New experimental methods and techniques, combined with the development of new
theoretical tools, have opened new avenues to explore nuclear reactions of significance for …

Classical novae are fascinating stellar explosions at the crossroads of stellar astrophysics,
nuclear physics, and cosmochemistry. In this review, we briefly summarize 30 years of …

Numerical values of charged-particle thermonuclear reaction rates for nuclei in the A= 14 to
40 region are tabulated. The results are obtained using a method, based on Monte Carlo …

The nuclear physics input used to compute the Monte Carlo reaction rates and probability
density functions that are tabulated in the second paper of this series (Paper II) is presented …

The quest to comprehend how nuclear processes influence astrophysical phenomena is
driving experimental and theoretical research programs worldwide. One of the main goals in …

The F 18 (p, α) O 15 reaction is key to determining the F 18 abundance in classical novae.
However, the cross section for this reaction has large uncertainties at low energies largely …

Knowledge of the F 18 (p, α) O 15 and F 18 (p, γ) Ne 19 astrophysical reaction rates are
important to understand γ-ray emission from nova explosions and heavy-element production …

The 18 F (p, α) 15 O reaction rate is crucial for understanding the final abundance of F 18
predicted by nova models. The γ-ray emission in the first few hours after a nova outburst is …

Nuclear astrophysics recently celebrated its 100th anniversary and remains an active field of
science. This article reviews several contemporary experimental techniques used to …

The TRIUMF-ISAC radioactive beam facility provides reaccelerated beams in the energy
range from 0.15 to 5 A MeV for A< 30 to a full suite of world class experimental apparatus …