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From the 1 of 14 linked papers with an AI index.

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20242026
most citedThe 2025 Evaluation of Experimental Thermonuclear Reaction Rates (ETR25)

1 citations · 1 across the 6 of their papers we have counts for

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nucl-ex2026

Direct Measurement of the CuNi Excitation Function to Constrain the Ni--Cu Cycle Strength and Its Impact on Explosive Nucleosynthesis

E. Lopez-Saavedra, M. L. Avila, W. -J. Ong +21

A new direct measurement of the 59Cu(p,a)56Ni excitation function from 2.43-5.88 MeV in the center-of-mass was performed in inverse kinematics using the high-efficiency MUSIC activ…

nucl-ex2026

-delayed proton pandemonium: A first detailed Cl()P decay scheme

Tamas Budner, Moshe Friedman, Lijie Sun +20

Positron decays of proton-rich nuclides exhibit large values, producing complex cascades which frequently involve various radiations, including protons and rays. Often, on…

nucl-ex20252 cited

Constraining the Synthesis of the Lightest p Nucleus 74Se

A. Tsantiri, A. Spyrou, E. C. Good +42

We provide the first experimental cross section of the reaction to constrain one of the main destruction mechanisms of the p nucleus $^{74}\tex…

nucl-ex20259 cited

First Proton-Induced Cross Sections on a Stored Rare Ion Beam: Measurement of 118Te(p,γ) for Explosive Nucleosynthesis

F. Dellmann, J. Glorius, Yu. A. Litvinov +75

We present the first nuclear cross-section measurements of (p,γ) and (p,n) reactions on 118Te at energies relevant for the γ-process nucleosynthesis. Absolute cross-section value…

nucl-ex2025

Bayesian Analysis of the Sr Reaction to Constrain the Sr Cross Section at Astrophysical Energies

Caleb Marshall, Taliah Lansing, David Gribble +3

The Alpha Optical Model Potential (\aomp \!) is a phenomenological approach used to describe elastic scattering where multiple reaction channels are open. It is one of the most cri…

nucl-ex2025

First measurement of 87Rb(α, xn) cross sections at weak r-process energies in supernova ν-driven ejecta to investigate elemental abundances in low-metallicity stars

C. Fougères, M. L. Avila, A. Psaltis +18

Observed abundances of Z ~ 40 elements in metal-poor stars vary from star to star, indicating that the rapid and slow neutron capture processes may not contribute alone to the synt…