960 papers
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.
This paper extends spherical coupled-cluster theory to open-shell nuclei with two nucleons removed, validating the method against experimental data for oxygen and calcium isotopes while demonstrating high accuracy for binding energies and excited states but noting an underestimation of electric dipole polarizabilities.
This paper extends the pion-nucleus multiple-scattering framework to include second-order rescattering dynamics and nuclear structure details derived from chiral effective field theory, demonstrating that these corrections are essential for accurately reproducing differential cross sections in -Ca elastic scattering within the -resonance region.
This paper presents ab initio calculations of the electric dipole polarizability for the neutron-rich isotope O using the Lorentz integral transform coupled-cluster approach with chiral two- and three-nucleon interactions, finding good agreement with experimental data in the low-energy region.
This study proposes that self-bound hybrid stars characterized by strong phase transitions and large density discontinuities can simultaneously resolve multiple observational tensions regarding the masses, radii, and tidal deformabilities of various compact objects, including anomalous low-mass pulsars, the massive GW190814 secondary, and standard NICER measurements.
This paper presents an updated version of the TGlauberMC Monte Carlo code (v3.3) with improved nuclear density profiles and nucleon substructure treatments to provide precise predictions for initial-state observables and centrality-dependent multiplicity in upcoming oxygen-oxygen, neon-neon, and proton-oxygen collisions at the LHC.
This paper derives model-independent expansions to quantify leading corrections to the smoothness and on-shell approximations in femtoscopy and coalescence, demonstrating that while these corrections are generally small (at or below the percent level) for LHC energy collisions, they can be efficiently evaluated with the same numerical complexity as standard methods.
This paper utilizes the Schwinger--Keldysh formalism to demonstrate that standard rate equations for nonequilibrium cascade dynamics are controlled Markovian approximations of a more fundamental multi-component system, where retaining the finite lifetimes of intermediate reservoirs reveals non-Markovian memory effects that govern delayed, history-dependent formation processes.
To celebrate the 50th anniversary of the J/ψ discovery, this paper reviews the progress of QCD-inspired quark potential models derived from charmonium spectra and emphasizes the critical role of unquenching dynamics, multiquark components, and exotic states in advancing our understanding of hadron structure and spectroscopy.
This paper proposes that neutron dark decay, potentially suppressed at high densities, provides a unified mechanism to explain both the existence of subsolar-mass compact objects like HESS J1731-347 and the two-solar-mass neutron star limit without relying on external merger processes.
This paper presents a comprehensive theoretical analysis of the two-neutrino double electron capture in Xe by improving nuclear and atomic structure calculations, which yields refined nuclear matrix elements, predicts specific capture fractions for various decay channels (notably 74% for the KK channel and 24% for the cumulative KL-KO channels), and provides updated atomic relaxation energies for background modeling in liquid Xenon experiments.