NSR Query Results
Output year order : Descending NSR database version of April 11, 2024. Search: Author = B.A.Li Found 187 matches. Showing 1 to 100. [Next]2023GU16 Phys.Rev. C 108, 034617 (2023) Interplay of effects of neutron skins in coordinate space and proton skins in momentum space on emission of hard photons in heavy-ion collisions near the Fermi energy
doi: 10.1103/PhysRevC.108.034617
2023LI20 Nucl.Phys. A1034, 122640 (2023) Principal Component Analysis of azimuthal flow in intermediate-energy heavy-ion reactions
doi: 10.1016/j.nuclphysa.2023.122640
2023LI46 Nucl.Phys. A1039, 122726 (2023) Bayesian inference of in-medium baryon-baryon scattering cross sections from HADES proton flow data
doi: 10.1016/j.nuclphysa.2023.122726
2023RI04 Phys.Rev. C 108, 055803 (2023) Empirical radius formulas for canonical neutron stars from bidirectionally selecting features of equations of state in extended Bayesian analyses of observational data
doi: 10.1103/PhysRevC.108.055803
2023ZH18 Eur.Phys.J. A 59, 86 (2023) Impact of symmetry energy on sound speed and spinodal decomposition in dense neutron-rich matter
doi: 10.1140/epja/s10050-023-01010-x
2023ZH42 Phys.Rev. C 108, 025803 (2023) Properties of first-order hadron-quark phase transition from inverting neutron star observables
doi: 10.1103/PhysRevC.108.025803
2022CA13 Phys.Rev. C 105, 064607 (2022) Investigating effects of relativistic kinematics, dimensionality, interactions, and short-range correlations on the ratio of quartic over quadratic nuclear symmetry energies
doi: 10.1103/PhysRevC.105.064607
2022YO08 Phys.Rev. C 106, 024902 (2022) G.-C.Yong, B.-A.Li, Z.-G.Xiao, Z.-W.Lin Probing the high-density nuclear symmetry energy with the Ξ-/Ξ0 ratio in heavy-ion collisions at √ sNN ≈ 3 GeV
doi: 10.1103/PhysRevC.106.024902
2021CA12 Phys.Rev. C 103, 034607 (2021) Intrinsic correlations among characteristics of neutron-rich matter imposed by the unbound nature of pure neutron matter
doi: 10.1103/PhysRevC.103.034607
2021CA15 Phys.Rev. C 103, 054611 (2021) Auxiliary function approach for determining symmetry energy at suprasaturation densities
doi: 10.1103/PhysRevC.103.054611
2021CO10 Phys.Rev. C 104, 024603 (2021) M.Colonna, Y.-X.Zhang, Y.-J.Wang, D.Cozma, P.Danielewicz, C.M.Ko, A.Ono, M.B.Tsang, R.Wang, H.Wolter, J.Xu, Z.Zhang, L.-W.Chen, H.-G.Cheng, H.Elfner, Z.-Q.Feng, M.Kim, Y.Kim, S.Jeon, C.-H.Lee, B.-A.Li, Q.-F.Li, Z.-X.Li, S.Mallik, D.Oliinychenko, J.Su, T.Song, A.Sorensen, F.-S.Zhang Comparison of heavy-ion transport simulations: Mean-field dynamics in a box
doi: 10.1103/PhysRevC.104.024603
2021GU23 Phys.Rev. C 104, 034603 (2021) Imprints of high-momentum nucleons in nuclei on hard photons from heavy-ion collisions near the Fermi energy NUCLEAR REACTIONS 124Sn(48Ca, X), E=45 MeV/nucleon; calculated multiplicity, production rate, and angular distributions of Eγ=50, 100, 150, 200, 250 MeV hard photons, transverse and longitudinal kinetic energies of nucleons in head-on collisions. 124Sn(48Ca, X), E=30, 45, 60 MeV/nucleon; calculated angular distributions of Eγ=50, 250 MeV. 12C(14N, X), E=20, 30, 40 MeV/nucleon; calculated Eγ<100 MeV hard photon energy spectra and angular distributions. 48Ca; calculated nucleon momentum distributions. Isospin- and momentum-dependent Boltzmann-Uehling-Uhlenbeck (IBUU04) transport model with and without nucleon high-momentum tail (HMT).
doi: 10.1103/PhysRevC.104.034603
2021LI51 Phys.Rev. C 104, 034610 (2021) Differential analysis of incompressibility in neutron-rich nuclei NUCLEAR STRUCTURE 40,42,44,46,48Ca, 106,108,110,112,114,116Cd, 112,114,116,118,120,122,124Sn, 204,206,208Pb; calculated isospin-dependent incompressibilty parameters of finite-mass nuclei and those of infinite nuclear matter by using a differential approach; and compared results with experiments at RCNP-Osaka on isoscalar giant monopole resonances (ISGMR) in even-even Pb, Sn, Cd, and Ca nuclei. Relevance to critical issues about nuclear matter compressibilities in nuclear physics and astrophysics.
doi: 10.1103/PhysRevC.104.034610
2021XI03 Phys.Rev. C 103, 035802 (2021) Bayesian inference of the dense-matter equation of state encapsulating a first-order hadron-quark phase transition from observables of canonical neutron stars
doi: 10.1103/PhysRevC.103.035802
2021XU05 Phys.Rev. C 104, 054324 (2021) Bayesian uncertainty quantification for nuclear matter incompressibility NUCLEAR STRUCTURE 208Pb, 120Sn; analyzed experimental data for centroid energies, electric polarizability in the isovector giant-dipole resonance (IVGDR), neutron-skin thickness and the excitation energy isoscalar giant monopole resonances (ISGMR) from RCNP-Japan, and Texas A and M University; deduced posterior probability distribution functions (PDFs) of isovector interaction parameters for 208Pb; deduced nuclear incompressibility. Bayesian statistical framework, with the standard Skyrme-Hartree-Fock model.
doi: 10.1103/PhysRevC.104.054324
2020LI44 Phys.Rev. C 102, 045807 (2020) Curvature-slope correlation of nuclear symmetry energy and its imprints on the crust-core transition, radius, and tidal deformability of canonical neutron stars
doi: 10.1103/PhysRevC.102.045807
2020XU08 Phys.Rev. C 102, 044316 (2020) Bayesian inference of nuclear symmetry energy from measured and imagined neutron skin thickness in 116, 118, 120, 122, 124, 130, 132Sn, 208Pb, and 48Ca NUCLEAR STRUCTURE 48Ca, 116,118,120,122,124,130,132Sn, 208Pb; calculated slope parameter of the symmetry energy, correlated posterior and prior probability distribution functions (PDFs) from real and imagined neutron skin thicknesses. Bayesian statistical framework using the Skyrme-Hartree-Fock model.
doi: 10.1103/PhysRevC.102.044316
2019LI39 Eur.Phys.J. A 55, 117 (2019) B.-A.Li, P.G.Krastev, D.-H.Wen, N.-B.Zhang Towards understanding astrophysical effects of nuclear symmetry energy
doi: 10.1140/epja/i2019-12780-8
2019ON02 Phys.Rev. C 100, 044617 (2019) A.Ono, J.Xu, M.Colonna, P.Danielewicz, C.M.Ko, M.B.Tsang, Y.-J.Wang, H.Wolter, Y.-X.Zhang, L.-W.Chen, D.Cozma, H.Elfner, Z.-Q.Feng, N.Ikeno, B.-A.Li, S.Mallik, Y.Nara, T.Ogawa, A.Ohnishi, D.Oliinychenko, J.Su, T.Song, F.-S.Zhang, Z.Zhang Comparison of heavy-ion transport simulations: Collision integral with pions and Δ resonances in a box
doi: 10.1103/PhysRevC.100.044617
2019WE05 Phys.Rev. C 99, 045806 (2019) D.-H.Wen, B.-A.Li, H.-Y.Chen, N.-B.Zhang GW170817 implications on the frequency and damping time of f-mode oscillations of neutron stars
doi: 10.1103/PhysRevC.99.045806
2019ZH19 Eur.Phys.J. A 55, 39 (2019) Extracting nuclear symmetry energies at high densities from observations of neutron stars and gravitational waves
doi: 10.1140/epja/i2019-12700-0
2018FA08 Phys.Rev. C 98, 025801 (2018) F.J.Fattoyev, E.F.Brown, A.Cumming, A.Deibel, C.J.Horowitz, B.-A.Li, Z.Lin Deep crustal heating by neutrinos from the surface of accreting neutron stars NUCLEAR REACTIONS 1H, Fe(p, π+), Fe(α, π+), E=290-550 MeV/nucleon; calculated multiplicity of pion production as a function of beam energy, total energy per accreted nucleon deposited by neutrinos in the inner crust for a neutron star using the four equations of state, total energy deposited by neutrinos into the inner crust; investigated a new mechanism of deep crustal heating of neutron stars in mass-transferring binaries by neutrinos from decay of charged pions produced at the surface of the neutron stars through p+p, p+Fe and α+Fe collisions.
doi: 10.1103/PhysRevC.98.025801
2018LI08 Prog.Part.Nucl.Phys. 99, 29 (2018) B.-An.Li, B.-J.Cai, L.-W.Chen, J.Xu Nucleon effective masses in neutron-rich matter
doi: 10.1016/j.ppnp.2018.01.001
2018SA46 Phys.Rev. C 98, 045801 (2018) H.S.Sahoo, G.Mitra, R.Mishra, P.K.Panda, B.-A.Li Neutron star matter with Δ isobars in a relativistic quark model
doi: 10.1103/PhysRevC.98.045801
2018WA31 Phys.Rev. C 98, 054608 (2018) H.-S.Wang, J.Xu, B.-A.Li, W.-Q.Shen Reexamining the isospin-relaxation time in intermediate-energy heavy-ion collisions NUCLEAR REACTIONS 40Ca(124Sn, X), E=25, 100, 200, 300 MeV/nucleon; calculated time evolutions of the ratio of the particle number in residues to the total particle number, and isospin equilibrium meter, isospin relaxation time as functions of symmetry energy and effective neutron-proton mass splitting. 70Zn(70Zn, X), E=35 MeV/nucleon; calculated contours of isospin asymmetry, correlation between the isospin asymmetry and reduced nucleon number density, time evolution of isovector dipole moment as function of symmetry energies and effective neutron-proton mass splittings. Isospin-dependent Boltzmann-Uehling-Uhlenbeck (IBUU) transport model using the lattice Hamiltonian method to calculate the mean-field potential from the improved isospin- and momentum-dependent interaction (ImMDI).
doi: 10.1103/PhysRevC.98.054608
2018WE03 Phys.Rev. C 97, 034620 (2018) G.-F.Wei, B.-A.Li, G.-C.Yong, L.Ou, X.-W.Cao, X.-Y.Liu Effects of retarded electrical fields on observables sensitive to the high-density behavior of the nuclear symmetry energy in heavy-ion collisions at intermediate energies NUCLEAR REACTIONS 197Au(197Au, X), E=400 MeV/nucleon; calculated contours of the electric fields and densities at the initial compression, maximum compression, and expansion stage, time evolution of π-/π+ ratio with symmetry energies, multiplicities of π- and π+, impact parameter dependence of π-/π+ ratio, ratio for neutrons and protons at supra-saturation densities at the maximum compression stage as a function of nucleon kinetic energy, neutron-proton differential flow in central and peripheral collisions; deduced effects of relativistically retarded electrical fields on π-/π+ ratio and neutron-proton differential transverse flow. Isospin- and momentum-dependent transport model IBUU11.
doi: 10.1103/PhysRevC.97.034620
2018ZH12 Phys.Rev. C 97, 034625 (2018) Y.-X.Zhang, Y.-J.Wang, M.Colonna, P.Danielewicz, A.Ono, M.B.Tsang, H.Wolter, J.Xu, L.-W.Chen, D.Cozma, Z.-Q.Feng, S.Das Gupta, N.Ikeno, C.-M.Ko, B.-A.Li, Q.-F.Li, Z.-X.Li, S.Mallik, Y.Nara, T.Ogawa, A.Ohnishi, D.Oliinychenko, M.Papa, H.Petersen, J.Su, T.Song, J.Weil, N.Wang, F.g-S.Zhang, Z.Zhang Comparison of heavy-ion transport simulations: Collision integral in a box
doi: 10.1103/PhysRevC.97.034625
2017KO08 Phys.Rev. C 95, 034324 (2017) H.-Y.Kong, J.Xu, L.-W.Chen, B.-A.Li, Y.-G.Ma Constraining simultaneously nuclear symmetry energy and neutron-proton effective mass splitting with nucleus giant resonances using a dynamical approach NUCLEAR STRUCTURE 208Pb; calculated parameters for the isovector giant dipole resonance (IVGDR), time evolution of the isoscalar giant dipole and quadrupole moments, correlation between the corresponding excitation energy and the isoscalar nucleon effective mass, symmetry energy slope parameter and the isovector nucleon effective mass as function of centroid energy and the electric dipole polarizability, Improved isospin- and momentum-dependent interaction (ImMDI) and an isospin-dependent Boltzmann-Uehling-Uhlenbeck (IBUU) transport mode.
doi: 10.1103/PhysRevC.95.034324
2017XI14 Phys.Rev. C 96, 044618 (2017) Y.Xia, J.Xu, B.-A.Li, W.-Q.Shen Simulating spin dynamics with spin-dependent cross sections in heavy-ion collisions NUCLEAR REACTIONS 1H(n, n), (p, p), E=100 MeV; 1n(n, n), E=100 MeV; calculated total elastic spin-averaged, spin-singlet, and spin-triplet cross sections, differential cross sections and spin-averaged differential cross sections. 197Au(197Au, X), E=100 MeV/nucleon; calculated rapidity dependence of spin differential transverse flow from spin-averaged and spin-dependent cross sections, rapidity dependence of elliptic flow of free nucleons and deuterons from the spin-averaged and the spin dependent cross sections. Spin-dependent Boltzmann-Uehling-Uhlenbeck transport model.
doi: 10.1103/PhysRevC.96.044618
2017YO08 Phys.Rev. C 96, 064614 (2017) Interplay of short-range correlations and nuclear symmetry energy in hard-photon production from heavy-ion reactions at Fermi energies NUCLEAR REACTIONS 112Sn(40Ca, γ), (48Ca, γ), (56Ca, γ), 112Sn(48Ca, γ), E=45 MeV/nucleon; calculated effect of high-momentum tails (HMTs) of single-nucleon momentum distributions on the hard photon yields in head-on collisions, effect of symmetry energy on the ratio of hard photon productions in neutron-rich and neutron-deficient reactions. Isospin- and momentum-dependent transport model for nucleon-nucleon short-range correlations (SRCs) and nuclear symmetry energy. NUCLEAR STRUCTURE 40,48Ca, 56Fe; calculated nucleon momentum distribution using the local Thomas-Fermi approximation. Comparison with experimental data.
doi: 10.1103/PhysRevC.96.064614
2016CA04 Phys.Rev. C 93, 014619 (2016) Symmetry energy of cold nucleonic matter within a relativistic mean field model encapsulating effects of high-momentum nucleons induced by short-range correlations
doi: 10.1103/PhysRevC.93.014619
2016CA40 Phys.Rev. C 94, 061302 (2016) Proton skins in momentum space and neutron skins in coordinate space in heavy nuclei NUCLEAR STRUCTURE 208Pb; calculated reduced nucleon momentum distribution of neutron-rich nucleonic matter, correlation between neutron skin and proton skin using high-momentum tail (HMT)-experimental and HMT-self-consistent Green's function (SCGF) parameter sets; deduced protons move faster than neutrons in neutron skins of heavy nuclei, neutron-proton (np) (isospin) asymmetry dependence of nuclear equation of state (EOS).
doi: 10.1103/PhysRevC.94.061302
2016XI09 Nucl.Phys. A955, 41 (2016) Y.Xia, J.Xu, B.-A.Li, W.-Q.Shen Spin transport in intermediate-energy heavy-ion collisions as a probe of in-medium spin-orbit interactions NUCLEAR REACTIONS 124Sn(124Sn, x), 197Au(197Au, x), E=50, 100, 200 MeV/nucleon; calculated nucleons and clusters directed and elliptic flows, spin-up and spin-down polarizations for different impact parameters using BUU transport code SIBIUU12.
doi: 10.1016/j.nuclphysa.2016.06.001
2016XU03 Phys.Rev. C 93, 044609 (2016) J.Xu, L.-W.Chen, M.Y.B.Tsang, H.Wolter, Y.-X.Zhang, J.Aichelin, M.Colonna, D.Cozma, P.Danielewicz, Z.-Q.Feng, A.Le Fevre, T.Gaitanos, C.Hartnack, K.Kim, Y.Kim, C.-M.Ko, B.-A.Li, Q.-F.Li, Z.-X.Li, P.Napolitani, A.Ono, M.Papa, T.Song, J.Su, J.-L.Tian, N.Wang, Y.-J.Wang, J.Weil, W.-J.Xie, F.-S.Zhang, G.-Q.Zhang Understanding transport simulations of heavy-ion collisions at 100A and 400A MeV: Comparison of heavy-ion transport codes under controlled conditions
doi: 10.1103/PhysRevC.93.044609
2015CA11 Phys.Rev. C 92, 011601 (2015) Isospin quartic term in the kinetic energy of neutron-rich nucleonic matter
doi: 10.1103/PhysRevC.92.011601
2015CA14 Phys.Rev. C 92, 015802 (2015) B.-J.Cai, F.J.Fattoyev, B.-A.Li, W.G.Newton Critical density and impact of Δ (1232) resonance formation in neutron stars
doi: 10.1103/PhysRevC.92.015802
2015HE03 Phys.Rev. C 91, 015810 (2015) X.-T.He, F.J.Fattoyev, B.-A.Li, W.G.Newton Impact of the equation-of-state-gravity degeneracy on constraining the nuclear symmetry energy from astrophysical observables
doi: 10.1103/PhysRevC.91.015810
2015HE07 Phys.Rev. C 91, 025803 (2015) O.Hen, B.-A.Li, W.-J.Guo, L.B.Weinstein, E.Piasetzky Symmetry energy of nucleonic matter with tensor correlations
doi: 10.1103/PhysRevC.91.025803
2015JI11 Eur.Phys.J. A 51, 119 (2015) W.-Z.Jiang, B.-A.Li, F.J.Fattoyev Small radii of neutron stars as an indication of novel in-medium effects
doi: 10.1140/epja/i2015-15119-7
2015KO12 Phys.Rev. C 91, 047601 (2015) H.-Y.Kong, Y.Xia, J.Xu, L.-W.Chen, B.-A.Li, Y.-G.Ma Reexamination of the neutron-to-proton-ratio puzzle in intermediate-energy heavy-ion collisions
doi: 10.1103/PhysRevC.91.047601
2015LI11 Phys.Rev. C 91, 044601 (2015) Effects of the kinetic symmetry energy reduced by short-range correlations in heavy-ion collisions at intermediate energies NUCLEAR REACTIONS 112Sn(112Sn, X), 124Sn(124Sn, X), E=50, 120 MeV/nucleon; calculated neutron/proton ratios as function of impact parameter, kinetic and potential symmetry energies, and transverse momentum. 197Au(197Au, X), E=400 MeV/nucleon; calculated π-/π+ ratio as function of impact parameter. Discussed role of isospin degree of freedom in heavy-ion collisions. Isospin-dependent Boltzmann-Uehling-Uhlenbeck (IBUU) transport model.
doi: 10.1103/PhysRevC.91.044601
2015LI36 Phys.Rev. C 92, 034603 (2015) Symmetry potential of the Δ(1232) resonance and its effects on the π-/π+ ratio in heavy-ion collisions near the pion-production threshold
doi: 10.1103/PhysRevC.92.034603
2015XU03 Phys.Rev. C 91, 014611 (2015) Thermal properties of asymmetric nuclear matter with an improved isospin- and momentum-dependent interaction
doi: 10.1103/PhysRevC.91.014611
2014CH07 Eur.Phys.J. A 50, 29 (2014) L.-W.Chen, C.M.Ko, B.-A.Li, C.Xu, J.Xu Probing isospin- and momentum-dependent nuclear effective interactions in neutron-rich matter
doi: 10.1140/epja/i2014-14029-6
2014FA05 Eur.Phys.J. A 50, 45 (2014) F.J.Fattoyev, W.G.Newton, B.-A.Li Probing the high-density behavior of symmetry energy with gravitational waves
doi: 10.1140/epja/i2014-14045-6
2014FA12 Phys.Rev. C 90, 022801 (2014) F.J.Fattoyev, W.G.Newton, B.-A.Li Quantifying correlations between isovector observables and the density dependence of the nuclear symmetry energy away from saturation density NUCLEAR STRUCTURE 48Ca, 208Pb; calculated correlations between nuclear symmetry energy S(ρ) and its slope L(ρ), neutron skin thickness, radii of neutron stars, and the crust-core transition pressure for different densities using Skyrme models SLy4 and NRAPR.
doi: 10.1103/PhysRevC.90.022801
2014LI05 Eur.Phys.J. A 50, 9 (2014) B.-A.Li, A.Ramos, G.Verde, I.Vidana Topical issue on nuclear symmetry energy
doi: 10.1140/epja/i2014-14009-x
2014NE02 Eur.Phys.J. A 50, 41 (2014) W.G.Newton, J.Hooker, M.Gearheart, K.Murphy, D.-H.Wen, F.J.Fattoyev, B.-A.Li Constraints on the symmetry energy from observational probes of the neutron star crust
doi: 10.1140/epja/i2014-14041-x
2014WE07 Phys.Rev. C 90, 014610 (2014) G.-F.Wei, B.-A.Li, J.Xu, L.-W.Chen Influence of neutron-skin thickness on the π-/π+ ratio in Pb + Pb collisions
doi: 10.1103/PhysRevC.90.014610
2014XI03 Eur.Phys.J. A 50, 37 (2014) Z.-G.Xiao, G.-C.Yong, L.-W.Chen, B.-A.Li, M.Zhang, G.-Q.Xiao, N.Xu Probing nuclear symmetry energy at high densities using pion, kaon, eta and photon productions in heavy-ion collisions
doi: 10.1140/epja/i2014-14037-6
2014XI04 Phys.Rev. C 89, 064606 (2014) Y.Xia, J.Xu, B.-A.Li, W.-Q.Shen Spin-orbit coupling and the up-down differential transverse flow in intermediate-energy heavy-ion collisions
doi: 10.1103/PhysRevC.89.064606
2014XU04 Eur.Phys.J. A 50, 21 (2014) Relationship between the symmetry energy and the single-nucleon potential in isospin-asymmetric nucleonic matter
doi: 10.1140/epja/i2014-14021-2
2013FA02 Phys.Rev. C 87, 015806 (2013) F.J.Fattoyev, J.Carvajal, W.G.Newton, B.-A.Li Constraining the high-density behavior of the nuclear symmetry energy with the tidal polarizability of neutron stars
doi: 10.1103/PhysRevC.87.015806
2013XU10 Phys.Rev. C 87, 067601 (2013) J.Xu, L.-W.Chen, C.M.Ko, B.-A.Li, Y.-G.Ma Energy dependence of pion in-medium effects on the π-/π+ ratio in heavy-ion collisions
doi: 10.1103/PhysRevC.87.067601
2012CH08 Phys.Rev. C 85, 024305 (2012) R.Chen, B.-J.Cai, L.-W.Chen, B.-A.Li, X.-H.Li, C.Xu Single-nucleon potential decomposition of the nuclear symmetry energy
doi: 10.1103/PhysRevC.85.024305
2012FA09 Phys.Rev. C 86, 025804 (2012) F.J.Fattoyev, W.G.Newton, J.Xu, B.-A.Li Generic constraints on the relativistic mean-field and Skyrme-Hartree-Fock models from the pure neutron matter equation of state NUCLEAR STRUCTURE 112,114,116,118,120,122,124,126,128,130,132Sn, 208Pb; calculated nuclear symmetry energy, neutron skin thickness. Microscopic pure neutron matter (PNM) calculations using relativistic mean-field (RMF) and Skyrme-Hartree-Fock (SHF) models with IU-FSU and SkIU-FSU parametrizations. 40,48Ca, 78Ni, 90Zr, 132Sn, 208Pb; analyzed relative deviation of the binding energies and charge radii. Comparison with experimental data. Discussed predictions of neutron skin thicknesses and neutron star radii.
doi: 10.1103/PhysRevC.86.025804
2012WE01 Phys.Rev. C 85, 025801 (2012) Sensitivity of the neutron star r-mode instability window to the density dependence of the nuclear symmetry energy
doi: 10.1103/PhysRevC.85.025801
2012XU08 Phys.Rev. C 86, 044623 (2012) Disentangling effects of collision geometry and symmetry energy in U + U collisions NUCLEAR REACTIONS 238U(238U, X), E=0.52 GeV/nucleon; calculated time evolution of the density contours, transverse flow, elliptic flow, n/p and π-/π+ ratios. Isospin-dependent Boltzmann-Uehling-Uhlenbeck (IBUU) transport model.
doi: 10.1103/PhysRevC.86.044623
2011LI54 J.Phys.:Conf.Ser. 312, 042006 (2011) B.-A.Li, L.-W.Chen, M.Gearheart, J.Hooker, C.M.Ko, P.G.Krastev, W.-K.Lin, W.G.Newton, D.-H.Wen, C.Xu, J.Xu Imprints of Nuclear Symmetry Energy on Properties of Neutron Stars
doi: 10.1088/1742-6596/312/4/042006
2011OU02 Phys.Rev. C 84, 064605 (2011) Magnetic effects in heavy-ion collisions at intermediate energies
doi: 10.1103/PhysRevC.84.064605
2011XU06 Nucl.Phys. A865, 1 (2011) C.Xu, B.-A.Li, L.-W.Chen, C.M.Ko Analytical relations between nuclear symmetry energy and single-nucleon potentials in isospin asymmetric nuclear matter
doi: 10.1016/j.nuclphysa.2011.06.027
2010CH34 Phys.Rev. C 82, 024321 (2010) L.-W.Chen, Che Ming Ko, B.-A.Li, J.Xu Density slope of the nuclear symmetry energy from the neutron skin thickness of heavy nuclei NUCLEAR STRUCTURE 16O, 40,48Ca, 56,78Ni, 90Zr, 100,120,132Sn, 208Pb; calculated binding energies, charge rms radii, and neutron skin thickness using Skyrme-Hartree-Fock approach. Comparison with experimental data.
doi: 10.1103/PhysRevC.82.024321
2010CH37 Nucl.Phys. A834, 664c (2010) L.-W.Chen, B.-A.Li, H.-R.Ma, J.Xu Nuclear constraints on the inner edge of neutron star crusts
doi: 10.1016/j.nuclphysa.2010.01.118
2010KE03 Phys.Rev. C 81, 054602 (2010) A.L.Keksis, L.W.May, G.A.Souliotis, M.Veselsky, S.Galanopoulos, Z.Kohley, D.V.Shetty, S.N.Soisson, B.C.Stein, R.Tripathi, S.Wuenschel, S.J.Yennello, B.A.Li Experimental studies of N/Z equilibration in peripheral collisions using fragment yield ratios NUCLEAR REACTIONS 112Sn, 124Sn(40Ca, X), 112Sn, 124Sn(48Ca, X), E=32 MeV; measured fragment spectra; deduced quasiprojectile N/Z ratio. Comparison with deep-inelastic transfer (DIT) code, statistical multifragmentation model (SMM), and isospin-dependent Boltzmann-Uehling-Uhlenbeck (IBUU) microscopic transport model.
doi: 10.1103/PhysRevC.81.054602
2010LI34 Nucl.Phys. A834, 509c (2010) B.-A.Li, L.-W.Chen, D.-H.Wen, Z.Xiao, C.Xu, G.-C.Yong, M.Zhang Recent Progress in Constraining the Equation of State of Dense Neutron-Rich Nuclear Matter with Heavy-Ion Reactions
doi: 10.1016/j.nuclphysa.2010.01.079
2010XU02 Phys.Rev. C 81, 044603 (2010) Improved single particle potential for transport model simulations of nuclear reactions induced by rare isotope beams
doi: 10.1103/PhysRevC.81.044603
2010XU06 Phys.Rev. C 81, 055803 (2010) J.Xu, L.-W.Chen, C.M.Ko, B.-A.Li Isospin- and momentum-dependent effective interactions for the baryon octet and the properties of hybrid stars
doi: 10.1103/PhysRevC.81.055803
2010XU07 Phys.Rev. C 81, 055805 (2010) J.Xu, L.-W.Chen, C.M.Ko, B.-A.Li Transition density and pressure in hot neutron stars
doi: 10.1103/PhysRevC.81.055805
2010XU08 Phys.Rev. C 81, 064612 (2010) Understanding the major uncertainties in the nuclear symmetry energy at suprasaturation densities
doi: 10.1103/PhysRevC.81.064612
2010XU10 Phys.Rev. C 82, 054607 (2010) Symmetry energy, its density slope, and neutron-proton effective mass splitting at normal density extracted from global nucleon optical potentials
doi: 10.1103/PhysRevC.82.054607
2010ZH36 Nucl.Phys. A834, 567c (2010) M.Zhang, Z.-G.Xiao, B.-A.Li, L.-W.Chen, G.-C.Young, S.-J.Zhu System size and beam energy effects on probing the high-density behavior of nuclear symmetry energy with pion ratio NUCLEAR REACTIONS 48Ca(48Ca, π+), (48Ca, π-), 124Sn(124Sn, π+), (124Sn, π-), 197Au(197Au, π+), (197Au, π-), E=0.25-0.6 GeV/nucleon; measured pion production yield ratios; deduced radii, symmetry energy. Comparison with isobar model.
doi: 10.1016/j.nuclphysa.2010.01.093
2009CH34 Phys.Rev. C 80, 014322 (2009) L.-W.Chen, B.-J.Cai, C.M.Ko, B.-A.Li, C.Shen, J.Xu Higher-order effects on the incompressibility of isospin asymmetric nuclear matter
doi: 10.1103/PhysRevC.80.014322
2009JI07 Phys.Rev. C 80, 044322 (2009) Effects of medium-induced ρ-ω meson mixing on the equation of state in isospin-asymmetric nuclear matter
doi: 10.1103/PhysRevC.80.044322
2009NE15 Phys.Rev. C 80, 065809 (2009) Constraining the gravitational binding energy of PSR J0737-3039B using terrestrial nuclear data
doi: 10.1103/PhysRevC.80.065809
2009WE03 Phys.Rev. C 80, 025801 (2009) D.-H.Wen, B.-A.Li, P.G.Krastev Imprints of the nuclear symmetry energy on gravitational waves from the axial w-modes of neutron stars
doi: 10.1103/PhysRevC.80.025801
2009XI01 Phys.Rev.Lett. 102, 062502 (2009) Z.Xiao, B.-A.Li, L.-W.Chen, G.-C.Yong, M.Zhang Circumstantial Evidence for a Soft Nuclear Symmetry Energy at Suprasaturation Densities
doi: 10.1103/PhysRevLett.102.062502
2009XU04 Phys.Rev. C 79, 035802 (2009) J.Xu, L.-W.Chen, B.-A.Li, H.-R.Ma Locating the inner edge of the neutron star crust using terrestrial nuclear laboratory data
doi: 10.1103/PhysRevC.79.035802
2009YO07 Phys.Rev. C 80, 044608 (2009) G.-C.Yong, B.-A.Li, L.-W.Chen, Xu.-C.Zhang Triton-3He relative and differential flows as probes of the nuclear symmetry energy at supra-saturation densities NUCLEAR REACTIONS 132Sn(124Sn, X), E=400 MeV/nucleon; calculated multiplicities and transverse flows of triton and 3He as a function of reduced rapidity in c.m. system using transport model calculations coupled with a phase-space coalescence afterburner. Discussed neutron and proton transverse flows.
doi: 10.1103/PhysRevC.80.044608
2009ZH14 Chin.Phys.Lett. 26, 052502 (2009) X.-C.Zhang, B.-A.Li, L.-W.Chen, G.-C.Yong Impact Parameter Dependence of the Double Neutron/Proton Ratio of Nucleon Emissions in Isotopic Reaction Systems NUCLEAR REACTIONS 124Sn(124Sn, xn), (124Sn, xp), E=50 MeV/nucleon; 112Sn(112Sn, xn), (112Sn, xn), E=50 MeV/nucleon; calculated double neutron/proton ratio of nucleon emissions, neutron spectra, proton spectra; deduced neutron/proton ratio dependence on symmetry energy. IBUU04 transport model.
doi: 10.1088/0256-307X/26/5/052502
2009ZH27 Phys.Rev. C 80, 034616 (2009) M.Zhang, Z.-G.Xiao, B.-A.Li, L.-W.Chen, G.-C.Yong, S.-J.Zhu Systematic study of the π-/π+ratio in heavy-ion collisions with the same neutron/proton ratio but different masses
doi: 10.1103/PhysRevC.80.034616
2008CH29 Int.J.Mod.Phys. E17, 1825 (2008) L.-W.Chen, C.M.Ko, B.-A.Li, G.-C.Yong Determining the density dependence of the nuclear symmetry energy using heavy-ion reactions
doi: 10.1142/S0218301308010817
2008LI09 J.Phys.(London) G35, 014044 (2008) B.-A.Li, L.-W.Chen, C.M.Ko, P.G.Krastev, A.W.Steiner, G.-C.Yong Constraining properties of neutron stars with heavy-ion reactions in terrestrial laboratories
doi: 10.1088/0954-3899/35/1/014044
2008YO01 Phys.Lett. B 661, 82 (2008) Neutron-proton bremsstrahlung from intermediate energy heavy-ion reactions as a probe of the nuclear symmetry energy? NUCLEAR REACTIONS 112Sn(112Sn, X), 124Sn(132Sn, X), E=50 MeV/nucleon; calculated hard photon yields and ratios, sensitivity to symmetry energy. Isospin- and momentum-dependent transport model. 12C(12C, X), E=45-85 MeV; analyzed inclusive photon production σ.
doi: 10.1016/j.physletb.2008.02.013
2007CH03 Chin.Phys.Lett. 24, 76 (2007) J.-Y.Chen, W.Zuo, L.Ma, F.Zhang, B.-A.Li Probing Balance Energy Using Momentum- and Isospin-Dependent Potential NUCLEAR REACTIONS 58Fe(48Ca, X), 58Ni(48Cr, X), E=50-90 MeV/nucleon; calculated transverse flow parameters, balance energy; deduced sensitivity to density dependence of symmetry energy.
doi: 10.1088/0256-307X/24/1/021
2007CH75 Phys.Rev. C 76, 054316 (2007) Isospin-dependent properties of asymmetric nuclear matter in relativistic mean field models NUCLEAR STRUCTURE Sn; calculated giant monopole resonances using relativistic mean field theory for even-A isotopes.
doi: 10.1103/PhysRevC.76.054316
2007JI12 Phys.Rev. C 76, 044604 (2007) W.-Z.Jiang, B.-A.Li, L.-W.Chen Mean free paths and in-medium scattering cross sections of energetic nucleons in neutron-rich nucleonic matter within the relativistic impulse approximation
doi: 10.1103/PhysRevC.76.044604
2007JI15 Phys.Rev. C 76, 054314 (2007) W.-Z.Jiang, B.-A.Li, L.-W.Chen Neutron-skin thickness of finite nuclei in relativistic mean-field models with chiral limits NUCLEAR STRUCTURE 16O, 40,48Ca, 90Zr, 114,132Sn, 208Pb; calculated binding energy, charge radii, neutron skin thickness using different theoretical models. Comparison with experimental data.
doi: 10.1103/PhysRevC.76.054314
2007KR16 Phys.Rev. C 76, 055804 (2007) Constraining a possible time variation of the gravitational constant G with terrestrial nuclear laboratory data
doi: 10.1103/PhysRevC.76.055804
2007LI68 Phys.Rev. C 76, 051601 (2007) B.-A.Li, L.-W.Chen, H.-R.Ma, J.Xu, G.-C.Yong Differential isospin-fractionation in dilute asymmetric nuclear matter NUCLEAR REACTIONS 124Sn(124Sn, X), E=50 MeV/nucleon; 124Sn(132Sn, X), E=400 MeV/nucleon; calculated neutron/proton ratios in gas and liquid phases.
doi: 10.1103/PhysRevC.76.051601
2007XU01 Phys.Rev. C 75, 014607 (2007) J.Xu, L.-W.Chen, B.-A.Li, H.-R.Ma Temperature effects on the nuclear symmetry energy and symmetry free energy with an isospin and momentum dependent interaction
doi: 10.1103/PhysRevC.75.014607
2007XU10 Phys.Lett. B 650, 348 (2007) J.Xu, L.-W.Chen, B.-A.Li, H.-R.Ma Effects of isospin and momentum dependent interactions on liquid-gas phase transition in hot asymmetric nuclear matter
doi: 10.1016/j.physletb.2007.05.035
2007YO04 Phys.Lett. B 650, 344 (2007) The neutron/proton ratio of squeezed-out nucleons and the high density behavior of the nuclear symmetry energy
doi: 10.1016/j.physletb.2007.05.050
2006CH55 Int.J.Mod.Phys. E15, 1385 (2006) Constraining the Skyrme effective interactions and the neutron skin thickness of nuclei using isospin diffusion data from heavy ion collisions NUCLEAR STRUCTURE 48Ca, 124,132Sn, 208Pb; analyzed data; deduced neutron skin thickness, symmetry energy parameters.
doi: 10.1142/S0218301306004946
2006DI15 Eur.Phys.J. A 30, 153 (2006) M.Di Toro, S.J.Yennello, B.-A.Li Isospin flows
doi: 10.1140/epja/i2006-10113-x
2006LI10 Phys.Lett. B 634, 378 (2006) B.-A.Li, L-W.Chen, G.-C.Young, W.Zuo Double neutron/proton ratio of nucleon emissions in isotopic reaction system as a robust probe of nuclear symmetry energy NUCLEAR REACTIONS 112Sn(112Sn, X), 124Sn(124Sn, X), E=50 MeV/nucleon; 112Sn(112Sn, X), 124Sn(132Sn, X), E=400 MeV/nucleon; calculated double neutron/proton yield ratios; deduced dependence on symmetry energy. Transport model.
doi: 10.1016/j.physletb.2006.02.003
2006LI47 Phys.Rev. C 74, 034610 (2006) Evolution of the symmetry energy of hot neutron-rich matter formed in heavy-ion reactions
doi: 10.1103/PhysRevC.74.034610
2006LI51 Phys.Rev. C 74, 044613 (2006) Z.-H.Li, L.-W.Chen, C.M.Ko, B.-A.Li, H.-R.Ma Nuclear symmetry potential in the relativistic impulse approximation
doi: 10.1103/PhysRevC.74.044613
2006LI61 Phys.Lett. B 642, 436 (2006) Constraining the radii of neutron stars with terrestrial nuclear laboratory data
doi: 10.1016/j.physletb.2006.09.065
2006YO02 Phys.Rev. C 73, 034603 (2006) G.-C.Yong, B.-A.Li, L.-W.Chen, W.Zuo Single and double π- /π+ ratios in heavy-ion reactions as probes of the high-density behavior of the nuclear symmetry energy NUCLEAR REACTIONS 112Sn(112Sn, X), 124Sn(132Sn, X), E=400 MeV/nucleon; calculated charged pion yield ratios, sensitivity to symmetry energy. Isospin- and momentum-dependent transport model.
doi: 10.1103/PhysRevC.73.034603
2006YO10 Phys.Rev.C 74, 064617 (2006) Double neutron-proton differential transverse flow as a probe for the high density behavior of the nuclear symmetry energy NUCLEAR REACTIONS 112Sn(112Sn, X), 124Sn(132Sn, X), E=400, 800 MeV/nucleon; calculated neutron-proton differential transverse flow, dependence on nuclear symmetry energy.
doi: 10.1103/PhysRevC.74.064617
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