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From the 1 of 13 linked papers with an AI index.

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13 papers

nucl-th2026

Nuclear -Ray Cascades as Markov Processes

A. Psaltis

A framework for computing -ray feeding probabilities in nuclear decay schemes based on absorbing Markov chains is presented. In this approach, excited nuclear states are treate…

astro-ph.GA2026

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters

Natalia Alvarez-Baena, Valentina D'Orazi, Christopher Sneden +11

The paper measures molybdenum, ruthenium, and zirconium abundances in 81 stars from 30 open clusters using high‑resolution HARPS‑N spectra to investigate the Galactic chemical evol…

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…

astro-ph.SR2026

The 2025 Evaluation of Experimental Thermonuclear Reaction Rates (ETR25)

Christian Iliadis, Richard Longland, Kiana Setoodehnia +3

This work describes the formalism for estimating thermonuclear reaction rates for astrophysical applications, emphasizing modern statistical approaches such as Monte-Carlo sampling…

astro-ph.HE2025

Direct measurement of Cu(,)Ni precludes a strong NiCu cycle in Type-I X-ray bursts

N. Bhathi, J. S. Randhawa, R. Kanungo +36

Model-observation comparisons of type-I X-ray bursts (XRBs) can reveal the properties of accreting neutron star systems, including the neutron star compactness. XRBs are powered by…