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.

Revisiting QCD-induced little inflation with chiral density wave state and its implications on pulsar timing array gravitational-wave signals

This paper investigates whether a chiral density wave phase at large baryon chemical potential can enable QCD-induced little inflation to produce observable nano-Hz gravitational waves, but concludes that the resulting latent heat is insufficient to support a viable cosmological scenario.

Tae Hyun Jung, Seyong Kim, Jong-Wan Lee, Chang Sub Shin, Hee Beom Yang2026-04-01⚛️ nucl-th

Magnetodynamic Characteristics and QGP Energy Dissipation in RMHD Framework with Relativistic Heavy-Ion Collisions

This study utilizes a (1+1)D relativistic magnetohydrodynamic framework with Bjorken flow to demonstrate how time-dependent ultra-strong magnetic fields and temperature-dependent magnetic susceptibility differentially influence Quark-Gluon Plasma energy density evolution, revealing that magnetic pressure suppresses decay in ultra-relativistic fluids while enhanced coupling accelerates dissipation in conformal fluids.

Huang-Jing Zheng, Sheng-Qin Feng2026-03-31⚛️ nucl-th

Truncation uncertainties for accurate quantum simulations of lattice gauge theories

This paper presents a new formalism for estimating truncation errors in the electric basis of lattice gauge theory simulations on quantum computers, leveraging Hilbert space fragmentation to demonstrate that errors decay factorially with field truncation, thereby improving previous error estimates by a factor of up to 1030610^{306} for models like the Schwinger model and pure U(1) gauge theory.

Anthony N. Ciavarella, Siddharth Hariprakash, Jad C. Halimeh, Christian W. Bauer2026-03-31⚛️ hep-lat

Sign Reversal of Boer-Mulders Functions from Semi-inclusive Deep-Inelastic Scattering to the Drell-Yan Process

This paper reviews the theoretical and experimental status of the predicted sign reversal of Boer-Mulders functions between semi-inclusive deep-inelastic scattering and Drell-Yan processes, demonstrating that current data supports this reversal for proton valence quarks while highlighting future prospects for testing it in pions at the Electron-Ion Collider.

Jen-Chieh Peng, Ming-Xiong Liu, Guanghua Xu2026-03-31⚛️ nucl-ex

Low-energy 3^{3}He(α,γα,γ)7^{7}Be reaction within the Skyrme potential framework

This paper employs a microscopic Skyrme Hartree-Fock-based folding potential model to simultaneously describe low-energy elastic scattering and calculate the astrophysical SS factor for the 3^{3}He(α,γ\alpha,\gamma)7^{7}Be reaction, yielding a recommended zero-energy value of S34(0)=0.610±0.024S_{34}(0) = 0.610 \pm 0.024 keV b that agrees well with experimental data.

Nguyen Le Anh, Nguyen Gia Huy, Dao Nhut Anh, Do Huy Tho, Hoang Thai An2026-03-31⚛️ nucl-th

Why Stellar Sequences Turn Over: Fixed Points, Instability, and Equation-of-State Universality

This paper reformulates stellar structure equations as a dynamical system to demonstrate that the maximum mass of stellar sequences corresponds to a fixed point in the relativistic regime, a framework that explains equation-of-state-insensitive relations and suggests that the pulsar J0740+6620 likely lies near this maximum only if a strong first-order phase transition occurs just above its central density.

Isaac Legred, Nicolas Yunes2026-03-31🔭 astro-ph