17–21 Jul 2023
Monash University
Australia/Melbourne timezone

Measurement of the anomalous spin precession frequency $\omega_a$ in the Muon $g-2$ experiment at Fermilab

19 Jul 2023, 11:05
15m
Monash University

Monash University

Talk Low energy Low energy

Speaker

Mr Lorenzo Cotrozzi (on behalf of the Muon g-2 collaboration) (University of Pisa and INFN Pisa)

Description

The muon anomaly, $a_\mu=(g_{\mu}-2)/2$, is a low-energy observable which can be both measured and computed to high precision, making it a sensitive test of the Standard Model (SM) and a probe for new physics. The current discrepancy between the experimental value and the Standard Model calculation from the Muon $g-2$ Theory Initiative [T. Aoyama et al. - Phys. Rep. 887, 1 (2020)] is $a_{\mu}^{exp}-a_{\mu}^{SM}=(251\pm59)\cdot10^{-11}$, with a significance of $4.2\,\sigma$.
The Fermilab E989 experiment aims, with the full statistical power, to measure $a_{\mu}$ with a precision of $140\,$parts per billion (ppb), a four-fold improvement with respect to the previous measurement at the Brookhaven E821 experiment (1997-2001).
In April 2021 the FNAL E989 collaboration published their first result, based on the first year of data taking (2018 campaign) [B. Abi et al. (Muon $g-2$ Collaboration), Phys. Rev. Lett. 126, 141801 (2021)], and this year a new result is expected to be published, based on the datasets collected during Run-2 and Run-3 (2019 and 2020 campaigns).
A $3.1$-GeV spin-polarized beam of muons is injected into a storage ring of $14\,$m of diameter, in the presence of a $1.45\,$T magnetic field. The anomaly $a_\mu$ can be extracted by accurately measuring the anomalous muon spin precession frequency, $\omega_a$, and the magnetic field environment using Nuclear Magnetic Resonance techniques. The measurement of $\omega_a$ is based on the arrival time distribution of decay positrons in the high-energy tail of the spectrum, observed by $24$ electromagnetic calorimeters that are placed around the inner circumference of the storage ring. The histogram of positron counts is fitted with a function that takes into account detector and beam dynamics effects.
This talk will present details about the improvements and upgrades to the positron reconstruction and to the $\omega_a$ analysis since the 2021 results, and it will describe the final statistical and systematic sources of uncertainty in the new result.

Primary author

Mr Lorenzo Cotrozzi (on behalf of the Muon g-2 collaboration) (University of Pisa and INFN Pisa)

Presentation materials