Nuclear theory sits at the fascinating intersection of particle physics and the forces that hold our universe together. This field explores how protons and neutrons bind inside atomic nuclei, seeking to understand the fundamental interactions that govern matter at its most dense and energetic levels. While the mathematics involved can be incredibly complex, the core questions are deeply human: how does the universe function at its smallest scales, and what happens when we push matter to its limits?

At Gist.Science, we make these cutting-edge discoveries accessible by processing every new preprint published in this category on arXiv. Our team transforms dense academic manuscripts into clear, plain-language summaries alongside detailed technical overviews, ensuring that both experts and curious readers can grasp the latest breakthroughs without getting lost in the jargon. Below are the latest papers in nuclear theory, distilled and ready for you to explore.

Physics-Informed Global Extraction of the Universal Small-xx Dipole Amplitude

This paper presents a physics-informed neural network approach to extract a universal small-xx dipole scattering amplitude directly from global DIS and photoproduction data without rigid parametric assumptions, successfully resolving the long-standing tension between total and charm cross-section channels while providing a smooth, non-negative input for Color Glass Condensate phenomenology.

Si-Wei Dai, Fu-Peng Li, Long-Gang Pang, Guang-You Qin, Shu-Yi Wei, Han-Zhong Zhang, Wenbin Zhao2026-03-10⚛️ hep-ph

s-process nucleosynthesis in low-mass AGB stars by the 13^{13}C(α\alpha,n)16^{16}O neutron source

This review traces the evolution of understanding s-process nucleosynthesis in low-mass AGB stars from early nuclear systematics to modern stellar modeling, highlighting how observational constraints necessitated a shift from the high-temperature 22^{22}Ne(α\alpha,n)25^{25}Mg neutron source to the low-temperature 13^{13}C(α\alpha,n)16^{16}O reaction as the primary mechanism for synthesizing elements between Sr and Pb.

Inma Domínguez, Carlos Abia, Maurizio Busso, Oscar Straniero, Sara Palmerini2026-03-10🔭 astro-ph

Microscopic quasifission dynamics of the 54Cr+243Am{}^{54}\text{Cr}+{}^{243}\text{Am} reaction

Using fully microscopic time-dependent Hartree-Fock simulations, this study reveals that the quasifission dynamics in the 54Cr+243Am^{54}\text{Cr}+^{243}\text{Am} reaction are governed by a complex interplay between collision geometry and incident energy, where specific energy windows can suppress shell effects to potentially enhance the fusion probability for synthesizing superheavy element 119.

Liang Li, Lu Guo2026-03-10⚛️ nucl-th

A Lattice QCD study of pΛp-\Lambda scattering in continuum and chiral limits

This paper presents the first systematic lattice QCD study of I=1/2I=1/2 proton-Λ\Lambda scattering across multiple pion masses and lattice spacings, yielding scattering parameters and cross sections that agree with experimental data and confirm attractive interactions critical for nuclear theory and neutron star modeling.

Hang Liu, Liuming Liu, Jin-Xin Tan, Wei Wang, Haobo Yan, Qian-Teng Zhu2026-03-09⚛️ hep-ph

Inverse-mapped density-dependent relativistic mean-field inference of the neutron-star equation of state with multi-messenger constraints

This study employs Bayesian inference within a density-dependent relativistic mean-field framework, constrained by multi-messenger data ranging from chiral effective field theory to massive pulsar observations, to reconstruct a thermodynamically consistent neutron-star equation of state that predicts a compact canonical radius of approximately 11.6 km and reveals strongly interacting matter cores with sound speeds exceeding the conformal limit.

Wen-Jie Xie, Cheng-Jun Xia2026-03-09🔭 astro-ph