⏳ Since not everybody could make it in time to register for EuCAIFCon, we extended the abstract submission deadline until Friday next week (26 Jan, 23:59 CET).

🎓 I just opened a PhD position in my group at GRAPPA Centre! On theoretical cosmology and deep learning. Application deadline: 29 February. More details here: vacatures.uva.nl/UvA/job/PhD-po…

In the case you missed this: Postdoc position on theoretical cosmology and deep learning with daan meerburg at RUG! Deadline is already in three days! rug.nl/about-ug/work-…

Matthew Schwartz, speaking about Theoretical High-Energy Physics and AI, and going from 'data science' to solving symbolic problems of #hepph and #hepth at #EuCAIFCon24

Great times at the #EUCaifCon24 poster session! Here some Quantum Universe students and collaborators showing off their recent work

Already last morning at #EUCAIFCon24 with IAIFI's Siddharth Mishra-Sharma reviewing AI & astroparticle physics

Now at #EuCAIFCon24: Kyle Cranmer's (Kyle Cranmer) outlook on AI for fundamental physics #AI4Science #EuCAIFCon

Kyle Cranmer getting ready to close the #eucaifcon24 conference in Amsterdam. Highlighting AI for lattice QCD simulations and the many initiatives in AI4Science

All active #NeutronStars should be surrounded by dense #AxionClouds if the axion has a mass in a specific range. This occurs because the polar caps of neutron stars produce axion clouds that are bound to the star and struggle to dissipate energy. 🔗 go.aps.org/4hbgocF