Publication data of Fuller, George M.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion19801985199019952000200520102015202020250250050007500100001250015000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications1980199020002010202005010015020025003691215
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion1980198519901995200020052010201520202025020406080
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestNeutrino Quantum KineticsAnalysis of Collective Neutrino Flavor Transformation in SupernovaePulsar kicks from a dark-matter sterile neutrinoCoherent Development of Neutrino Flavor in the Supernova EnvironmentThe Quark - hadron phase transition and primordial nucleosynthesisCosmological and Astrophysical Neutrino Mass MeasurementsNeutrino-neutrino scattering and matter enhanced neutrino flavor transformation in SupernovaeNeutrino-neutrino scattering and matter enhanced neutrino flavor transform…The Quark - Hadron Phase Transition in the Early Universe: Isothermal Baryon Number Fluctuations and Primordial NucleosynthesisThe Quark - Hadron Phase Transition in the Early Universe: Isothermal Baryon…The extremely metal - poor, neutron - capture - rich star CS 22892-052: A Comprehensive abundance analysisThe extremely metal - poor, neutron - capture - rich star CS 22892-052: A Co…A Connection between flavor mixing of cosmologically significant neutrinos and heavy element nucleosynthesis in supernovaeA Connection between flavor mixing of cosmologically significant neutrinos a…Collective neutrino flavor transformation in supernovaeStellar Weak Interaction Rates for Intermediate Mass Nuclei.. 3. Rate Tables for the Free Nucleons and a = 21 to a = 60Stellar Weak Interaction Rates for Intermediate Mass Nuclei.. 3. Rate Tables fo…Stellar Weak Interaction Rates for Intermediate Mass Nuclei. 2. A = 21 to A = 60Stellar Weak Interaction Rates for Intermediate Mass Nuclei. 2. A = 21 to A =…Direct detection of warm dark matter in the X-rayStellar weak interaction rates for intermediate-mass nuclei. IV - Interpolation procedures for rapidly varying lepton capture rates using effective log (ft)-valuesStellar weak interaction rates for intermediate-mass nuclei. IV - Interpolation …Simulation of Coherent Non-Linear Neutrino Flavor Transformation in the Supernova Environment. 1. Correlated Neutrino TrajectoriesSimulation of Coherent Non-Linear Neutrino Flavor Transformation in the Sup…Collective Neutrino OscillationsSterile neutrino hot, warm, and cold dark matterA New dark matter candidate: Nonthermal sterile neutrinos19801985199019952000200520102015202020250250050007500100001250015000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Neutrino Quantum KineticsAnalysis of Collective Neutrino Flavor Transformation in SupernovaePulsar kicks from a dark-matter sterile neutrinoCoherent Development of Neutrino Flavor in the Supernova EnvironmentThe Quark - hadron phase transition and primordial nucleosynthesisCosmological and Astrophysical Neutrino Mass MeasurementsNeutrino-neutrino scattering and matter enhanced neutrino flavor transformation in SupernovaeNeutrino-neutrino scattering and matter enhanced neutrino flavor transform…The Quark - Hadron Phase Transition in the Early Universe: Isothermal Baryon Number Fluctuations and Primordial NucleosynthesisThe Quark - Hadron Phase Transition in the Early Universe: Isothermal Baryon…The extremely metal - poor, neutron - capture - rich star CS 22892-052: A Comprehensive abundance analysisThe extremely metal - poor, neutron - capture - rich star CS 22892-052: A Co…A Connection between flavor mixing of cosmologically significant neutrinos and heavy element nucleosynthesis in supernovaeA Connection between flavor mixing of cosmologically significant neutrinos a…Collective neutrino flavor transformation in supernovaeStellar Weak Interaction Rates for Intermediate Mass Nuclei.. 3. Rate Tables for the Free Nucleons and a = 21 to a = 60Stellar Weak Interaction Rates for Intermediate Mass Nuclei.. 3. Rate Tables fo…Stellar Weak Interaction Rates for Intermediate Mass Nuclei. 2. A = 21 to A = 60Stellar Weak Interaction Rates for Intermediate Mass Nuclei. 2. A = 21 to A =…Direct detection of warm dark matter in the X-rayStellar weak interaction rates for intermediate-mass nuclei. IV - Interpolation procedures for rapidly varying lepton capture rates using effective log (ft)-valuesStellar weak interaction rates for intermediate-mass nuclei. IV - Interpolation …Simulation of Coherent Non-Linear Neutrino Flavor Transformation in the Supernova Environment. 1. Correlated Neutrino TrajectoriesSimulation of Coherent Non-Linear Neutrino Flavor Transformation in the Sup…Collective Neutrino OscillationsSterile neutrino hot, warm, and cold dark matterA New dark matter candidate: Nonthermal sterile neutrinos19801985199019952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average198019851990199520002005201020152020202502004006008001000