activity
20072026
most citedCharged-Particle Thermonuclear Reaction Rates: II. Tables and Graphs of Reaction Rates and Probability Density Functions

277 citations · 1k across the 32 of their papers we have counts for

collaborators

32 papers

nucl-ex2026

Core Breaking at Low Spin in Zn from Nuclear Resonance Fluorescence

S. R. Johnson, R. V. F. Janssens, B. A. Brown +11

Low-spin excited states in Zn have been studied at the High Intensity Gamma-Ray Source (HIS) from the ground state up to the particle emission threshold using the nuclear…

nucl-ex2025

Indirect Measurement of the Mg Direct Capture Reaction Rate via (He,d) Spectroscopy

Kaixin Song, Richard Longland, Caleb Marshall +3

The cross section of the reaction is dominated by direct capture at low energies relevant for stellar burning. Such cross sections can be constr…

nucl-ex2025

Investigation of P levels near the proton threshold by Nuclear Resonance Fluorescence and the impact on the Si(p,)P thermonuclear rate

David Gribble, Christian Iliadis, Robert V. F. Janssens +13

We investigated the nuclear structure of P near the proton threshold using Nuclear Resonance Fluorescence (NRF) to refine the properties of key resonances in the Si(p…

astro-ph.HE2025★ 1 cited

Low-metallicity nova explosions: a site for weak rp-process nucleosynthesis

Athanasios Psaltis, Jordi José, Richard Longland +1

Classical novae are common cataclysmic events involving a binary system of a white dwarf and a main sequence or red giant companion star. In metal-poor environments, these explosio…

nucl-ex2024

High Resolution Study of Ca to Constrain Potassium Nucleosynthesis in NGC 2419

William Fox, Richard Longland, Caleb Marshall +1

The globular cluster NGC 2419 was the first to exhibit a Mg-K anticorrelation, linked to hydrogen burning at temperatures between 80-260 MK. However, the key K-destroying reaction,…

nucl-ex2023★ 4 cited

Spin-parities of sub-threshold resonances in the F(p, )O reaction

F. Portillo, R. Longland, A. L. Cooper +4

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