Publication data of Ellis, Paul J.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion197019801990200020102020010002000300040005000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications19701980199020002010202002550751001250246810
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion19701980199020002010202005101520253035
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestCoulomb and nuclear inelastic excitations and the optical potential for heavy ionsCoulomb and nuclear inelastic excitations and the optical potential for heavy …Investigation of the (d52) 2 and (d52s12) two-particle configurations in O-18 using the O-17 (d, p) O-18 reaction at 18 MeVInvestigation of the (d52) 2 and (d52s12) two-particle configurations in O-1…Low-energy theorems for gluodynamics at finite temperatureDileptons and photons from coarse grained microscopic dynamics and hydrodynamics compared to experimental dataDileptons and photons from coarse grained microscopic dynamics and hydro…An Effective Lagrangian with broken scale and chiral symmetry: 2. Pion phenomenologyAn Effective Lagrangian with broken scale and chiral symmetry: 2. Pion phen…Thermal conductivity of dense quark matter and cooling of starsRedundance of Delta isobar parameters in effective field theoriesRole of fluctuations in the linear sigma model with quarksThe weak coupling model applied to the nuclei with A = 16–19An Effective Lagrangian with broken scale and chiral symmetry applied to nuclear matter and finite nucleiAn Effective Lagrangian with broken scale and chiral symmetry applied to nu…Properties of rho and omega mesons at finite temperature and density as inferred from experimentProperties of rho and omega mesons at finite temperature and density as inf…Kaon condensation in neutron star matter with hyperonsKaon condensation in proto neutron star matterAn introductory guide to effective operators in nucleiThe weak coupling model applied to the nuclei with A = 16–19Pion nucleon scattering in a new approach to chiral perturbation theoryStrangeness in hadronic stellar matterComposition and structure of protoneutron starsIsospin asymmetry in nuclei and neutron stars197019801990200020102020010002000300040005000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Coulomb and nuclear inelastic excitations and the optical potential for heavy ionsCoulomb and nuclear inelastic excitations and the optical potential for heavy …Investigation of the (d52) 2 and (d52s12) two-particle configurations in O-18 using the O-17 (d, p) O-18 reaction at 18 MeVInvestigation of the (d52) 2 and (d52s12) two-particle configurations in O-1…Low-energy theorems for gluodynamics at finite temperatureDileptons and photons from coarse grained microscopic dynamics and hydrodynamics compared to experimental dataDileptons and photons from coarse grained microscopic dynamics and hydro…An Effective Lagrangian with broken scale and chiral symmetry: 2. Pion phenomenologyAn Effective Lagrangian with broken scale and chiral symmetry: 2. Pion phen…Thermal conductivity of dense quark matter and cooling of starsRedundance of Delta isobar parameters in effective field theoriesRole of fluctuations in the linear sigma model with quarksThe weak coupling model applied to the nuclei with A = 16–19An Effective Lagrangian with broken scale and chiral symmetry applied to nuclear matter and finite nucleiAn Effective Lagrangian with broken scale and chiral symmetry applied to nu…Properties of rho and omega mesons at finite temperature and density as inferred from experimentProperties of rho and omega mesons at finite temperature and density as inf…Kaon condensation in neutron star matter with hyperonsKaon condensation in proto neutron star matterAn introductory guide to effective operators in nucleiThe weak coupling model applied to the nuclei with A = 16–19Pion nucleon scattering in a new approach to chiral perturbation theoryStrangeness in hadronic stellar matterComposition and structure of protoneutron starsIsospin asymmetry in nuclei and neutron stars1970198019902000201020200255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average197019801990200020102020050100150200