Imprint of α-Clustering on Ab Initio Correlations in Relativistic Light Ion CollisionsThis study investigates the influence of α-cluster structures in relativistic light nuclear collisions. Using a cluster framework, I extract the characteristics of the nucleonic configurations…Hadi Mehrabpour·Jun 15, 2025SaveLearn
Impact of particle production mechanisms on pseudorapidity distribution and directed flow in Au+Au and Cu+Cu collisions at sNN = 19.6 GeV using AMPT modelThe STAR experiment at the top RHIC energy has observed that the directed flow (v1) of inclusive light hadrons is independent of the collision system size at a given…Muhammad Farhan Taseer, Subhash Singha·Jun 13, 2025SaveLearn
Microscopic theory of angular momentum distributions across the full range of fission fragmentsModern nuclear theory provides qualitative insights into the fundamental mechanisms of nuclear fission and is increasingly capable of making reliable quantitative predictions. Most quantities of…Petar Marević, Nicolas Schunck, Marc Verriere·Jun 12, 2025SaveLearn
HFB3: an axial HFB solver with Gogny forces using a 2-center HO basis (C++/Python)The HFB3 program solves the axial nuclear Hartree-Fock-Bogoliubov (HFB) equations using bases formed by either one or two sets of deformed Harmonic Oscillator (HO) solutions with D1-type and D2-type…N. Dubray, J. P. Ebran, P. Carpentier et al.·Jun 12, 2025SaveLearn
Geometry of Configuration Mixing in Bose-Fermi SystemsA geometric interpretation for an algebraic interacting boson-fermion model with configuration mixing is presented. The formalism is based on an extended Bose-Fermi matrix coherent states and is…A. Leviatan, N. Gavrielov·Jun 12, 2025SaveLearn
Gapless superfluidity in neutron stars: Normal-fluid fractionOur previous investigation within the time-dependent nuclear energy-density functional theory showed that the nuclear superfluids contained inside cold neutron stars could become gapless under…Valentin Allard, Nicolas Chamel·Jun 12, 2025SaveLearn
Schwinger-Keldysh approach to tunneling transport at a hadron-quark interfaceWe theoretically discuss quantum tunneling transport and frictions at a hadron-quark matter interface based on the Schwinger-Keldysh approach combined with the tunneling Hamiltonian, which has been…Tingyu Zhang, Hiroyuki Tajima, Motoi Tachibana·Jun 11, 2025SaveLearn
Charged-current quasielastic neutrino scattering off nuclei with nucleon-nucleon short-range correlationsIn recent years, many studies on neutrino-nucleus scattering have been carried out to investigate nuclear structures and the interactions between neutrinos and nucleons. This paper develops a…Jian Liu, Qiang Su, Qinglin Niu et al.·Jun 11, 2025SaveLearn
Heavy-heavy and heavy-light mesons in cold nuclear matterWe review the in-medium modifications of effective masses (Lorentz scalar potentials or phenomenon of mass shift) of heavy-heavy and heavy-light mesons in symmetric nuclear matter and their nuclear…J. J. Cobos-Martínez, Guilherme N. Zeminiani, Kazuo Tsushima·Jun 10, 2025SaveLearn
Symmetry energy and neutron matter equation of state at 0/3 from the electric dipole polarizability in 48Ca, 68Ni and 208PbBased on the quasiparticle random phase approximation implemented via the finite amplitude method, we employ a set of representative relativistic mean-field models to investigate the sensitivity of…Mengying Qiu, Lie-Wen Chen, Zheng Zheng Li et al.·Jun 10, 2025SaveLearn
Microscopic analysis of the giant monopole resonance excitation energyA systematic study of the isoscalar giant monopole resonance (ISGMR) in a wide range of nuclei from various isotopic chains is performed within the microscopic self-consistent Skyrme HF+BCS method…M. K. Gaidarov, M. V. Ivanov, Y. I. Katsarov et al.·Jun 10, 2025SaveLearn
Bulk Viscosity of Two-Flavor Color Superconducting Quark Matter in Neutron Star MergersThis work investigates the bulk viscosity of warm, dense, neutrino-transparent, color-superconducting quark matter, where damping of density oscillations in the kHz frequency range arises from…Mark Alford, Arus Harutyunyan, Armen Sedrakian et al.·Jun 9, 2025SaveLearn
Dependence of angular momentum of fission fragments on total kinetic energy in spontaneous fission of 252CfA weak dependence of the angular momentum of 144Ba fragments, produced in the spontaneous fission of 252Cf, on the total kinetic energy (TKE) was recently observed Giha2025. To…A. Rahmatinejad, T. M. Shneidman, G. G. Adamian et al.·Jun 9, 2025SaveLearn
Nuclear transparency and shadowing of the two-step process in the A(e,e'π+) reactionWe investigate nuclear transparency induced by pion electroproduction on nuclei, A(e,e'π+), with our interest in the role of the two-step process in the Glauber multiple scattering theory.…Tae Keun Choi, Kook-Jin Kong, Byung-Geel Yu·Jun 9, 2025SaveLearn
What is the Quark-Gluon Plasma made of?This article surveys our present understanding of the internal structure of the fully developed quark-gluon plasma at temperatures outside the crossover region. The theoretical part of the review…Berndt Müller·Jun 8, 2025SaveLearn
Estimation of Electron Screening Potential in the 6Li(d,α)4He Reaction Using Multi-Layer Perceptron Neural NetworkReactions between light charged nuclei at sub-Coulomb energies are crucial in astrophysical environments, but accurate cross-section measurements are hindered by electron screening. Traditional…D. Chattopadhyay·Jun 7, 2025SaveLearn
Effects of vibration and rigidity modes of motion on the spectral statistics of spherical nucleiIn this paper, we investigated the effects of eta-vibration and eta-rigidity on the energy levels from the viewpoint of statistical fluctuations of nuclear systems. To this aim, a…H. Sabri, A. Hosseinnezhad·Jun 7, 2025SaveLearn
Charge symmetry breaking effects of ω-0 mixing in relativistic mean-field modelWe present a relativistic mean-field model that incorporates charge symmetry breaking (CSB) of nuclear force via ω - 0 meson mixing, along with corrections to the electromagnetic…Yusuke Tanimura, Tomoya Naito, Hiroyuki Sagawa et al.·Jun 7, 2025SaveLearn
Representing Equations of State With Strong First-Order Phase TransitionsParametric representations of the high-density nuclear equation of state are used in constructing models for interpreting the astrophysical observations of neutron stars. This study explores how…Lee Lindblom, Steve M. Lewis, Fridolin Weber·Jun 6, 2025SaveLearn
Femtoscopic signatures of unique nuclear structures in relativistic collisionsOne of the most vital topics of today's high-energy nuclear physics is the investigation of the nuclear structure of the collided nuclei. Recent studies at the Relativistic Heavy Ion Collider (RHIC)…Daniel Kincses·Jun 6, 2025SaveLearn
Bayesian inference of neutron star crust properties using an ab initio-benchmarked meta-modelAccurate modeling of the neutron star crust is essential for interpreting multimessenger observations and constraining the nuclear equation of state (EoS). However, standard phenomenological EoS…S. Burrello, F. Gulminelli, M. Antonelli et al.·Jun 5, 2025SaveLearn
Bayesian Inference of the Landau Parameter G'0 from Joint Gamow-Teller MeasurementsThe Landau-Migdal parameter G'0 characterizes the main part of the spin-isospin dependent nucleon-nucleon interaction. Consequently, the G'0 is closely related to the Gamow-Teller resonance…Zidu Lin, Gianluca Colò, A. W. Steiner et al.·Jun 5, 2025SaveLearn
Simulated-Annealing Optimization of Mean-Field Parameters in a Correlated-Basis Nuclear Model with Realistic Short-Range CorrelationsWe optimize a six-parameter spherical Woods-Saxon mean field within a first-order correlated-basis-function description of finite nuclei containing central, spin-isospin, and tensor Short-Range…Tianyang Ma, Shalom Shlomo·Jun 5, 2025SaveLearn
The 9Be photodisintegration cross section within Cluster Effective Field TheoryA low-energy calculation of 9Be photodisintegration cross section is presented within an αα n cluster approach. The α n and αα contact interactions are derived…Ylenia Capitani, Elena Filandri, Chen Ji et al.·Jun 5, 2025SaveLearn
The quark-gluon plasma: diagnosis with thermal hadron production from the early history until detailed characterization at high energy collidersIn nuclear collisions at relativistic energies, matter is created which resembles closely the matter that filled all space until about 15 microseconds after the big bang. Here we summarize selected…Peter Braun-Munzinger, Krzysztof Redlich, Johanna Stachel·Jun 5, 2025SaveLearn