Effects of Symmetry Energy on the Equation of State for Hybrid Neutron StarsIn this paper, the implications of the symmetry energy on the hadron and quark phase transitions in the compact star, including the properties of the possible configurations of the quark-hadron…Parada T. P. Hutauruk, Hana Gil, Seung-il Nam et al.·Jul 18, 2023SaveLearn
Postfission properties of uranium isotopes: A hybrid method with Langevin dynamics and the Hauser-Feshbach statistical modelBackground: Precise understanding of nuclear fission is crucial for experimental and theoretical nuclear physics, astrophysics, and industrial applications; however, the complete physical mechanics…Shyoya Tanaka, Nobuya Nishimura, Futoshi Minato et al.·Jul 18, 2023SaveLearn
Proton 0.01 MeV resonance width and low-energy S-factor of p+10B fusionPurpose: In this paper, the proton resonance width of the near-threshold resonance is calculated using two different approaches. The values of the proton width are used to calculate the…A. M. Mukhamedzhanov·Jul 18, 2023SaveLearn
Canonical Ensemble vs. Grand Canonical Ensemble in the Description of Multicomponent Bosonic SystemsThe thermodynamics of a system of interacting bosonic particles and antiparticles in the presence of the Bose-Einstein condensate is studied in the framework of the Skyrme-like mean-field model. It…D. Anchishkin, V. Gnatovskyy, D. Zhuravel et al.·Jul 17, 2023SaveLearn
Energy Loss in Small Collision SystemsWe present leading hadron suppression predictions in Pb+Pb and p+Pb collisions from a convolved radiative and collisional energy loss model in which partons propagate through a realistic…Coleridge Faraday, W. A. Horowitz·Jul 17, 2023SaveLearn
On the problems of creating a nuclear-optical frequency standard based on 229ThThe most probable candidate for the role of a nuclear optical standard is the 8.338-eV isomer of the 229mTh isotope of the thorium nucleus. Ways of using the resonance properties of the electron…F. F. Karpeshin, L. F. Vitushkin·Jul 15, 2023SaveLearn
Exploring the Macroscopic Properties and Nonradial Oscillations of Proto-Neutron Stars: Effects of Temperature, Entropy, and Lepton FractionNeutron stars (NSs) have traditionally been viewed as cold, zero-temperature entities. However, recent progress in computational methods and theoretical modelling has opened up the exploration of…Sayantan Ghosh, Shahebaj Shaikh, Probit J Kalita et al.·Jul 13, 2023SaveLearn
Simultaneous calculation of elastic scattering, fusion, and direct cross sections for reactions of weakly-bound projectilesSimultaneous analyses are performed for cross section data of elastic scattering, fusion, Coulomb breakup, and other direct yields for the 6He+209Bi system at near-Coulomb-barrier energies.…H. M. Maridi, N. Keeley, K. Rusek·Jul 13, 2023SaveLearn
Nature of the N* and resonances via coupled-channel dynamicsThis work aims at determining the composition of certain N* and resonances, i.e. whether they are compact states formed directly by quarks and gluons, or hadronic molecules generated from…Yu-Fei Wang, Ulf-G. Meißner, Deborah Rönchen et al.·Jul 13, 2023SaveLearn
Proton and Neutron Pairing Properties within a mixed volume-surface pairing force using SKI3-HFB TheoryThis work aims at a systematic investigations of the pairing properties and Fermi properties from the proton drip-line to the neutron drip-line. In order to provide more accurate mass formula with…Malik A. Hasan, Ali H. Taqi·Jul 13, 2023SaveLearn
Illuminating early-stage dynamics of heavy-ion collisions through photons at RHIC BES energiesHeavy-ion collisions at sNN 10 GeV probe the QCD phase diagram at large baryon densities. Because the longitudinal Lorentz contraction is small at these collision energies,…Chun Shen, Abel Noble, Jean-François Paquet et al.·Jul 13, 2023SaveLearn
Chiral magnetovortical instabilityWe demonstrate that in a chiral plasma subject to an external magnetic field, the chiral vortical effect can induce a new type of magnetohydrodynamic instability which we refer to as the chiral…Shuai Wang, Xu-Guang Huang·Jul 13, 2023SaveLearn
Fingerprints of the triaxial deformation from energies and B(E2) transition probabilities of γ-bands in transitional and deformed nucleiThe energies and B(E2) transitions involving the states of the ground- and γ-bands in thirty transitional and deformed nuclei are calculated using the triaxial projected shell model (TPSM)…S. P. Rouoof, Nazira Nazir, S. Jehangir et al.·Jul 13, 2023SaveLearn
The study of hadronic rescattering on K*0 resonance yield in baryon-rich QCD matterThe effect of hadronic rescattering on K*0 resonance yield can be studied by measuring K*0/K ratio as a function of centrality or multiplicity. This study investigates how the size of the…Aswini Kumar Sahoo, Subhash Singha, Md. Nasim·Jul 13, 2023SaveLearn
- production as a probe of equation of state of dense matter near the QCD phase transition in relativistic heavy-ion collisionsThe production of doubly strange hyperon - and trebly strange hyperon - in relativistic Au+Au collisions at sNN = 4.2 GeV is explored based on a relativistic transport…Zhi-Min Wu, Gao-Chan Yong·Jul 13, 2023SaveLearn
What is ab initio?Microscopic nuclear theory is based on the tenet that atomic nuclei can be accurately described as collections of point-like nucleons interacting via two- and many-body forces obeying nonrelativistic…R. Machleidt·Jul 12, 2023SaveLearn
Relativistic second-order viscous hydrodynamics from kinetic theory with extended relaxation-time approximationWe use the extended relaxation time approximation for the collision kernel, which incorporates a particle-energy dependent relaxation time, to derive second-order viscous hydrodynamics from the…Dipika Dash, Sunil Jaiswal, Samapan Bhadury et al.·Jul 12, 2023SaveLearn
Short-range expansion for the quantum many-body problemIn this work we derive a systematic short-range expansion of the many-body wave function. At leading order, the wave function is factorized to a zero-energy s-wave correlated pair and spectator…Ronen Weiss, Diego Lonardoni, Stefano Gandolfi·Jul 12, 2023SaveLearn
Empirical radius formulas for canonical neutron stars from bidirectionally selecting EOS features in extended Bayesian analyses of observational dataGiven the significant advancement in Bayesian inference of nuclear Equation of State (EOS) from gravitational wave and X-ray observations of neutron stars (NSs), especially since GW170817, is there a…Jake Richter, Bao-An Li·Jul 11, 2023SaveLearn
Simultaneous study of scattering and fusion hindrance near Coulomb barrier in F+Pb systemsA phenomenological optical potential is used to study the elastic angular distributions for the system 19F+208Pb close to the Coulomb barrier. This potential is constructed by taking into…Kamala Kanta Jena, Bidhubhusan Sahu, Jajati K. Nayak et al.·Jul 11, 2023SaveLearn
Quantum entanglement patterns in the structure of atomic nuclei within the nuclear shell modelQuantum entanglement offers a unique perspective into the underlying structure of strongly-correlated systems such as atomic nuclei. In this paper, we use quantum information tools to analyze the…A. Pérez-Obiol, S. Masot-Llima, A. M. Romero et al.·Jul 11, 2023SaveLearn
Interplay of effects of neutron skins in coordinate space and proton skins in momentum space on hard photons emission in heavy-ion collisions around Fermi EnergyWithin an isospin- and momentum-dependent Boltzmann-Uehling-Uhlenbeck (IBUU) transport model, we investigate the hard photons emission from neutron-proton bremsstrahlung in reaction system of…Wen-Mei Guo, Bao-An Li, Gao-Chan Yong·Jul 11, 2023SaveLearn
Impact of the 6Li asymptotic normalization constant onto α-induced reactions of astrophysical interestIndirect methods have become the predominant approach in experimental nuclear astrophysics for studying several low-energy nuclear reactions occurring in stars, as direct measurements of many of…Chloë Hebborn, Melina L. Avila, Konstantinos Kravvaris et al.·Jul 11, 2023SaveLearn
Neutron star equation of state: identifying hadronic matter characteristicsThe general behavior of the nuclear equation of state (EOS), relevant for the description of neutron stars (NS), is studied within a relativistic mean field description of nuclear matter. Different…Constança Providência, Tuhin Malik, Milena Bastos Albino et al.·Jul 11, 2023SaveLearn
Effects of neutron-rich nuclei masses on symmetry energyWe explore the impact of neutron-rich nuclei masses on the symmetry energy properties using the mass table evaluated by the deformed relativistic Hartree-Bogoliubov theory in continuum (DRHBc) model.…Seonghyun Kim, Dukjae Jang, Soonchul Choi et al.·Jul 11, 2023SaveLearn