Publication data of Bi, Xiao-Jun: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion2000200520102015202020250100020003000400050006000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications200020052010201520202025050100150200250048121620
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Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestConstraints on the dark matter annihilation scenario of Fermi 130 GeV $gamma$-ray line emission by continuous gamma-rays, Milky Way halo, galaxy clusters and dwarf galaxies observationsConstraints on the dark matter annihilation scenario of Fermi 130 GeV $gam…Thermal leptogenesis in a model with mass varying neutrinosOn the e+ e- excesses and the knee of the cosmic ray spectra - hints of cosmic rays acceleration in young supernova remnantsOn the e+ e- excesses and the knee of the cosmic ray spectra - hints of cos…Cosmological evolution of interacting dark energy models with mass varying neutrinosCosmological evolution of interacting dark energy models with mass varying …Limits on axion-like particles from Mrk 421 with 4.5-year period observations by ARGO-YBJ and Fermi-LATLimits on axion-like particles from Mrk 421 with 4.5-year period observations …A Promising Interpretation of Diphoton Resonance at 750 GeVConstraining the interaction strength between dark matter and visible matter: II. scalar, vector and spin-3/2 dark matterConstraining the interaction strength between dark matter and visible matte…Constraints and tests of the OPERA superluminal neutrinosQuantitative study of the AMS-02 electron/positron spectra: Implications for pulsars and dark matter propertiesQuantitative study of the AMS-02 electron/positron spectra: Implications for …Two-zone diffusion of electrons and positrons from Geminga explains the positron anomalyTwo-zone diffusion of electrons and positrons from Geminga explains the posi…Parameters in a class of leptophilic models from PAMELA, ATIC and FERMIImplications of the AMS-02 positron fraction in cosmic raysConstraining the interaction strength between dark matter and visible matter: I. fermionic dark matterConstraining the interaction strength between dark matter and visible matte…Propagation of cosmic rays in the AMS-02 eraPulsar interpretation for the AMS-02 resultDiscriminating different scenarios to account for the cosmic e + /- excess by synchrotron and inverse Compton radiationDiscriminating different scenarios to account for the cosmic e + /- excess by …The 750 GeV diphoton excess at the LHC and dark matter constraintsFull Calculation of Clumpiness Boost factors for Antimatter Cosmic Rays in the light of Lambda-CDM N-body simulation results. Abandoning hope in clumpiness enhancement?Full Calculation of Clumpiness Boost factors for Antimatter Cosmic Rays in the…PAMELA data and leptonically decaying dark matter200020052010201520202025010002000300040005000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Constraints on the dark matter annihilation scenario of Fermi 130 GeV $gamma$-ray line emission by continuous gamma-rays, Milky Way halo, galaxy clusters and dwarf galaxies observationsConstraints on the dark matter annihilation scenario of Fermi 130 GeV $gam…Thermal leptogenesis in a model with mass varying neutrinosOn the e+ e- excesses and the knee of the cosmic ray spectra - hints of cosmic rays acceleration in young supernova remnantsOn the e+ e- excesses and the knee of the cosmic ray spectra - hints of cos…Cosmological evolution of interacting dark energy models with mass varying neutrinosCosmological evolution of interacting dark energy models with mass varying …Limits on axion-like particles from Mrk 421 with 4.5-year period observations by ARGO-YBJ and Fermi-LATLimits on axion-like particles from Mrk 421 with 4.5-year period observations …A Promising Interpretation of Diphoton Resonance at 750 GeVConstraining the interaction strength between dark matter and visible matter: II. scalar, vector and spin-3/2 dark matterConstraining the interaction strength between dark matter and visible matte…Constraints and tests of the OPERA superluminal neutrinosQuantitative study of the AMS-02 electron/positron spectra: Implications for pulsars and dark matter propertiesQuantitative study of the AMS-02 electron/positron spectra: Implications for …Two-zone diffusion of electrons and positrons from Geminga explains the positron anomalyTwo-zone diffusion of electrons and positrons from Geminga explains the posi…Parameters in a class of leptophilic models from PAMELA, ATIC and FERMIImplications of the AMS-02 positron fraction in cosmic raysConstraining the interaction strength between dark matter and visible matter: I. fermionic dark matterConstraining the interaction strength between dark matter and visible matte…Propagation of cosmic rays in the AMS-02 eraPulsar interpretation for the AMS-02 resultDiscriminating different scenarios to account for the cosmic e + /- excess by synchrotron and inverse Compton radiationDiscriminating different scenarios to account for the cosmic e + /- excess by …The 750 GeV diphoton excess at the LHC and dark matter constraintsFull Calculation of Clumpiness Boost factors for Antimatter Cosmic Rays in the light of Lambda-CDM N-body simulation results. Abandoning hope in clumpiness enhancement?Full Calculation of Clumpiness Boost factors for Antimatter Cosmic Rays in the…PAMELA data and leptonically decaying dark matter2000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average2000200520102015202020250100200300400500