Gertrude Scharff-Goldhaber Prize 2023 Ceremony
Tuesday 15 August 2023 -
12:00
Monday 14 August 2023
Tuesday 15 August 2023
12:00
Welcome
-
Jessica Gasparik
(
Brookhaven National Lab
)
Marc-André Pleier
(
BNL
)
Welcome
Jessica Gasparik
(
Brookhaven National Lab
)
Marc-André Pleier
(
BNL
)
12:00 - 12:10
Room: hybrid event - zoom and 510 LSR
12:10
Equity, Diversity and Inclusion at BNL
-
Dmitri Denisov
(
Brookhaven National Laboratory
)
Equity, Diversity and Inclusion at BNL
Dmitri Denisov
(
Brookhaven National Laboratory
)
12:10 - 12:20
Room: hybrid event - zoom and 510 LSR
12:20
Memories of Gertrude Scharff-Goldhaber
-
Michael H. Goldhaber
Alfred Scharff Goldhaber
(
SBU
)
Memories of Gertrude Scharff-Goldhaber
Michael H. Goldhaber
Alfred Scharff Goldhaber
(
SBU
)
12:20 - 12:30
Room: hybrid event - zoom and 510 LSR
12:35
Energy Dependence of Breit-Wheeler Process in Heavy-Ion Collisions and its Application to Nuclear Charge Radius Measurements
-
Xiaofeng Wang
(
Shandong Univeristy
)
Energy Dependence of Breit-Wheeler Process in Heavy-Ion Collisions and its Application to Nuclear Charge Radius Measurements
Xiaofeng Wang
(
Shandong Univeristy
)
12:35 - 12:55
Room: hybrid event - zoom and 510 LSR
The Breit-Wheeler process is the simplest process for creating matter and antimatter from the collision of two photons. This conversion of light into matter is a direct corollary of Einstein’s mass-energy equivalence, E = mc^2. The process was theorized in 1934, but went nearly a century without experimental confirmation until it was discovered by the STAR Collaboration at RHIC in 2021. This discovery was made at top RHIC energy in gold-gold collisions. While the process is now well established at high energies, there is a peculiar feature predicted by Quantum Electrodynamics (QED) that the interaction cross section will diverge (infrared divergence) at low photon energy. The flexibility of RHIC, allowing heavy-ion collisions at lower energies, allows this prediction to be tested and other characteristics of the newfound process to be uncovered. In this presentation, we will present measurements of the energy dependence of Breit-Wheeler process in gold-gold collisions at STAR. The corresponding results computed by QED are consistent with STAR measurements and found to be sensitive to the nuclear charge distribution. Following this approach we demonstrate that the experimental measurements of the Breit-Wheeler process in heavy-ion collisions can be used to quantitatively constrain the nuclear charge radius of high energy atomic nuclei.