From masses and radii of neutron stars to EOS of nuclear matter through neural networkThe equation of state (EOS) of dense nuclear matter is a key factor to determine the internal structure and properties of neutron stars. However, the EOS of high-density nuclear matter has great…Zehan Wu, Dehua Wen·Dec 25, 2023SaveLearn
The imprint of conservation laws on correlated particle productionThe study of event-by-event fluctuations of net-baryon number in a subspace of full phase space is a promising direction for deciphering the structure of strongly interacting matter created in…Peter Braun-Munzinger, Krzysztof Redlich, Anar Rustamov et al.·Dec 24, 2023SaveLearn
New quantification of symmetry energy from neutron skin thicknesses of 48Ca and 208PbPrecise knowledge of the nuclear symmetry energy can be tentatively calibrated through multimessenger constraints. The neutron skin thickness of a heavy nucleus is one of the most sensitive…Rong An, Shuai Sun, Li-Gang Cao et al.·Dec 24, 2023SaveLearn
Time Scales in Many-Body Fast Neutrino Flavor ConversionTime scales associated with many-body fast neutrino flavor conversions in core-collapse supernova are explored in the context of an effective two-flavor model with axial symmetry. We present a…Ramya Bhaskar, Alessandro Roggero, Martin J. Savage·Dec 23, 2023SaveLearn
Interference of resonances in two-proton emission of 16NeWe investigate the two-proton (2p) emission from 16Ne with the time-dependent 14O+p+p three-body calculations. Two 0+ resonances are suggested to participate. For the 0+1…Tomohiro Oishi, Masaaki Kimura·Dec 22, 2023SaveLearn
Toward Initial Conditions of Conserved ChargesAt top collider energies where baryon stopping is negligible, the initial state of heavy ion collisions is overall charge neutral and predominantly composed of gluons. Nevertheless, there can also be…Patrick Carzon·Dec 22, 2023SaveLearn
Can we observe effects of early nonequilibrium dynamics using collective flowThe rapid expansion of the fireball created in a heavy-ion collision causes strong departures from local equilibrium. Such effects are especially important in the very early phase of the collision,…Piotr Bozek·Dec 22, 2023SaveLearn
Entanglement in few-nucleon scattering eventsWe investigate the spin entanglement in few-nucleon scattering processes involving nucleons and deuterons. For this purpose, we consider the entanglement power introduced by Beane et al. We analyze…Tanja Kirchner, Wael Elkamhawy, Hans-Werner Hammer·Dec 22, 2023SaveLearn
Systematic study of the rotational bands in the A 250 mass regionFor the first time, we conducted a comprehensive analysis of the rotational bands in the \( A250 \) mass region. Utilizing a variety of rotational energy models and formulas, we have extracted…Anshul Dadwal, Xiao-Tao He·Dec 22, 2023SaveLearn
Pairing effects on pure rotational energy of nucleiBy applying the angular-momentum projection (AMP) to the self-consistent axial mean-field solutions with the semi-realistic effective Hamiltonian M3Y-P6, the pairing effects on the pure rotational…K. Abe, H. Nakada·Dec 22, 2023SaveLearn
Equation of state at neutron-star densities and beyond from perturbative QCDWe explore the consequences of imposing robust thermodynamic constraints arising from perturbative Quantum Chromodynamics (QCD) when inferring the dense-matter equation-of-state (EOS). We find that…Oleg Komoltsev, Rahul Somasundaram, Tyler Gorda et al.·Dec 21, 2023SaveLearn
Event-by-event Kinetic Description of Pre-Equilibrium Charge Evolution in QCD PlasmaWe use QCD effective kinetic theory to calculate far-from-equilibrium dynamics on an event-by-event basis within the KMPST framework. We present non-equilibrium charge response functions and…Travis Dore, Xiaojian Du, Sören Schlichting·Dec 21, 2023SaveLearn
Towards consistent nuclear interactions from chiral Lagrangians II: Symmetry preserving regularizationLow-energy nuclear structure and reactions can be described in a systematically improvable way using the framework of chiral effective field theory. This requires solving the quantum mechanical…Hermann Krebs, Evgeny Epelbaum·Dec 21, 2023SaveLearn
Effect of the equation of state for dilute neutron matter on the composition of the inner crust of neutron starsThe composition of the inner crust of neutron stars is usually studied using phenomenological interactions such as Skyrme energy-density functionals. But most of these functionals do not agree well…Sunny Kumar Gupta, Michael Urban·Dec 21, 2023SaveLearn
Deuteron production in a combined thermal and coalescence framework for heavy-ion collisions in the few-GeV energy regimeA recently formulated thermal model for hadron production in heavy-ion collisions in the few-GeV energy regime is combined with the idea that some part of protons and neutrons present in the original…Wojciech Florkowski, Radoslaw Ryblewski, Piotr Salabura et al.·Dec 21, 2023SaveLearn
Microscopic study of M1 resonances in Sn isotopesThe magnetic dipole (M1) resonances of even-even 112-120, 124Sn isotopes are investigated in the framework of the self-consistent Skyrme Hartree-Fock (HF) + BCS and Quasiparticle Random Phase…Shuai Sun, Li-Gang Cao, Feng-Shou Zhang et al.·Dec 21, 2023SaveLearn
Probing configuration of α clusters with spectator particles in relativistic heavy-ion collisionsWe propose to use spectator particle yield ratios to probe the configuration of α clusters in 12C and 16O by their collisions at RHIC and LHC energies. The idea is illustrated based…Lu-Meng Liu, Song-Jie Li, Zhen Wang et al.·Dec 21, 2023SaveLearn
Relativistic heat conduction in the large-flux regimeWe propose a general procedure for evaluating, directly from microphysics, the constitutive relations of heat-conducting fluids in regimes of large fluxes of heat. Our choice of hydrodynamic…Lorenzo Gavassino·Dec 21, 2023SaveLearn
Impact of tensor interactions and scalar mixing on covariant energy density functionalsThe recent pioneering campaigns conducted by the Lead Radius Experiment (PREX) and the Calcium Radius Experiment (CREX) collaborations have uncovered major deficiencies in the theoretical description…Marc Salinas, Jorge Piekarewicz·Dec 20, 2023SaveLearn
Complete fusion of 6Li with 28Si and 64Ni nuclei in the framework of the continuum discretized coupled channel methodThe complete fusion of 6Li with 28Si and 64Ni nuclei, ranging from subbarrier energies up to values well above the Coulomb barrier, is studied using the continuum discretized coupled…S. R. Souza, L. F. Canto, R. Donangelo·Dec 20, 2023SaveLearn
The role of longitudinal decorrelations for measurements of anisotropic flow in small collision systemsWithin a (3+1)D viscous hydrodynamic model we compute anisotropic flow in small system collisions as performed at the Relativistic Heavy Ion Collider and measured by the STAR and PHENIX…Sangwook Ryu, Bjoern Schenke, Chun Shen et al.·Dec 19, 2023SaveLearn
One and Two-Body Current Contributions to Lepton-Nucleus ScatteringModeling lepton-nucleus scattering with the accuracy required to extract neutrino-oscillation parameters from long- and short-baseline experiments necessitates retaining most quantum-mechanical…Alessandro Lovato, Noemi Rocco, Noah Steinberg·Dec 19, 2023SaveLearn
Tracing baryon and electric charge transport in isobar collisionsIt is of fundamental interest to understand the carrier of conserved quantum charges within protons and nuclei at high energy. Preliminary data from isobar collisions at RHIC reveal a scaled…Gregoire Pihan, Akihiko Monnai, Björn Schenke et al.·Dec 19, 2023SaveLearn
Nonperturbative study of quantum many-body correlation effects in neutron stars: Equation of stateAlthough neutron stars have been studied for decades, their internal structure remains enigmatic, mainly due to large uncertainties in the equation of state. In neutron stars, the nucleons are…Hao-Fu Zhu, Xufen Wu, Guo-Zhu Liu·Dec 19, 2023SaveLearn
Constraints on Phase Transitions in Neutron Star MatterRecent inference results of the sound velocity in the cores of neutron stars are summarized. Implications for the equation of state and the phase structure of highly compressed baryonic matter are…Len Brandes, Wolfram Weise·Dec 19, 2023SaveLearn