AC nuclear Stark effect in H-atom via super-intense laser-atom interactionWe investigate the nuclear Stark effect induced in hydrogen-like atomic nuclei under super-intense laser fields. Since laser wavelengths are generally larger than nuclear dimensions, direct…Ali Raza Mirza, Rizwan Abbas, Atif Shahbaz·Feb 18, 2025SaveLearn
Analytic continuation in coupling constant applied to two-proton emittersFor quantum meta-stable problems with three particles, the 6Be and 16Ne nuclei as two-proton (2p) emitters provide a testing field. Considering the complexity of many-body meta-stable…Tomohiro Oishi, Masaaki Kimura·Feb 18, 2025SaveLearn
Quantum Dynamical Microscopic Approach to Stellar Carbon BurningThe process of carbon burning is vital to understanding late stage stellar evolution of massive stars and the conditions of certain supernovae. Carbon burning is a complex problem, involving quantum…Grant Close, Paul Stevenson, Alexis Diaz-Torres·Feb 16, 2025SaveLearn
Stochastic baryon charge transport in relativistic hydrodynamicsWe utilize 3+1D stochastic hydrodynamics to study correlations and fluctuations of baryon charge in high-energy heavy-ion collisions. The baryon charge fluctuations are important observables to probe…Nicolas Borghini, Baochi Fu, Sören Schlichting·Feb 16, 2025SaveLearn
Conformality Thresholds in Neutron StarsThe dense-matter equation of state (EOS) under neutron-star conditions is investigated. We focus on the qualitative behavior of the speed of sound and its average. We characterize and compare the…Michał Marczenko·Feb 15, 2025SaveLearn
Chiral Symmetry in Dense Matter with Meson CondensationKaon condensation in hyperon-mixed matter [(Y+K) phase], which may be realized in neutron stars, is discussed on the basis of chiral symmetry. With the use of the effective chiral Lagrangian for…Takumi Muto, Toshiki Maruyama, Toshitaka Tatsumi·Feb 15, 2025SaveLearn
Modeling of acceleration in heavy-ion collisions: occurrence of temperature below the Unruh temperatureIt has recently been shown that extremely strong electric fields can be created in central collisions of heavy ions, due to which the Schwinger effect can be significant. A direct analogue of the…G. Yu. Prokhorov, D. A. Shohonov, O. V. Teryaev et al.·Feb 14, 2025SaveLearn
Chiral symmetry and peripheral neutron-α scatteringWe propose and demonstrate that peripheral neutron-α scattering at low energies can serve as a sensitive and clean probe of the long-range three-nucleon forces. To this aim, we perform ab…Yilong Yang, Evgeny Epelbaum, Jie Meng et al.·Feb 14, 2025SaveLearn
Improvement to Generalized Separable Expansion Method in Lippmann-Schwinger EquationRealistic nucleon-nucleon (NN) potentials are generally not in separable form, but there is a way to convert them into separable potentials, called the generalized separable expansion (GSE). When the…Hiroyuki Kamada·Feb 14, 2025SaveLearn
Source function from two-particle correlation function through entropy-regularized Richardson-Lucy deblurringSource functions are obtained from p-p and d--α correlation functions by applying the Richardson-Lucy (RL) deblurring to the Koonin-Pratt (KP) equation. To prevent fitting of noise in…C. K. Tam, Z. Chajęcki, P. Danielewicz et al.·Feb 13, 2025SaveLearn
Low-energy spectra of nobelium isotopes: Skyrme random-phase-approximation analysisLow-energy spectra in the isotopic chain 250-262No are systematically investigated within the fully self-consistent Quasiparticle Random-Phase-Approximation (QRPA) using Skyrme forces SLy4,…V. O. Nesterenko, M. A. Mardyban, A. Repko et al.·Feb 13, 2025SaveLearn
Quarkonium Spectroscopy in the Quark-Gluon PlasmaThe properties of bound states are fundamental to hadronic spectroscopy and play a central role in the transition from hadronic matter to a quark-gluon plasma (QGP). In a strongly coupled QGP (sQGP),…Zhanduo Tang, Biaogang Wu, Andrew Hanlon et al.·Feb 13, 2025SaveLearn
Bose-Einstein condensation of five α clusters in 20Ne and supersolidityWe show that the five α cluster states recently observed in 20Ne, slightly above the five α threshold energy, are Bose-Einstein condensates of five α clusters. The states…S. Ohkubo, J. Takahashi, Y. Yamanaka·Feb 13, 2025SaveLearn
Causality constraints on radiative transferThe standard formula, due to Spiegel, for the smoothing of temperature fluctuations by radiative transfer is unstable in relativity. This is due to the fact that Spiegel neglected the transit time of…Lorenzo Gavassino·Feb 12, 2025SaveLearn
A variation on "compositeness" (including higher partial waves)The ``spatial interpretation of compositeness'', presented and discussed in [1,2] in the context of non-relativistic potential scattering, is extended to higher partial waves. A particular set of…Peter C. Bruns·Feb 12, 2025SaveLearn
φ meson in nuclear matter and atomic nucleiThe properties (masses and decay widths) of the φ meson are investigated in nuclear matter from the φ meson self-energy, using the tree-level φ KK Lagrangian, and, incorporating…Arpita Mondal, Amruta Mishra·Feb 12, 2025SaveLearn
Complete set of observables in pseudo-scalar meson photoproduction -- Controversy solvedThe long-standing debate over whether the complete set of observables in pseudo-scalar meson photoproduction consists of eight or merely four elements continues to persist. From the perspective of…A. Švarc·Feb 12, 2025SaveLearn
Fixing effective range parameters in elastic α-12C scattering: an impact on resonant 24+ state of 16O and SE2 factor of 12C(α,γ)16OElastic α-12C scattering for l=2 and E2 transition of radiative α capture on 12C, 12C(α,γ)16O, are studied in cluster effective field theory. Due…Shing-Ichi Ando·Feb 12, 2025SaveLearn
Directly probing existence of α-cluster structure in 20Ne by relativistic heavy-ion collisionsCan relativistic heavy-ion collisions only probe the global shape of colliding nuclei, or their detailed internal structure as well? Taking 20Ne as an example, we attempt to directly probe its…Lu-Meng Liu, Hai-Cheng Wang, Song-Jie Li et al.·Feb 12, 2025SaveLearn
Benchmarking nuclear matrix elements of 0ββ decay with high-energy nuclear collisionsReducing uncertainties in the nuclear matrix elements (NMEs) remains a critical challenge in designing and interpreting experiments aimed at discovering neutrinoless double beta (0ββ)…Yi Li, Xin Zhang, Giuliano Giacalone et al.·Feb 12, 2025SaveLearn
Inelastic neutrino-nucleus scattering off 203/205Tl in terms of the nuclear recoil energy using a hybrid nuclear modelNuclear structure calculations in the context of a novel hybrid nuclear model, combining the nuclear shell model and the microscopic quasiparticle-phonon model are presented. The predictivity of the…Matti Hellgren, Dimitrios K. Papoulias, Jouni Suhonen·Feb 11, 2025SaveLearn
Building Neutron Stars with the MUSES Calculation EngineExploring the equation of state of dense matter is an essential part of interpreting the observable properties of neutron stars. We present here the first results for dense matter in the…Mateus Reinke Pelicer, Nikolas Cruz-Camacho, Carlos Conde et al.·Feb 11, 2025SaveLearn
Moments of inertia of rare-earth nuclei and the nuclear time-odd mean fields within exact solutions of the adiabatic theoryWe systematically analyse the nuclear moments of inertia determined within the Skyrme and Gogny density functional theories. The time-odd mean fields generated by collective rotation are…Xuwei Sun, Jacek Dobaczewski, Markus Kortelainen et al.·Feb 11, 2025SaveLearn
α+α+3He cluster structure in 11CWe study the α + α + 3He cluster structure of 11C within the microscopic cluster model. The calculations essentially reproduce the energy spectra for both negative and…Ying-Yu Cao, De-Ye Tao, Bo Zhou et al.·Feb 11, 2025SaveLearn
Electric dipole excitations near the neutron separation energies in 96MoElectric dipole strength near the neutron separation energy significantly impacts nuclear structure properties and astrophysical scenarios. These excitations are complex in nature and may involve the…Eun Jin In, Emanuel Chimanski, Jutta Escher et al.·Feb 10, 2025SaveLearn