6020576
New multisite observations of Delta Scuti stars V624 Tauri and HD 23194
1 Observatorio Astronómico Nacional, Instituto de Astronoḿıa, Universidad Nacional Autónoma de México, A.P. 877 Ensenada, BC 22860, Mexico 2 Observatoire de Paris, LESIA, UMR 8109, F-92195, Meudon, France 3 Beijing Observatory, Chinese Academy of Sciences, Beijing, P.R. China 4 Instituto de Astrof́ısica de Canarias, E-38205 La Laguna, Tenerife, Spain 5 Instituto de Astronoḿıa, Universidad Nacional Autónoma de México, Ap. P. 70-264, Mexico, D.F. 04510, Mexico
101147336
Impedance Computation of Main Components in CSNS/RCS
33315431
Spin structure of nucleons in a quark model with constituent gluons.
16718501
The Kaon-Photoproduction Of Nucleons In The Chiral Quark Model
In this paper, we develop a general framework to study the mesonphotoproductions of nucleons in the chiral quark model. The S and U channel resonance contributions are expressed in terms of the ChewGoldberger-Low-Nambu (CGLN) amplitudes. The kaon-photoproduction processes, γp → K+Λ, γp → K+Σ0, and γp → K0Σ+, are calculated. The initial results show that the quark model provides a much improved description of the reaction mechanism for the kaon-photoproductions of the nucleon with less parameters than the traditional phenomenological approaches. PACS numbers: 13.75.Gx, 13.40.Hq, 13.60.Le,12.40.Aa
120492049
Octupole degree of freedom for nuclei near 152Sm in a reflection-asymmetric relativistic mean-field approach
The potential energy surfaces of even-even isotopes near 152Sm are investigated within the constrained reflection-asymmetric relativistic mean-field approach using parameter sets PK1 and NL3. It is shown that the critical-point candidate nucleus 152Sm marks the shape/phase transition not only from U(5) to SU(3) symmetry, but also from the octupole deformed ground state in 150Sm to the quadrupole deformed ground state in 154Sm. The important role of the octupole deformation driving pair (?2f7/2, ?1i13/2) is demonstrated based on the components of the single-particle levels near the Fermi surface. In addition, the patterns of both the proton and the neutron octupole deformation driving pairs (?2f7/2, ?1i13/2) and (?2d5/2, ?1h11/2) are investigated.
119334067
Longitudinal transitions of baryon resonances in the constituent quark model
A longitudinal transition operator that satisfies the gauge invariance requirement is introduced in the constituent quark model. The corresponding longitudinal transitions from the ground state of the nucleon to resonances of the baryon are calculated. The study shows that the longitudinal coupling plays an important role in the understanding of the structure of the baryon.
99545358
The influence of cluster emission and the symmetry energy on neutron - proton spectral double ratios
Abstract The emissions of neutrons, protons and bound clusters from central 124 Sn +  124 Sn and 112 Sn +  112 Sn collisions are simulated using the Improved Quantum Molecular Dynamics model for two different density-dependent symmetry-energy functions. The calculated neutron–proton spectral double ratios for these two systems are sensitive to the density dependence of the symmetry energy, consistent with previous work. Cluster emission increases the double ratios in the low energy region relative to values calculated in a coalescence-invariant approach. To circumvent uncertainties in cluster production and secondary decays, it is important to have more accurate measurements of the neutron–proton ratios at higher energies in the center of mass system, where the influence of such effects is reduced.
123197092
Mass parameters for relative and neck collective motions in heavy ion fusion reactions
Mass parameters for the relative and neck motions in fusion reactions of symmetric systems $^{90}\mathrm{Zr}+^{90}\mathrm{Zr}$, $^{110}\mathrm{Pd}+^{110}\mathrm{Pd}$, and $^{138}\mathrm{Ba}+^{138}\mathrm{Ba}$ are studied by means of a microscopic transport model. The shape of the nuclear system is determined by an equidensity surface obtained from the density distribution of the system. The relative and neck motions are then studied and the mass parameters for these two motions are deduced. The mass parameter for the relative motion is around the reduced mass when the reaction partners are at the separated configuration and increases with a decrease of the distance between two reaction partners after the touching configuration. The mass parameter for the neck motion first decreases slightly up to the touching configuration and then increases with the neck width, and its magnitude is from less than a tenth to several times more than the total mass of the system. The mass parameters obtained from the microscopic transport model are larger than the ones obtained from the hydrodynamic model and smaller than those obtained from the linear response function theory. The mass parameters for both motions depend on the reaction systems, but the one for the relative motion depends on the incompressibility of the EoS more obviously than that for neck motion.
119107991
Transport model study of nuclear stopping in heavy-ion collisions over the energy range from 0.09A to 160A GeV
Nuclear stopping in heavy-ion collisions over a beam energy range from SIS and AGS up to SPS is studied in the framework of the modified Ultrarelativistic Quantum Molecular Dynamics transport model, in which mean field potentials of both formed and "preformed" hadrons (from string fragmentation) and medium-modified nucleon-nucleon elastic cross sections are considered. It is found that nuclear stopping is influenced by both the stiffness of the equation of state and medium modifications of nucleon-nucleon cross sections at SIS energies. At high SPS energies, a two-bump structure is shown in the experimental rapidity distribution of free protons, which can be understood by considering the preformed hadron potentials.
124137012
Study of in-medium Delta Delta elastic scattering cross section
124278788
Covariant Description of the Δ in Relativistic Transport Theory
We have derived the relativistic Boltzmann-Uehling-Uhlenbeck equation for delta distribution function based on the same effective Lagrangian in which we derive the equation of nucleon. The equations of nucleon and delta are coupled with each other through self-energy terms and should be solved simultaneously.