10 October 2022 to 31 December 2028
Zoom Webinar
Europe/London timezone

High performance computing in the muon g-2 experiment at Fermilab

Date: Tuesday 10 October 2023 at 15:00 (Europe/London)
Speaker: Dr Saskia Charity, Senior Research Associate in the particle physics cluster at the University of Liverpool

Abstract

Despite being enormously successful over the last century, the Standard Model (SM) of Particle Physics has several major deficiencies. With nothing to say about Dark Matter or Dark Energy, which make up over 95% of the universe, the field of particle physics is charged with finding “new physics” which is missing from the SM. By making ultra-precise measurements and comparing them with SM predictions, we can perform robust tests of the SM and try to determine significant discrepancies that point to the existence of new physics.

The Muon g–2 Experiment at Fermilab recently published the measurement of the muon anomalous magnetic moment to 0.20 parts-per-million (ppm). This is the most precise measurement ever made at a particle accelerator. The measurement represents a dataset of 100 billion decay positrons, recorded using electromagnetic calorimeters. The result is dominated by the statistical uncertainty and over the next few years this is expected to halve when the total dataset which contains over 3x as much data, has been analysed. By this time, uncertainties in the theoretical prediction should be at a comparable level to the experimental precision, enabling a stringent test of the SM that could provide a clear signal of new physics. There has been widespread excitement in this result worldwide, appearing in media from the BBC News to the New York Times.

This seminar will cover the numerous major high-performance computing requirements associated with making such a precise measurement. One example is data storage and processing: the total dataset contains 7 PB of raw data (4.5 million files) which must be reconstructed and analysed efficiently. This involves a multi-stage parallel workflow of 5000 jobs using grid computing, and the automated staging of data from tape storage to analysis machine. Another example is data collection: the experiment records 2GB of data every 8 seconds, which must be transferred to offline storage efficiently to prevent a backlog that prevents recording more data. The online computing requirements and fast reconstruction for data quality monitoring will be presented. Finally, the analysis strategy for making the final measurement will be presented, which includes several cutting-edge techniques including Artificial Intelligence/Machine Learning and GPU processing.

In particular, we will see how deep generative models can be embedded within principled physical Bayesian modelling to solve a number of astronomical ill-posed inverse problems ranging from de-blending galaxy images, all the way to inferring the distribution of dark matter from weak gravitational lensing measurements. Dr Lanusse will also illustrate how the same generative modelling techniques can alleviate the need for analytic likelihoods in cosmological inference, enabling instead Simulation-Based Inference in which the physical model is implemented in the form of a numerical simulator. And finally, he will highlight the power of the computational frameworks initially developed for Deep Learning when applied to physical modelling, with applications ranging from speeding up cosmological MCMCs to performing inference over the initial conditions of N-body simulations.

The talk is now available on YouTube: https://youtu.be/E1q-MkNsRSY 

 

Biography

Dr Saskia Charity is a senior Research Associate in the Particle Physics Cluster at the University of Liverpool, working on the g-2 and mu2e experiments at Fermilab and the MUonE experiment at CERN. Between 2018-2022 she was a Fermilab post-doc in the Muon Department, where she worked on many different aspects of the g-2 experiment. She is the analysis coordinator for the magnetic field analysis in the g-2 experiment. She received her Ph.D. from the University of Liverpool where she worked on track reconstruction algorithms for the g-2 straw tracking detectors. She received her MPhys in Physics with Philosophy from the University of York in 2014.