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202 FRIB Graduate Brochure

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Christopher Wrede<br />

Professor of Physics<br />

Keywords: Nuclear Astrophysics, Thermonuclear Reaction Rates, Fundamental<br />

Symmetries, Beta Decay<br />

Experimental Nuclear Physics<br />

About<br />

• MSc, Physics, Simon Fraser University, 2003<br />

• MS, M. Phil., Physics, Yale University, 2006<br />

• PhD, Physics, Yale University, 2008<br />

• Joined the laboratory in August 2011<br />

• wrede@frib.msu.edu<br />

Research<br />

How Students can Contribute as Part<br />

of my Research Team<br />

Students in our group have opportunities to propose,<br />

prepare, execute, analyze, and interpret nuclear-physics<br />

experiments at <strong>FRIB</strong> and other laboratories, to publish<br />

the results in leading scientific journals, and to present<br />

the results at national and international conferences. Our<br />

alumni have advanced to positions in national laboratories,<br />

academic institutions, and industry.<br />

Our research focuses on studying nuclei experimentally<br />

to probe fundamental questions about our Universe.<br />

For example, we measure nuclear reactions, decays, and<br />

masses in the laboratory to learn about the reactions<br />

that power exploding stars or affect their synthesis of<br />

chemical elements. In the near future, our program at<br />

<strong>FRIB</strong> will be focused on measuring the beta and electroncapture<br />

decays of proton-rich nuclides using the GADGET<br />

and PXCT detection systems. With these experiments, we<br />

hope to constrain the nuclear-structure details that are<br />

most influential on photodisintegration in supernovae<br />

and the explosive burning of hydrogen and helium on the<br />

surfaces of accreting compact stars such as white dwarfs<br />

and neutron stars. Similar experiments can allow us to<br />

test hypotheses that could explain the origins of dark<br />

matter in the universe or to better constrain the effects<br />

of isospin-symmetry breaking in nuclei on tests of the<br />

unitarity of the Cabibbo-Kobayashi-Maskawa matrix, a<br />

cornerstone of the Standard Model.<br />

Biography<br />

I was born in Vancouver, Canada, to Finnish parents,<br />

and began my research career in experimental nuclear<br />

astrophysics at Canada’s TRIUMF laboratory. In 2008,<br />

I obtained a PhD in Physics from Yale University based<br />

on work at the Wright Nuclear Structure Laboratory<br />

in the same research field. From there, I moved to<br />

a postdoctoral Research Associate position at the<br />

University of Washington’s Center for Experimental<br />

Nuclear Physics and Astrophysics. Since 2011, I have been<br />

leading a research group at NSCL and <strong>FRIB</strong> with a primary<br />

interest in nuclear astrophysics and secondary interests in<br />

fundamental symmetries and nuclear structure.<br />

The Gaseous Detector with Germanium Tagging<br />

(GADGET) prior to an <strong>FRIB</strong> experiment to determine the<br />

isotopic ratios expected in microscopic grains of stardust.<br />

Selected Publications<br />

Low-energy<br />

23<br />

Al B-delayed proton decay and<br />

22<br />

Na<br />

destruction in novae, M. Friedman et al., Phys. Rev. C 101,<br />

052802(R) (<strong>202</strong>0)<br />

GADGET: a Gaseous Detector with Germanium Tagging, M.<br />

Friedman et al., Nucl. Instrum Methods Phys. Res., Sect. A<br />

940, 93 (2019)<br />

Doppler Broadening in 20 Mg (B, p, y) 19 Ne Decay, B. E.<br />

Glassman, D. Perez-Loureiro, C. Wrede et al., Phys. Rev. C<br />

99, 065801 (2019)<br />

80<br />

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