Publication data of Wen, De-Hua: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion2002200420062008201020122014201620182020202220240200400600800
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications201020202005201520250122436486001.534.567.5
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion2002200420062008201020122014201620182020202220240246810121416
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestProbing the momentum dependence of the symmetry potential by the free n/p ratio of pre-equilibrium emissionProbing the momentum dependence of the symmetry potential by the free n…High-density nuclear symmetry energy extracted from astrophysical observationsHigh-density nuclear symmetry energy extracted from astrophysical observa…Effects of symmetry energy in the $^{132} m {Sn}+^{124} m {Sn}$ reaction at 300 MeV/nucleonEffects of symmetry energy in the $^{132} m {Sn}+^{124} m {Sn}$ rea…Implications of supermassive neutron stars for the form of the equation of state of hybrid starsImplications of supermassive neutron stars for the form of the equation of st…Energy release from hadron-quark phase transition in neutron stars and the axial $w$-mode of gravitational wavesEnergy release from hadron-quark phase transition in neutron stars and the …New quasi-universal relations for static and rapid rotating neutron starsImprints of Nuclear Symmetry Energy on Properties of Neutron StarsUniversal behavior of a compact star based upon the gravitational binding energyUniversal behavior of a compact star based upon the gravitational binding e…Can the maximum mass of neutron stars rule out any equation of state of dense stellar matter before gravity is well understood?Can the maximum mass of neutron stars rule out any equation of state of de…Decomposition of the sensitivity of the symmetry energy observablesImprint of the speed of sound in nuclear matter on global properties of neutron starsImprint of the speed of sound in nuclear matter on global properties of neutr…Breaking the EOS-Gravity Degeneracy with Masses and Pulsating Frequencies of Neutron StarsBreaking the EOS-Gravity Degeneracy with Masses and Pulsating Frequencies…Constraining the nuclear symmetry energy and properties of the neutron star from GW170817 by Bayesian analysisConstraining the nuclear symmetry energy and properties of the neutron sta…Imprints of the nuclear symmetry energy on gravitational waves from the axial w-modes of neutron starsImprints of the nuclear symmetry energy on gravitational waves from the axi…Constraints on the symmetry energy from observational probes of the neutron star crustConstraints on the symmetry energy from observational probes of the neutro…GW170817 implications on the frequency and damping time of f-mode oscillations of neutron starsGW170817 implications on the frequency and damping time of f-mode oscill…Sensitivity of the neutron star r-mode instability window to the density dependence of the nuclear symmetry energySensitivity of the neutron star r-mode instability window to the density depe…Super-soft symmetry energy encountering non-Newtonian gravity in neutron starsSuper-soft symmetry energy encountering non-Newtonian gravity in neutron…Towards Understanding Astrophysical Effects of Nuclear Symmetry Energy2002200420062008201020122014201620182020202220240200400600800
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Probing the momentum dependence of the symmetry potential by the free n/p ratio of pre-equilibrium emissionProbing the momentum dependence of the symmetry potential by the free n…High-density nuclear symmetry energy extracted from astrophysical observationsHigh-density nuclear symmetry energy extracted from astrophysical observa…Effects of symmetry energy in the $^{132} m {Sn}+^{124} m {Sn}$ reaction at 300 MeV/nucleonEffects of symmetry energy in the $^{132} m {Sn}+^{124} m {Sn}$ rea…Implications of supermassive neutron stars for the form of the equation of state of hybrid starsImplications of supermassive neutron stars for the form of the equation of st…Energy release from hadron-quark phase transition in neutron stars and the axial $w$-mode of gravitational wavesEnergy release from hadron-quark phase transition in neutron stars and the …New quasi-universal relations for static and rapid rotating neutron starsImprints of Nuclear Symmetry Energy on Properties of Neutron StarsUniversal behavior of a compact star based upon the gravitational binding energyUniversal behavior of a compact star based upon the gravitational binding e…Can the maximum mass of neutron stars rule out any equation of state of dense stellar matter before gravity is well understood?Can the maximum mass of neutron stars rule out any equation of state of de…Decomposition of the sensitivity of the symmetry energy observablesImprint of the speed of sound in nuclear matter on global properties of neutron starsImprint of the speed of sound in nuclear matter on global properties of neutr…Breaking the EOS-Gravity Degeneracy with Masses and Pulsating Frequencies of Neutron StarsBreaking the EOS-Gravity Degeneracy with Masses and Pulsating Frequencies…Constraining the nuclear symmetry energy and properties of the neutron star from GW170817 by Bayesian analysisConstraining the nuclear symmetry energy and properties of the neutron sta…Imprints of the nuclear symmetry energy on gravitational waves from the axial w-modes of neutron starsImprints of the nuclear symmetry energy on gravitational waves from the axi…Constraints on the symmetry energy from observational probes of the neutron star crustConstraints on the symmetry energy from observational probes of the neutro…GW170817 implications on the frequency and damping time of f-mode oscillations of neutron starsGW170817 implications on the frequency and damping time of f-mode oscill…Sensitivity of the neutron star r-mode instability window to the density dependence of the nuclear symmetry energySensitivity of the neutron star r-mode instability window to the density depe…Super-soft symmetry energy encountering non-Newtonian gravity in neutron starsSuper-soft symmetry energy encountering non-Newtonian gravity in neutron…Towards Understanding Astrophysical Effects of Nuclear Symmetry Energy2002200420062008201020122014201620182020202220240255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average200220042006200820102012201420162018202020222024020406080100