2020 Fall Meeting of the APS Division of Nuclear Physics
Volume 65, Number 12
Thursday–Sunday, October 29–November 1 2020;
Time Zone: Central Time, USA
Session SE: Mini-Symposium: The Next Generation Nuclear Workforce II
10:30 AM–11:18 AM,
Sunday, November 1, 2020
Chair: Paul Gueye, MSU-NSCL/FRIB
Abstract: SE.00001 : Physicists Inspiring the Next Generation: Exploring the Nuclear Matter
10:30 AM–11:06 AM
Preview Abstract
Abstract
Author:
Yannick Gueye
(Michigan State University)
A joint collaboration between the National Society of Black Physicists
(NSBP) and the National Radio Astronomy Observatory (NRAO) launched a
two-week program geared toward middle and high school students in the Summer
2014. The program, known as ``Physicists Inspiring the Next Generation
(PING): Exploring the Cosmos'', involved 20 pre-college students and 4
undergraduate students. Students were tasked to collect data from the 21 cm
emission line of the hydrogen atom from specific locations in the universe
using the 40 ft radio-telescope of the Green Bank Observatory located in
Greenbank, WV. The program is now part of the outreach programs of NRAO and
is being held annually. In the Summer 2019, a one week-long pilot program
``Physicists Inspiring the Next Generation (PING): Exploring the Nuclear
Matter'' was conducted at the Facility for Rare Isotope Beams/National
Superconducting Cyclotron Laboratory in East Lansing, MI. The program
included 4 high school students and 2 undergraduate students. Students were
tasked to build two parallel plate avalanche chambers to be used as beam
monitoring systems for nuclear physics experiments conducted by the MoNA
Collaboration at this facility. One additional difference from the original
astronomy focused PING program is the extension of the high school students
beyond the summer that continued over the entire academic year. One student
was tasked to model one of the MoNA experiments scheduled in the Summer 2020
that will study $^{\mathrm{13}}$Be and his isomer using the Geant4 Monte
Carlo based G4beamline software and ROOT analysis tool. The setup consists
of six silicon detectors, a beryllium target, a cesium iodide calorimeter
and a veto scintillator. More specifically, the goal was to reconstruct the
momentum and angular distributions of all isotopes exiting the CsI and
depositing some energy in the veto detector. The PING program has inspired
several students to pursue an education in STEM, some currently pursuing
B.S. and Ph.D. degrees in physics and astronomy. We will provide an overview
of the PING program and highlight some personal experiences that make this
program very successful.