Publication data of Rigopoulos, Gerasimos I.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion2010202020052015202505001000150020002500
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications201020202005201520250122436486001.22.43.64.86
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion200220042006200820102012201420162018202020222024051015202530
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestFunctional renormalization group for stochastic inflationSupernovae data and perturbative deviation from homogeneityOn second order gauge invariant perturbations in multi-field inflationary modelsOn second order gauge invariant perturbations in multi-field inflationary mo…Parametric Decay of the CurvatonInflation is always semi-classical: diffusion domination overproduces Primordial Black HolesInflation is always semi-classical: diffusion domination overproduces Primordi…Path Integral for Inflationary PerturbationsEffective long wavelength scalar dynamics in de SitterDecoherence from Isocurvature perturbations in InflationSelf Regulation of Infrared Correlations for Massless Scalar Fields during InflationSelf Regulation of Infrared Correlations for Massless Scalar Fields during Inflati…The Subdominant CurvatonA Simple route to non-Gaussianity in inflationFeynman Diagrams for Stochastic Inflation and Quantum Field Theory in de Sitter SpaceFeynman Diagrams for Stochastic Inflation and Quantum Field Theory in de S…Non-linear inflationary perturbationsInfrared correlations in de Sitter space: Field theoretic versus stochastic approachInfrared correlations in de Sitter space: Field theoretic versus stochastic appr…Quantitative bispectra from multifield inflationOn the divergences of inflationary superhorizon perturbationsNon-linear perturbations in multiple-field inflationLarge non-Gaussianity in multiple-field inflationThe separate universe approach and the evolution of nonlinear superhorizon cosmological perturbationsThe separate universe approach and the evolution of nonlinear superhorizon …2010202020052015202505001000150020002500
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Functional renormalization group for stochastic inflationSupernovae data and perturbative deviation from homogeneityOn second order gauge invariant perturbations in multi-field inflationary modelsOn second order gauge invariant perturbations in multi-field inflationary mo…Parametric Decay of the CurvatonInflation is always semi-classical: diffusion domination overproduces Primordial Black HolesInflation is always semi-classical: diffusion domination overproduces Primordi…Path Integral for Inflationary PerturbationsEffective long wavelength scalar dynamics in de SitterDecoherence from Isocurvature perturbations in InflationSelf Regulation of Infrared Correlations for Massless Scalar Fields during InflationSelf Regulation of Infrared Correlations for Massless Scalar Fields during Inflati…The Subdominant CurvatonA Simple route to non-Gaussianity in inflationFeynman Diagrams for Stochastic Inflation and Quantum Field Theory in de Sitter SpaceFeynman Diagrams for Stochastic Inflation and Quantum Field Theory in de S…Non-linear inflationary perturbationsInfrared correlations in de Sitter space: Field theoretic versus stochastic approachInfrared correlations in de Sitter space: Field theoretic versus stochastic appr…Quantitative bispectra from multifield inflationOn the divergences of inflationary superhorizon perturbationsNon-linear perturbations in multiple-field inflationLarge non-Gaussianity in multiple-field inflationThe separate universe approach and the evolution of nonlinear superhorizon cosmological perturbationsThe separate universe approach and the evolution of nonlinear superhorizon …2002200420062008201020122014201620182020202220240255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average200220042006200820102012201420162018202020222024050100150200