Publication data of Nilsson, Ulf S.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion19952000200520102015202020250100200300400500
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications199520002005201020152020202504812162001.534.567.5
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion199520002005201020152020202502468101214
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersA Field theory for partially polarized quantum Hall statesStationary Bianchi type II perfect fluid modelsA Dynamical systems approach to geodesics in Bianchi cosmologiesIsotropization of two component fluidsSpatially selfsimilar locally rotationally symmetric perfect fluid modelsAnisotropic universes with isotropic cosmic microwave background radiation: Letter to the editorAnisotropic universes with isotropic cosmic microwave background radiation:…Nontilted Bianchi VII(0) models: The Radiation fluidDynamics of M theory cosmologyAn Almost isotropic cosmic microwave temperature does not imply an almost isotropic universeAn Almost isotropic cosmic microwave temperature does not imply an almost…Critical phenomena and a new class of selfsimilar spherically symmetric perfect fluid solutionsCritical phenomena and a new class of selfsimilar spherically symmetric perfe…Timelike selfsimilar spherically symmetric perfect fluid modelsSpatially selfsimilar spherically symmetric perfect fluid modelsGeneral relativistic stars: Linear equations of statePhysical interpretation of selfsimilar spherically symmetric perfect fluid models: Combining the comoving and homothetic approachPhysical interpretation of selfsimilar spherically symmetric perfect fluid mode…General relativistic stars: Polytropic equations of state19952000200520102015202020250100200300400500
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)A Field theory for partially polarized quantum Hall statesStationary Bianchi type II perfect fluid modelsA Dynamical systems approach to geodesics in Bianchi cosmologiesIsotropization of two component fluidsSpatially selfsimilar locally rotationally symmetric perfect fluid modelsAnisotropic universes with isotropic cosmic microwave background radiation: Letter to the editorAnisotropic universes with isotropic cosmic microwave background radiation:…Nontilted Bianchi VII(0) models: The Radiation fluidDynamics of M theory cosmologyAn Almost isotropic cosmic microwave temperature does not imply an almost isotropic universeAn Almost isotropic cosmic microwave temperature does not imply an almost…Critical phenomena and a new class of selfsimilar spherically symmetric perfect fluid solutionsCritical phenomena and a new class of selfsimilar spherically symmetric perfe…Timelike selfsimilar spherically symmetric perfect fluid modelsSpatially selfsimilar spherically symmetric perfect fluid modelsGeneral relativistic stars: Linear equations of statePhysical interpretation of selfsimilar spherically symmetric perfect fluid models: Combining the comoving and homothetic approachPhysical interpretation of selfsimilar spherically symmetric perfect fluid mode…General relativistic stars: Polytropic equations of state19952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average1995200020052010201520202025010203040