NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = D.Wen Found 25 matches. 2024WU07 Chin.Phys.C 48, 024101 (2024) From masses and radii of neutron stars to EOS of nuclear matter through neural network
doi: 10.1088/1674-1137/ad0e04
2023SU11 Phys.Rev. C 108, 025801 (2023) Implications of supermassive neutron stars for the form of the equation of state of hybrid stars
doi: 10.1103/PhysRevC.108.025801
2022WA24 Eur.Phys.J. A 58, 132 (2022) Constraining properties of massive neutron star through R-mode
doi: 10.1140/epja/s10050-022-00781-z
2021LI10 Eur.Phys.J. A 57, 31 (2021) Constraining the nuclear symmetry energy and properties of the neutron star from GW170817 by Bayesian analysis
doi: 10.1140/epja/s10050-021-00342-w
2020MA08 Phys.Rev. C 101, 024904 (2020) H.-H.Ma, D.Wen, K.Lin, W.L.Qian, B.Wang, Y.Hama, T.Kodama Hydrodynamic results on multiplicity fluctuations in heavy-ion collisions
doi: 10.1103/PhysRevC.101.024904
2020WE12 Eur.Phys.J. A 56, 222 (2020) D.Wen, K.Lin, W.-L.Qian, B.Wang, Y.Hama, T.Kodama On nonlinearity in hydrodynamic response to the initial geometry in relativistic heavy-ion collisions
doi: 10.1140/epja/s10050-020-00235-4
2019CH17 Chin.Phys.C 43, 054108 (2019) Suitable resolution of EOS tables for neutron star investigations
doi: 10.1088/1674-1137/43/5/054108
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
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
2019ZH16 Phys.Rev. C 99, 035803 (2019) Imprint of the speed of sound in nuclear matter on global properties of neutron stars
doi: 10.1103/PhysRevC.99.035803
2017WE05 Phys.Rev. C 95, 065804 (2017) Theoretical constraints on the properties of low-mass neutron stars from the equation of state of nuclear matter in the inner crust
doi: 10.1103/PhysRevC.95.065804
2016CH52 Phys.Rev. C 94, 064621 (2016) S.-J.Cheng, G.-C.Yong, D.-H.Wen Effects of the symmetry energy in the 132Sn + 124Sn reaction at 300 MeV/nucleon NUCLEAR REACTIONS 124Sn(132Sn, X), E=300 MeV/nucleon; calculated neutron/proton and π-/π+ ratios with densities higher than the normal nuclear matter density, baryon density, average multiplicity and kinetic energy spectra of π- and π+, production of Δ resonances as a function of time. Isospin-dependent Boltzmann-Uehling-Uhlenbeck (IBUU) transport model. Relevance to ongoing experiments at RIBF-RIKEN facility using the SAMURAI time-projection chamber.
doi: 10.1103/PhysRevC.94.064621
2015LI05 Phys.Rev. C 91, 024604 (2015) Probing the momentum dependence of the symmetry potential by the free n/p ratio of pre-equilibrium emission NUCLEAR REACTIONS 124Sn(132Sn, X), E=200, 400 MeV/nucleon; calculated relative sensitivity of pre-equilibrium free n/p ratio, location of baryon number in momentum space as a function of time using IBUU04 transport model. Comparison with experimental data.
doi: 10.1103/PhysRevC.91.024604
2015LI12 Phys.Rev. C 91, 044609 (2015) Decomposition of the sensitivity of the symmetry energy observables NUCLEAR REACTIONS 197Au(197Au, X), E=200, 400 MeV/nucleon; calculated baryon density and probability distribution, relative sensitivity of the symmetry energy. Isospin-dependent IBUU transport model.
doi: 10.1103/PhysRevC.91.044609
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
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
2011LI12 Phys.Rev. C 83, 045802 (2011) W.Lin, B.Li, J.Xu, C.M.Ko, D.H.Wen Energy release from hadron-quark phase transition in neutron stars and the axial w mode of gravitational waves
doi: 10.1103/PhysRevC.83.045802
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
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
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
2008CH17 Phys.Rev. C 77, 065804 (2008) W.Chen, B.-j.Li, D.-h.Wen, L.-g.Liu 3P2 superfluidity in neutron star matter
doi: 10.1103/PhysRevC.77.065804
2006CH02 Chin.Phys.Lett. 23, 271 (2006) W.Chen, Y.-Y.Lam, D.-H.Wen, L.-G.Liu Influence of Hyperon on 1S0 Superfluidity of Nucleons in Neutron Star Matter
doi: 10.1088/0256-307X/23/1/078
2005CH41 Chin.J.Phys.(Taiwan) 43, 445 (2005) A Study of the Tachyon Pole in the Chiral σ-ω Model
2004WE10 Eur.Phys.J. A 21, 349 (2004) D.Wen, W.Chen, X.Wang, B.Ai, G.Liu, D.Dong, L.Liu Structures of rotating traditional neutron stars and hyperon stars in the relativistic σ-ω model
doi: 10.1140/epja/i2003-10214-0
2003CH21 Chin.Phys.Lett. 20, 436 (2003) Softness of Nuclear Matter and the Production of Strange Particles in Neutron Stars
doi: 10.1088/0256-307X/20/3/336
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