Synopsis: Nuclear star gazing

The study of reaction rates between unstable, light nuclei can lead to a better understanding of thermonuclear processes in massive stars and novae.
Synopsis figure
Illustration: NASA

Calculating thermonuclear reaction rates in stars requires detailed information about the cross sections for the relevant reactions. However, the nuclei involved in these reactions are often unstable and thus difficult to produce as a beam or target. While many researchers are actively pursuing new facilities to produce such radioactive beams, in some cases important nuclear physics information can be determined indirectly. In a paper appearing in Physical Review C, Christopher Wrede, now at the University of Washington, and collaborators at Yale University and TRIUMF in Vancouver, Canada, determine the reaction rate for proton capture by 30P that leads to 31S and a photon [the reaction is represented symbolically by 30P(p,γ)31S ]. They do this by measuring the detailed level structure in 31S using reactions with stable nuclear targets, even though 30P itself is unstable.

The 30P(p,γ)31S reaction is crucial to understanding nucleosynthesis in certain explosive environments such as novae, Type I x-ray bursts, and Type II supernovae. The authors use reactions involving stable 31P and 32S targets—in particular the 31P(3He,t)31S, 31P(3He,t)31S*(p)30P, and 32S(d,t)31S reactions—to extract resonance energies, spins, and proton branching ratios, which yield new information on the 30P(p,γ)31S reaction in the temperature range between ten million and ten billion degrees. They compare the measurements to nuclear statistical model calculations. Generally, statistical models are not useful for studying lighter nuclear systems where the level density is low, but the good agreement with Wrede et al.’s results suggest that the nuclear statistical model can be used for some lighter systems. – Brad Filippone


More Features »


More Announcements »

Subject Areas

Nuclear Physics

Previous Synopsis

Fluid Dynamics

Viscous pull

Read More »

Next Synopsis

Statistical Physics

Forget them not

Read More »

Related Articles

Focus: Proton-Neutron Equilibration Takes Just 0.3 Zeptoseconds
Nuclear Physics

Focus: Proton-Neutron Equilibration Takes Just 0.3 Zeptoseconds

The equilibration of nuclei containing a large imbalance of protons and neutrons can occur in 3×10−22 seconds, according to experiments—important information for models of element-creation in supernovae. Read More »

Synopsis: Starting Fluid for Laser Fusion
Energy Research

Synopsis: Starting Fluid for Laser Fusion

A laser-based fusion experiment demonstrates that liquid fuel capsules could rectify problems encountered with ice-based fuel capsules. Read More »

Focus: More Hints of Exotic Cosmic-Ray Origin

Focus: More Hints of Exotic Cosmic-Ray Origin

New Space Station data support a straightforward model of cosmic-ray propagation through the Galaxy but also add to previous signs of undiscovered cosmic-ray sources such as dark matter. Read More »

More Articles