Publication data of Krasinski, Andrzej: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion19701980199020002010202005001000150020002500
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications197019801990200020102020030609012015002.557.51012.5
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion1970198019902000201020200510152025
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestSolutions of the Einstein Field Equations for a Rotating Perfect Fluid, Part 2 - Properties of the Flow-Stationary and Vortex-Homogeneous SolutionsSolutions of the Einstein Field Equations for a Rotating Perfect Fluid, Part 2 - P…On the thermodynamical interpretation of perfect fluid solutions of the Einstein equations with no symmetryOn the thermodynamical interpretation of perfect fluid solutions of the Einst…Geometry and topology of the quasi-plane Szekeres modelInhomogeneous cosmological modelsPhysical and geometrical interpretation of the epsilon <= 0 Szekeres modelsOn the Global Geometry of the Stephani UniverseAn introduction to general relativity and cosmologyAlternative methods of describing structure formation in the Lemaitre-Tolman modelAlternative methods of describing structure formation in the Lemaitre-Tolman…Redshift propagation equations in the $eta' eq 0$ Szekeres modelsImitating accelerated expansion of the Universe by matter inhomogeneities: Corrections of some misunderstandingsImitating accelerated expansion of the Universe by matter inhomogeneities: …More examples of structure formation in the Lemaitre-Tolman modelEllipsoidal Spacetimes, Sources for the Kerr MetricStructure formation in the Lemaitre-Tolman modelFormation of voids in the universe within the Lemaitre-Tolman modelFormation of a galaxy with a central black hole in the Lemaitre-Tolman modelYou can't get through Szekeres wormholes: Or, regularity, topology and causality in quasispherical Szekeres modelsYou can't get through Szekeres wormholes: Or, regularity, topology and caus…A (giant) void is not mandatory to explain away dark energy with a Lemaitre -- Tolman modelA (giant) void is not mandatory to explain away dark energy with a Lemaitre …Inhomogeneous cosmological models: Exact solutions and their applicationsThe Cosmological constant and the theory of elementary particles19701980199020002010202005001000150020002500
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Solutions of the Einstein Field Equations for a Rotating Perfect Fluid, Part 2 - Properties of the Flow-Stationary and Vortex-Homogeneous SolutionsSolutions of the Einstein Field Equations for a Rotating Perfect Fluid, Part 2 - P…On the thermodynamical interpretation of perfect fluid solutions of the Einstein equations with no symmetryOn the thermodynamical interpretation of perfect fluid solutions of the Einst…Geometry and topology of the quasi-plane Szekeres modelInhomogeneous cosmological modelsPhysical and geometrical interpretation of the epsilon <= 0 Szekeres modelsOn the Global Geometry of the Stephani UniverseAn introduction to general relativity and cosmologyAlternative methods of describing structure formation in the Lemaitre-Tolman modelAlternative methods of describing structure formation in the Lemaitre-Tolman…Redshift propagation equations in the $eta' eq 0$ Szekeres modelsImitating accelerated expansion of the Universe by matter inhomogeneities: Corrections of some misunderstandingsImitating accelerated expansion of the Universe by matter inhomogeneities: …More examples of structure formation in the Lemaitre-Tolman modelEllipsoidal Spacetimes, Sources for the Kerr MetricStructure formation in the Lemaitre-Tolman modelFormation of voids in the universe within the Lemaitre-Tolman modelFormation of a galaxy with a central black hole in the Lemaitre-Tolman modelYou can't get through Szekeres wormholes: Or, regularity, topology and causality in quasispherical Szekeres modelsYou can't get through Szekeres wormholes: Or, regularity, topology and caus…A (giant) void is not mandatory to explain away dark energy with a Lemaitre -- Tolman modelA (giant) void is not mandatory to explain away dark energy with a Lemaitre …Inhomogeneous cosmological models: Exact solutions and their applicationsThe Cosmological constant and the theory of elementary particles1970198019902000201020200255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average1970198019902000201020200255075100125150175