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.

⚛️ nuclear theory

Coulomb and nuclear polarization of the nucleon density in the dinuclear configuration of the 40^{40}Ca + 208^{208}Pb system

This study investigates the Coulomb and nuclear polarization of nucleon density in the 40^{40}Ca + 208^{208}Pb system using a deformed Woods-Saxon mean field, revealing that the repulsive Coulomb tidal field dominates the induced oblate deformation while the attractive nuclear field partially counteracts it at small separations, with polarization energy primarily driven by dipole rather than quadrupole effects.

Bakhodir Kayumov2026-07-31
⚛️ nuclear theory

Impact of Kaon Condensation on the Thermal Evolution of the CCO in HESS J1731--347 Supernova Remnant

This study concludes that while negatively charged kaon condensation can explain the low mass and small radius of the central compact object in HESS J1731--347, it fails to simultaneously account for its observed high surface temperature because the phase transition causes rapid cooling that results in temperatures far below the inferred range.

D. G. Nanopoulos, P. S. Koliogiannis, V. Petousis, M. Veselsky, Ch. C. Moustakidis2026-07-31
⚛️ nuclear theory

Estimating amplitude of matter density fluctuations in solar and supernova models using neutrino flavor evolution

This paper demonstrates that statistical data assimilation can effectively estimate the amplitude of matter density fluctuations in solar and core-collapse supernova models by analyzing neutrino flavor evolution, with the method showing particular reliability in solar scenarios.

Caroline Laber-Smith, Hansen Torres, Lily Newkirk, Dhriti Rathod, A. Baha Balantekin, Amol V. Patwardhan2026-07-31
⚛️ nuclear theory

Binary neutron stars in the next-generation era: Multi-messenger detection prospects and constraints on the equation of state, mass distribution, and cosmology

This paper projects that next-generation gravitational-wave observatories like the Einstein Telescope and Cosmic Explorer will enable hundreds of multi-messenger binary neutron star detections annually, allowing for precise constraints on the neutron star equation of state, mass distribution, and cosmological parameters through joint hierarchical Bayesian inference.

Hauke Koehn, Thibeau Wouters, Gilad Sadeh, Peter T. H. Pang, Mattia Bulla, Chris Van Den Broeck, Michael W. Coughlin, Ti (…)2026-07-31
⚛️ nuclear theory

Pauli Consistent αα--αα Interaction from Inverse Scattering via Phase Function Wavefunctions and RGM Antisymmetrization

This study employs the phase function method to reconstruct α\alpha--α\alpha scattering wavefunctions and, after incorporating Pauli exclusion effects via the resonating group method, validates a double Gaussian interaction model that accurately reproduces the 8Be^{8}\mathrm{Be} resonance energy and scattering parameters while identifying two Pauli-forbidden states.

Anil Khachi, Shikha Awasthi, Tarachand Verma, Ranjana Joshi2026-07-30
⚛️ nuclear theory

Structure of multi-Λ\Lambda hypernuclei with a Skyrme-type ΛΛ\Lambda\Lambda interaction constrained by data on double-Λ\Lambda hypernuclei and neutron stars

This study utilizes a Skyrme-type ΛΛ\Lambda\Lambda interaction constrained by double-Λ\Lambda hypernuclei and neutron star data to demonstrate that multi-Λ\Lambda hypernuclei are particularly effective for isolating the role of repulsive pp-wave interactions near normal density, while density-dependent terms remain more critical for high-density neutron star environments.

Yusuke Tanimura, Chang Ho Hyun, Myung-Ki Cheoun2026-07-30