Publication data of Martinez-Pinedo, Gabriel: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion1995200020052010201520202025025005000750010000125001500017500
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications1995200020052010201520202025080160240320400048121620
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion1995200020052010201520202025010203040506070
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestShell model calculations of stellar weak interaction rates. 1. Gamow-Teller distributions and spectra of nuclei in the mass range A = 45 - 65Shell model calculations of stellar weak interaction rates. 1. Gamow-Teller dist…The consequences of nuclear electron capture in core collapse supernovaeNeutrino nucleosynthesisCharged-current weak interaction processes in hot and dense matter and its impact on the spectra of neutrinos emitted from proto-neutron star coolingCharged-current weak interaction processes in hot and dense matter and its …RATE TABLES FOR THE WEAK PROCESSES OF pf -SHELL NUCLEI IN STELLAR ENVIRONMENTSRATE TABLES FOR THE WEAK PROCESSES OF pf -SHELL NUCLEI IN STELLAR …Full pf shell model study of A=48 nucleiLarge-scale evaluation of β-decay rates of r-process nuclei with the inclusion of first-forbidden transitionsLarge-scale evaluation of β-decay rates of r-process nuclei with the inclusion …Electron capture rates on nuclei and implications for stellar core collapseImproved axion emissivity from a supernova via nucleon-nucleon bremsstrahlungImproved axion emissivity from a supernova via nucleon-nucleon bremsstrah…Effective $g_A$ in the pf shellRadioactivity and thermalization in the ejecta of compact object mergers and their impact on kilonova light curvesRadioactivity and thermalization in the ejecta of compact object mergers and…Neutrino-induced nucleosynthesis of a>64 nuclei: the nu p-processNuclear Weak Interaction Processes in StarsShell model calculations of stellar weak interaction rates: 2.. Weak rates for nuclei in the mass range A = 45-65 in supernovae environmentShell model calculations of stellar weak interaction rates: 2.. Weak rates for n…Origin of the heaviest elements: The rapid neutron-capture processEnergy density functional study of nuclear matrix elements for neutrinoless $etaeta$ decayEnergy density functional study of nuclear matrix elements for neutrinoless …Theory of Core-Collapse SupernovaeElectromagnetic Counterparts of Compact Object Mergers Powered by the Radioactive Decay of R-process NucleiElectromagnetic Counterparts of Compact Object Mergers Powered by the Ra…The Shell Model as Unified View of Nuclear Structure1995200020052010201520202025025005000750010000125001500017500
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Shell model calculations of stellar weak interaction rates. 1. Gamow-Teller distributions and spectra of nuclei in the mass range A = 45 - 65Shell model calculations of stellar weak interaction rates. 1. Gamow-Teller dist…The consequences of nuclear electron capture in core collapse supernovaeNeutrino nucleosynthesisCharged-current weak interaction processes in hot and dense matter and its impact on the spectra of neutrinos emitted from proto-neutron star coolingCharged-current weak interaction processes in hot and dense matter and its …RATE TABLES FOR THE WEAK PROCESSES OF pf -SHELL NUCLEI IN STELLAR ENVIRONMENTSRATE TABLES FOR THE WEAK PROCESSES OF pf -SHELL NUCLEI IN STELLAR …Full pf shell model study of A=48 nucleiLarge-scale evaluation of β-decay rates of r-process nuclei with the inclusion of first-forbidden transitionsLarge-scale evaluation of β-decay rates of r-process nuclei with the inclusion …Electron capture rates on nuclei and implications for stellar core collapseImproved axion emissivity from a supernova via nucleon-nucleon bremsstrahlungImproved axion emissivity from a supernova via nucleon-nucleon bremsstrah…Effective $g_A$ in the pf shellRadioactivity and thermalization in the ejecta of compact object mergers and their impact on kilonova light curvesRadioactivity and thermalization in the ejecta of compact object mergers and…Neutrino-induced nucleosynthesis of a>64 nuclei: the nu p-processNuclear Weak Interaction Processes in StarsShell model calculations of stellar weak interaction rates: 2.. Weak rates for nuclei in the mass range A = 45-65 in supernovae environmentShell model calculations of stellar weak interaction rates: 2.. Weak rates for n…Origin of the heaviest elements: The rapid neutron-capture processEnergy density functional study of nuclear matrix elements for neutrinoless $etaeta$ decayEnergy density functional study of nuclear matrix elements for neutrinoless …Theory of Core-Collapse SupernovaeElectromagnetic Counterparts of Compact Object Mergers Powered by the Radioactive Decay of R-process NucleiElectromagnetic Counterparts of Compact Object Mergers Powered by the Ra…The Shell Model as Unified View of Nuclear Structure19952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average199520002005201020152020202502505007501000125015001750