Events at Physics |
Events on Friday, September 18th, 2026
- Preliminary Exam
- Intersecting AI and high energy theoretical physics
- Time: 9:00 am - 11:00 am
- Place: 5280 Chamberlin
- Speaker: Haotian Cao, Physics PhD Graduate Student
- Abstract: Artificial intelligence (AI) is increasingly advancing research in theoretical physics and pure mathematics. In this talk, I'll present two uses of AI in the context of conformal field theory and scattering amplitudes.
We first discuss an inverse problem emerging in two-dimensional conformal field theory (CFT): reconstructing tensor products of CFTs from their low-lying spectra. We specifically focus on rational conformal field theories (RCFTs) such as Wess-Zumino-Witten models characterized by affine Kac-Moody algebras. The discrete and structured nature of this problem for RCFTs motivates a sequence-to-sequence Transformer architecture that maps spectral information to the constituent affine algebras and central charges. We further demonstrate the model's ability to generalize to theories with larger central charges and to theories with unseen affine algebras during training.
We then turn to the amplitude bootstrap for N=4 super Yang-Mills theory (SYM) in the planar limit. We use agentic AI workflow to prove a mathematical conjecture related to the construction of a good basis in this program. Rather than relying solely on informal mathematical proofs, we use a systematic and iterative agentic AI workflow that translates the conjecture into formal mathematical statements, identifies the required intermediate lemmas, and constructs and verifies their proofs. - Host: Kyle Cranmer
- Physics Department Colloquium
- Exploring the Extreme Universe with Gamma-ray Observatories
- Time: 3:30 pm - 4:30 pm
- Place: Chamberlin 2241 -
- Speaker: Reshimi Mukherjee, Columbia/Barnard College
- Abstract: Very-high-energy (VHE) gamma-ray astrophysics has emerged as an exciting and vital field, with major discoveries made through experiments in space and on the ground. In space, the Fermi gamma-ray telescope studies some of the most violent processes in the Universe, and explores nature's highest energy accelerators. At even higher energies, gamma-ray astronomy can be carried out using ground-based telescopes, which detect the flashes of blue light from air-showers caused by gamma rays impacting the upper atmosphere. Some of the most exciting sources detected at very high energies are blazars, with relativistic jets, and Galactic sources including supernova remnants, pulsar wind nebulae, and binary systems. Gamma-ray production in all these sources occurs due to particle acceleration in extreme conditions of gravitational or magnetic fields, implying the existence of shocks and cataclysmic explosions. Gamma-ray astronomy works synergistically with the study of ultra high energy cosmic rays and observation of the Universe with the elusive high-energy neutrino. Multi-messenger astronomy has emerged as one of the most effective ways to observe the Universe. This talk will outline the scientific motivation for high energy gamma-ray astronomy, describe the techniques involved, and survey the astrophysics of the extreme Universe, as revealed by observations made with gamma rays, in particular with the VERITAS observatory in southern Arizona. In addition, the talk will cover future prospects and new directions with the GRAMS project, next-generation mission for gamma-ray and antimatter studies using a liquid Argon (LAr) Time Projection Chamber (TPC), that will provide unprecedented sensitivity to gamma rays in the under-explored “MeV-gap” region in high energy astrophysics.
- Host: Ke Fang