| March 2025 |
| Monday | Tuesday | Wednesday | Thursday | Friday |
| 3 Roman Scoccimarro, Pairwise velocities at infinity and the redshift-space power spectrum (12:30 PM - 1:30 PM) | 4 JJ Zanazzi, Resonance locking and hot Jupiters (2:00 PM - 3:15 PM) + Abstract: | 5 Giorgio Gratta, nEXO and the quest for neutrino-less double beta decay. (2:00 PM - 3:15 PM) + Abstract: | 6 Janosz Dewberry, Shake, rattle, and roll: waves, tides, and turbulence in stellar and planetary system (1:00 PM - 2:15 PM) + Abstract: Giorgio Gratta, Testing Gravity at Ever Shorter Scale: A Trip into Exotic Experimental Physics (4:00 PM - 5:30 PM) + Abstract: | 7 Cara Giovanetti, Cosmology, Astrophysics, and Computation to Advance the Detection Prospects of Dark Matter (10:30 AM - 12:30 PM) + Abstract: Calkins (3:30 PM - 4:30 PM) |
| 10 Jesse Liu, Colliding light to measure tau g–2 (12:30 PM - 1:30 PM) + Abstract: | 11 Richard Anantua, A Message from the Horizon Scale by EHT: Deciphering Observational Signatures of Sgr A* and M87* (2:00 PM - 3:15 PM) + Abstract: Mathew Calkins, Office Hours (5:30 PM - 6:30 PM) | 12 , HEP Journal Club (12:30 PM - 1:30 PM) Junwu Huang, Novel string production mechanisms & gravitational wave detectors (2:00 PM - 3:15 PM) + Abstract: Mathew Calkins, Office Hours (4:30 PM - 5:30 PM) | 13 Jacob Barandes, What's Wrong with Quantum Theory, and How to Fix It (4:00 PM - 5:30 PM) + Abstract: | 14 Calkins (3:30 PM - 4:30 PM) |
| 17 Anthony Pullen, Probing Dusty Galaxies with FIR Surveys (12:30 PM - 1:30 PM) | 18 Tony Zhou (host), ACT DR6 Webinar Inbox (11:00 AM - 12:30 PM) + Abstract: Carol Cuesta Lazaro, Beyond the Observable: A Machine Learning Perspective on Modern Cosmology (11:15 AM - 12:30 PM) + Abstract: | 19 , HEP Journal Club (12:30 PM - 1:30 PM) Daniel Harlow, Quantum mechanics and observers for gravity in a closed universe (2:00 PM - 3:15 PM) + Abstract: | 20 | 21 Tianli Wang, A CFT Dual for Celestial MHV Amplitudes (1:00 PM - 2:00 PM) + Abstract: Calkins (3:30 PM - 4:30 PM) |
| 24 , SPRING BREAK; Campus Closed Rhine Samajdar (2:00 PM - 3:15 PM) | 25 , SPRING BREAK; Campus Closed | 26 , SPRING BREAK; Campus Closed | 27 , SPRING BREAK; Campus Closed | 28 , SPRING BREAK; Campus Closed Calkins (3:30 PM - 4:30 PM) |
| 31 Connor Hainje, A new formula for the area of a triangle, and applications (12:30 PM - 1:30 PM) Aurelio Amerio, Searching dark matter subhalos among unassociated Fermi-LAT sources (2:00 PM - 3:00 PM) + Abstract: William Pannell, Gradient flow and the curvature of theory space (3:10 PM - 4:10 PM) + Abstract: | 1 Bart Ripperda, Are We There Yet? First-principles Modeling of Multimessenger sSignals in the Plasma Universe (11:00 AM - 12:15 PM) + Abstract: Raagini Patki, A Novel Bispectrum extracting the Kinematic SZ effect as a Cosmological Probe (2:00 PM - 2:30 PM) + Abstract: | 2 , HEP Journal Club (12:30 PM - 1:30 PM) Csaba Csaki, Exploring QCD-like dynamics from supersymmetric cousins (2:00 PM - 3:15 PM) -- Abstract: Understanding the dynamics of QCD and the effects of confinement is one of the important remaining challenges for standard model physics. Here I will explain how some of these questions can be addressed in a cousin of ordinary QCD which is obtained by starting from a supersymmetric version, and then gradually breaking supersymmetry via anomaly mediation. These theories have phases identical to QCD, though the underlying dynamics causing confinement may be different. Within these theories one can find the eta' potential and theta dependence and address the phase structure of spontaneous CP breaking at theta = Pi. One can also derive the analog of the chiral Lagrangian, and explicitly check the magnitude of a dynamically generated up mass. Surprisingly we find that within these models the dynamically generated up quark mass could be sufficiently large to account for the entire up mass. | 3 Alessandra Buonanno, Theoretical Challenges in Gravitational-Wave Astronomy (4:00 PM - 5:30 PM) + Abstract: | 4 Dalimil Mazac, Spectral gaps and conformal field theory (10:00 AM - 11:15 AM) + Abstract: Calkins (3:30 PM - 4:30 PM) |