Publication data of Langanke, Karlheinz: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion198019902000201020200250050007500100001250015000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications19801990200020102020080160240320400048121620
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion197519801985199019952000200520102015202020250102030405060
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestShell-model half-lives including first-forbidden contributions for r-process waiting-point nucleiShell-model half-lives including first-forbidden contributions for r-process wait…The Role of neutrino induced reactions on lead and iron in neutrino detectorsPresupernova evolution with improved rates for weak interactionsSignal for supernova muon-neutrino and tau-neutrino neutrinos in water Cherenkov detectorsSignal for supernova muon-neutrino and tau-neutrino neutrinos in water Che…The Role of Fission in Neutron Star Mergers and its Impact on the r-Process PeaksThe Role of Fission in Neutron Star Mergers and its Impact on the r-Process Pe…Nuclear robustness of the r process in neutron-star mergersComposition of the innermost supernova ejectaNeutrino nucleus reactions and nuclear structureShell 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 nucleosynthesisRATE TABLES FOR THE WEAK PROCESSES OF pf -SHELL NUCLEI IN STELLAR ENVIRONMENTSRATE TABLES FOR THE WEAK PROCESSES OF pf -SHELL NUCLEI IN STELLAR …Electron capture rates on nuclei and implications for stellar core collapseShell model Monte Carlo methodsNeutrino-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 processTheory of Core-Collapse Supernovae198019902000201020200250050007500100001250015000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Shell-model half-lives including first-forbidden contributions for r-process waiting-point nucleiShell-model half-lives including first-forbidden contributions for r-process wait…The Role of neutrino induced reactions on lead and iron in neutrino detectorsPresupernova evolution with improved rates for weak interactionsSignal for supernova muon-neutrino and tau-neutrino neutrinos in water Cherenkov detectorsSignal for supernova muon-neutrino and tau-neutrino neutrinos in water Che…The Role of Fission in Neutron Star Mergers and its Impact on the r-Process PeaksThe Role of Fission in Neutron Star Mergers and its Impact on the r-Process Pe…Nuclear robustness of the r process in neutron-star mergersComposition of the innermost supernova ejectaNeutrino nucleus reactions and nuclear structureShell 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 nucleosynthesisRATE TABLES FOR THE WEAK PROCESSES OF pf -SHELL NUCLEI IN STELLAR ENVIRONMENTSRATE TABLES FOR THE WEAK PROCESSES OF pf -SHELL NUCLEI IN STELLAR …Electron capture rates on nuclei and implications for stellar core collapseShell model Monte Carlo methodsNeutrino-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 processTheory of Core-Collapse Supernovae197519801985199019952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average1980199020002010202002004006008001000