Features Nano Astrophysics Nuclear Physics Theoretical Physics Featured Courses Home The Department of Physics and Astronomy - http://www.physics.unc.edu
 
side

Search the Site

Printer-Friendly Version

Home

Photonuclear Physics

The Photonuclear Group makes use of the world class High Intensity γ ray Source (HIγS) operated at the Triangle Universities Nuclear Laboratory to address many different problems. Below is an overview of the different problems being investigated by the group. To view more about a topic, simply click on the link to find out more information.
Homeland Security In today's post-9/11 world, the US has an ongoing program to reduce the threat of domestic nuclear terrorism. The Photonuclear Group actively participates in this program by measuring nuclear data required to improve the effectiveness of new detection technologies.
Photofission Photons are an excellent probe to investigate fission at excitation energies near the fission barrier. Because electromagnetic transitions selectively populate a relatively few number of nuclear levels, fission induced by photons exhibit very interesting phenomena such as anisotropic angular distributions. UNC is actively involved in empirical studies to understand the implications these distributions have on the fission process.
48Ca 48Ca is a medium mass nucleus which has the special property of being doubly magic, the number of protons and neutrons completely fill their respective nuclear shells just as a electrons fill the p level of a noble gas. It is the most neutron rich, stable isotope of the Ca isotopic chain which begins with the doubly magic 40Ca. Because of this, it is a very important nucleus to understanding nuclear fp shell. The Photonuclear Group measures photoabsorption observables which help in the understanding of the complex level structures of medium to heavy nuclei.
9Be There are no stable nuclei in the universe composed of 5 or 8 nucleons. The existence of nuclei with mass greater than 8 in the present universe requires that these so called "mass gaps" were bridged over following the Big Bang. The α(αn,γ)9Be and 8Be(n,γ) are vital to traversing this and the Photonuclear Group seeks to study them via the inverse reaction 9Be(γ,n).
 
Maintained by: webmaster@physics.unc.edu  |  Last updated: 9 December, 2011