Bulletin of the American Physical Society
Fall 2022 Meeting of the APS Division of Nuclear Physics
Volume 67, Number 17
Thursday–Sunday, October 27–30, 2022; Time Zone: Central Daylight Time, USA; New Orleans, Louisiana
Session EA: Probing Nuclear Geometry with Photons from JLab to RHIC and LHC
10:30 AM–12:18 PM,
Friday, October 28, 2022
Hyatt Regency Hotel
Room: Celestin D
Chair: Janet Seger, Creighton University
Abstract: EA.00002 : Discovery of the Breit-Wheeler Process and its Application to Nuclear Charge and Mass Radii Measurements*
11:06 AM–11:42 AM
Presenter:
Daniel Brandenburg
(Brookhaven National Laboratory)
Author:
Daniel Brandenburg
(Brookhaven National Laboratory)
Collaboration:
STAR Collaboration
In this talk I present the recent discovery of the Breit-Wheeler process by the STAR collaboration achieved by harnessing photons manifest from the ultra-Lorentz boosted Coulomb fields of colliding heavy nuclei. In this experimental setup, the linear polarization of the colliding photons leads to an angular modulation in the momentum of the produced electron-positron pairs that uniquely identifies the Breit-Wheeler process. Furthermore, the momentum distribution of the produced electron-positron pairs provides precise information about the spatial distribution of the colliding electromagnetic fields and the underlying nuclear charge distributions - information which at first seems to violate the uncertainty principle.
The discovery of the Breit-Wheeler process also provides a novel tool for studying the mass distribution of heavy nuclei at high energies and helps resolve a decade long puzzle -- the anomalously large nuclear mass radii extracted from photonuclear interactions in heavy-ion collisions. By utilizing a technique in photonuclear interactions that was developed for the Breit-Wheeler process which is sensitive to photon polarization, it is possible to measure the mass radii of large nuclei at high energy to sub-femtometer precision. Finally, I'll close with perspectives on photon physics in existing and future high energy experiments.
*DOE Office of Science: DE-FG02-10ER41666
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