| September 2023 |
| Monday | Tuesday | Wednesday | Thursday | Friday |
| 28 , A Quantum Al-Khawarizm for Spacetime: A Workshop on von Neumann Algebras in Quantum Field Theory & Gravity (9:00 AM - 6:00 PM) + Abstract: | 29 , A Quantum Al-Khawarizm for Spacetime: A Workshop on von Neumann Algebras in Quantum Field Theory & Gravity (9:00 AM - 6:00 PM) + Abstract: | 30 , A Quantum Al-Khawarizm for Spacetime: A Workshop on von Neumann Algebras in Quantum Field Theory & Gravity (9:00 AM - 6:00 PM) + Abstract: | 31 | 1 |
| 4 | 5 | 6 Taeho Ryu, Two types of nuclear transients - tidal disruption events and disruptive collisions (12:30 PM - 1:00 PM) + Abstract: , HEP Journal Club (12:30 PM - 1:30 PM) Bobby Acharya, Model G2-holonomy Singularities, M-theory and QFT’s in 3,4 and 5 dimensions. (2:00 PM - 3:15 PM) + Abstract: Jack Donahue, Zig Zag Zug (5:00 PM - 7:00 PM) + Abstract: | 7 Daniel Rokhsar, The Past Has Left Its Traces On The World, And We Only Have To Know How To Read Them (4:00 PM - 5:30 PM) + Abstract: | 8 |
| 11 Michael Blanton, Intro to the CCPP (12:30 PM - 1:30 PM) + Abstract: | 12 Kaze Wong, Challenges and Opportunities from gravitational waves: data scientists on diet (2:00 PM - 3:15 PM) -- Abstract: The gravitational wave (GW) community has made numerous exciting discoveries in the past 7 years, from the first detection to a catalog of ~80 GW events, containing all sorts of surprises such as binary neutron stars and neutron star-black hole mergers. In the coming decade, there will be next-generation facilities such as the third-generation GW detectors network and space-based GW observatory, that will provide many more surprising events. There are quite a number of open modeling and data analysis problems in GW that await to be solved in order to unlock the full potential of next-generation detections. Despite the recent rapid development of machine learning and efforts trying to solve these problems in GW, it seems GW has a number of traits that make applying machine learning to GW difficult. In this talk, I will discuss a number of challenges and opportunities in GW, and some insights from GW on how we should apply modern techniques such as machine learning to physical science in general. Tom Shachar, RG flows on two-dimensional spherical defects (3:30 PM - 4:45 PM) + Abstract: Calvin Chen, How to "See" a Black Hole? (8:00 PM - 9:30 PM) + Abstract: | 13 , HEP Journal Club (12:30 PM - 1:30 PM) Da Liu, Search for light dark matter with quadratic interactions (2:00 PM - 3:15 PM) + Abstract: Gaston Giribet (4:00 PM - 6:00 PM) | 14 Laure Zanna, Discovering new physics from data for improved multiscale climate simulations (4:00 PM - 5:30 PM) + Abstract: | 15 Gleb Aminov, What languages do black holes speak? (1:30 PM - 2:30 PM) + Abstract: |
| 18 Michael Blanton, Mini-Symposium: Center for Cosmology & Particle Physics (12:30 PM - 2:00 PM) + Abstract: | 19 Nia Imara, A Star is Born (2:00 PM - 3:15 PM) + Abstract: | 20 , HEP Journal Club (12:30 PM - 1:30 PM) Hirosi Ooguri, Symmetry Resolution at High Energy (2:00 PM - 3:15 PM) + Abstract: , CCPP Pheno Journal Club (3:30 PM - 4:30 PM) | 21 Hiroshi Oguri, Constraints on Quantum Gravity (4:00 PM - 5:30 PM) + Abstract: | 22 Popov, Postdoc HepTh Discussion Group (12:00 PM - 1:30 PM) |
| 25 Ahmed Almheiri, The black hole information non-paradox (12:30 PM - 1:30 PM) Jordan Flitter, Searching for dark matter signatures in the 21cm signal (2:00 PM - 2:30 PM) + Abstract: | 26 Giulio Fabbian, (Towards) Cosmology and astrophysics with the Euclid mission (2:00 PM - 3:15 PM) + Abstract: | 27 , HEP Journal Club (12:30 PM - 1:30 PM) Josh Foster, Multiscale and Multiphysics Simulations for BSM Cosmology and Phenomenology (2:00 PM - 3:15 PM) + Abstract: Gabriele Rigo, The Two Scales of New Physics in Higgs Couplings (3:30 PM - 4:30 PM) + Abstract: | 28 Christopher Tiede, Binary Black Hole Accretion (12:30 PM - 1:00 PM) + Abstract: Miles Stoudenmire, Quantum Computing on Classical Machines with Tensor Networks (4:00 PM - 5:30 PM) + Abstract: | 29 Popov, Postdoc HepTh Discussion Group (12:00 PM - 1:30 PM) Zare (3:30 PM - 5:00 PM) |