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.

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

Particle spectra in the integrated hydrokinetic model at RHIC Beam-Energy-Scan energies

This study utilizes an extended Integrated HydroKinetic Model to analyze light-hadron production in Au+Au collisions at RHIC Beam-Energy-Scan energies, demonstrating that both crossover and first-order phase transition equations of state can similarly describe soft particle spectra when parameters are adjusted, with the most significant distinctions appearing in proton and kaon yields at the lowest energy of 7.7 GeV.

Narendra Rathod, Yuri Sinyukov, Musfer Adzhymambetov, Hanna Zbroszczyk2026-03-09⚛️ hep-ph

Rotating neutron stars within the macroscopic effective-surface approximation

This paper extends the macroscopic effective-surface model of neutron stars to rotating systems by deriving analytical expressions for angular momentum and adiabatic moments of inertia within General Relativity, revealing that strong gravity and surface correlations significantly constrain the accessible neutron star radii.

A. G. Magner, S. P. Maydanyuk, A. Bonasera, H. Zheng, S. N. Fedotkin, A. I. Levon, T. Depastas, U. V. Grygoriev, A. A. Uleiev2026-03-09🔭 astro-ph