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NSR database version of April 27, 2024.

Search: Author = D.H.Wen

Found 16 matches.

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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
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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
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2017WE05      Phys.Rev. C 95, 065804 (2017)

Y.-M.Wen, D.-H.Wen

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
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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
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2015LI05      Phys.Rev. C 91, 024604 (2015)

H.-L.Liu, G.-C.Yong, D.-H.Wen

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
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2015LI12      Phys.Rev. C 91, 044609 (2015)

H.-l.Liu, G.-C.Yong, D.-H.Wen

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
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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
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2012WE01      Phys.Rev. C 85, 025801 (2012)

D.-H.Wen, W.G.Newton, B.-A.Li

Sensitivity of the neutron star r-mode instability window to the density dependence of the nuclear symmetry energy

doi: 10.1103/PhysRevC.85.025801
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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
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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
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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
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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
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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
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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
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2005CH41      Chin.J.Phys.(Taiwan) 43, 445 (2005)

W.Chen, D.-h.Wen, L.-g.Liu

A Study of the Tachyon Pole in the Chiral σ-ω Model

2003CH21      Chin.Phys.Lett. 20, 436 (2003)

W.Chen, D.-H.Wen, L.-G.Liu

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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