Theory Seminar
Random unitaries in extremely low depth
-
Demonstrating fast thermalization of the magic and output distributions of random quantum circuits.
-
Efficient implementations of classical shadow tomography.
-
New superpolynomial quantum learning advantages.
-
Establishing computational hardness for recognizing phases of matter in quantum experiments.
Universal Signatures of First-Order Phase Transitions in Cosmology
Simulations of Gauge Theories on Quantum Computers
Gauge theories describe the fundamental interactions, but their complexity makes questions involving real-time dynamics beyond the reach of classical computation. Quantum computers open a new path by naturally representing quantum fields and evolving them in real time thus circumventing for example the sign problem that limits classical Monte Carlo methods. In this talk, we will discuss the challenges and recent progress in encoding and simulating Gauge theories on fault-tolerant quantum computers.
Uncertainty-aware generative models for autonomous discovery in particle theory
The Fermi Function, Factorization and the Neutron’s Lifetime
The neutron lifetime is a precision observable of the Standard Model probing the CKM matrix element |Vud| and beyond the Standard Model physics. For nuclear beta decay, in the region of small electron velocity or the limit of large nuclear charge Z, a Fermi function is used to account for enhanced perturbative effects. In this talk, I will present the derivation of the quantum field theoretic analog of the Fermi function valid for neutron beta decay in which neither of the aforementioned limits apply. This QFT analog is related to renormalization group effects of objects occurring in the context of a factorization formula valid in the limit of small electron mass. I will introduce this factorization formula and present results through two-loop order. The main phenomenological results are two-loop input to the long-distance corrections to neutron beta decay and an accompanying calculation of |Vud|.
Temperature-Resistant Order in 2+1 Dimensions
High temperatures are typically thought to increase disorder. Here we examine this idea in Quantum Field Theory in 2+1 dimensions. For this sake we explore a novel class of tractable models, consisting of nearly-mean-field scalars interacting with critical scalars. We identify UV-complete, local, unitary models in this class and show that symmetry breaking $\mathbb{Z}_2 \to \emptyset$ occurs at any temperature in some regions of the phase diagram. This phenomenon, previously observed in models with fractional dimensions, or in the strict planar limits, or with non-local interactions, is now exhibited in a local, unitary 2+1 dimensional model with a finite number of fields.
Fractionally Charged Particles at the Energy Frontier
The pattern in the Standard Model (SM) charges can be traced to an ambiguity in the gauge group of the SM. The easiest way to resolve this ambiguity would be to discover a particle with electric charge that is an integer multiple of e/6 (beyond +/- e, 0). The discovery of such fractionally charged particles would also challenge and potentially rule out many minimal unification models. In this talk I will review the connection between the `global structure' of the SM and the charges particles can have, then explore the phenomenology of fractionally charged particles, focusing on the constraints provided by current searches at the Large Hadron Collider (LHC). By reinterpreting existing results, we assess the bounds on various fractionally charged representations, uncovering scenarios where collider limits are unexpectedly weak or entirely absent.
Status update on the muon g-2
I will summarize the discussions at the recent plenary workshop at KEK and give an update of recent lattice calculations.
Prospects of supermassive millicharged particles as dark matter
We explore the prospects of very heavy millicharged particles as candidates for some or all of dark matter (DM). Constraints on their properties like charge, dipole moment and mass are obtained by translating the current limits set by state-of-the-art nuclear recoil experiments like XENONnT and LZ. We contrast the extracted limits with those coming from astrophysical considerations, such as the decoupling of DM from regular matter during the recombination epoch and the suitability of the dynamical environments in the galactic halo for these heavy and charged beyond the Standard Model particles to remain lodged-in and available for future detections.
Thanks!