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.

From closed shells to open shells: Coupled-cluster calculations of atomic nuclei

This study provides a comprehensive comparison of coupled-cluster formulations based on symmetry-broken reference states and equation-of-motion techniques, demonstrating that both approaches yield consistent descriptions of bulk nuclear properties across calcium and nickel isotopic chains when using chiral effective field theory interactions.

F. Marino, F. Bonaiti, P. Demol, S. Bacca, T. Duguet, G. Hagen, G. R. Jansen, T. Papenbrock, A. Tichai2026-03-02⚛️ nucl-ex

Particle number projected energies at finite temperature

This study incorporates particle number projection into finite-temperature Skyrme density functional calculations to rigorously determine deformation-dependent energies, revealing that while even-odd staggering diminishes near the critical temperature and fission barriers remain similar to unprojected results, the method provides valuable insights into nuclear level densities at both ground states and barriers.

Jiawei Chen, Yu Qiang, Junchen Pei2026-03-02⚛️ nucl-th

Realistic Equations of State Informing Neutron Star Post-Merger Gravitational-Wave Frequencies

By employing realistic relativistic mean field equations of state with consistent thermal treatments, this study demonstrates that post-merger gravitational-wave peak frequencies span 2.5 to 4 kHz, thereby highlighting the necessity for broadband observatories with kilohertz sensitivity and validating the KAGRA high-frequency design over its broadband counterpart.

Spencer J. Magnall, Nilaksha Barman, Debarati Chatterjee, Paul D. Lasky, Simon Goode2026-03-02⚛️ nucl-th

High-Precision Mass Measurements of Proton-Rich Rh, Pd, Cd isotopes in the vicinity of 100Sn and Impact on X-Ray Burst and Supernova Nucleosynthesis

Using high-precision mass measurements of proton-rich Rh, Pd, and Cd isotopes near the doubly magic 100^{100}Sn nucleus, this study significantly refines nuclear mass models and demonstrates that these new data reduce abundance uncertainties in X-ray burst simulations while shifting reaction flows toward A=90A=90 production and suppressing heavier nucleosynthesis.

D. S. Hou, W. D. Xian, M. Rosenbusch, M. Wada, P. Schury, A. Takamine, Y. Luo, J. Lee, H. Ishiyama, S. Nishimura, C. Y. Fu, A. Dohi, H. Feng, Z. He, S. Kimura, T. Niwase, V. H. Phong, T. T. Yeung, Q. (…)2026-03-02⚛️ nucl-ex

SS factor of 13^{13}C(αα,nn)16^{16}O at low energies in cluster effective field theory

This paper employs cluster effective field theory, fitted to recent experimental data from the LUNA and JUNA collaborations, to calculate the SS factor of the 13^{13}C(α\alpha,nn)16^{16}O reaction at low energies and extrapolate it to the Gamow peak relevant for low-mass AGB stars, identifying the near-breakup threshold 1/2+1/2^+ state of 17^{17}O as the primary source of uncertainty.

Shung-Ichi Ando2026-03-02⚛️ nucl-ex

Comparing effective temperatures in standard and Tsallis distributions from transverse momentum spectra in small collision systems

This study investigates transverse momentum spectra of light charged hadrons in RHIC d+Au and p+p collisions at sNN=200\sqrt{s_{NN}}=200 GeV, revealing that effective temperatures derived from standard and Tsallis distributions exhibit systematic decreases across distribution types and collision centralities, while maintaining perfect linear relationships between them.

Peng-Cheng Zhang, Pei-Pin Yang, Ting-Ting Duan, Hailong Zhu, Fu-Hu Liu, Khusniddin K. Olimov2026-02-27⚛️ nucl-ex