Laureates

“For his groundbreaking contributions to the scientific definition of the most sensitive radio telescope and his numerous innovations in characterizing the dynamic universe, resulting in precise measurements of the interstellar magnetic field and advancing the field of fast radio bursts into a high-statistics era.”

“For his pioneering and groundbreaking theoretical and numerical simulation contributions that have advanced our understanding of supernovae, gamma-ray bursts, and binary stellar evolution connecting them.”

“For the innovative detection and comprehensive analysis of a large population of fast radio bursts, significantly increasing their statistics, including repeating sources, which have boosted our understanding of their origin and their application in mapping the universe structure and composition.”

“For his many lasting contributions to the foundation of mathematical physics including the dynamics of relativistic gravitational fields.”

“For his persistent devotion to the study of the quantum field theory boundary conditions at the black hole horizon.”

“For extending Relativistic astrophysics across international frontiers, a true companion in the search for the deeper meaning of Einstein's great theory.”

“For unwavering support for the MG meetings since their inception, a true companion in the search for the deeper meaning of Einstein's great theory.”

“For the creation of the world's best X-ray map of the entire sky as part of the SRG/eROSITA scientific program.”

“For the creation of the world's best X-ray map of the entire sky as part of the SRG/eROSITA scientific program.”

“For the creation of the world's best X-ray map of the entire sky as part of the SRG/eROSITA scientific program.”

“For his collaboration with David Wilkinson in realizing the NASA Explorer WMAP mission and as founding director of the Atacama Cosmology Telescope.”

“For the development of theoretical tools in the scrutinising, through the CMB, of the first observable electromagnetic appearance of our Universe.”

“For the proof of the positivity of total mass in the theory of general relativity and perfecting as well the concept of quasi-local mass, for his proof of the Calabi conjecture, for his continuous inspiring role in the study of black holes physics.”

“For obtaining important constraints on inflation, primordial non-Gaussianity, CMB lensing, reionization, and Galactic dust and magnetic fields.”

“To HEPL for having developed interdepartmental activities at Stanford University at the frontier of fundamental physics, astrophysics and technology.”

“For heralding the role of binary systems in the evolution of massive stars.”

“For fostering Research in black holes, gravitational waves and cosmology.”

“For applying the mathematics of chaotic systems to physics and cosmology.”

“For pioneering the physics of hot neutron stars and their cooling.”

“For deepening Einstein's geometrical approach to physics in the best tradition of Paul Dirac and Hermann Weyl.”

“For his work on white dwarfs motivating Enrico Fermi's return to astrophysics and guiding the basic understanding of neutron star matter and fields.”

“For the tremendous success of its scientific space missions in astronomy, astrophysics, cosmology and fundamental physics.”

“For exploring the nuclear physics and yet unsolved problems of the endpoint of thermonuclear evolution of stars, leading to new avenues of research in physics and astrophysics.”

“For the discovery of a general solution of the Einstein equations with a cosmological singularity of an oscillatory chaotic character known as the BKL singularity.”

“For the discovery of a general solution of the Einstein equations with a cosmological singularity of an oscillatory chaotic character known as the BKL singularity.”

“For guiding the Gamma-ray Burst Monitor Project on board the BeppoSAX satellite, which led to the discovery of GRB X-ray afterglows, and to their optical identification.”

“For its innovative status as a joint institute established by Stockholm University and the Royal Institute of Technology and for fostering contributions to cosmology and astrophysics in the tradition established by Oskar Klein.”

“For pioneering contributions in the discovery of dark matter and cosmic web and fostering research in the historical Tartu Observatory.”

“For her fundamental contributions to the X-ray studies of galaxies and clusters tracing their formation and evolution and for her role in collaborations using clusters to study dark matter and in analyzing the effects of outbursts from supermassive black holes on the intracluster gas.”

“For his fundamental contributions to pulsar astrophysics, and notably for having first confirmed the existence of spin-orbit precession in binary pulsars.”

“For outstanding contributions to mathematics and theoretical physics, renewing basic geometrical concepts and developing new mathematical and physical aspects of spacetime.”

“For his fundamental contribution to Einstein's theory of general relativity: The gravitational field of a spinning mass as an example of algebraically special metrics.”

“For his committed support for the international development of relativistic astrophysics and for his dedication to fostering an enlightened relationship between science and religion.”

“For his outstanding scientific contributions to the physics of compact astrophysical objects and for leading the highly successful ROSAT mission which discovered more then 200,000 galactic and extragalactic X-ray sources.”

“For the successful endeavor of re-establishing freedom of thinking and teaching within a democratic society in the spirit of the Humboldt tradition.”

“For separate as well as joint work in establishing the mathematical framework for proving the existence and uniqueness of solutions to Einstein's gravitational field equations.”

“For separate as well as joint work in establishing the mathematical framework for proving the existence and uniqueness of solutions to Einstein's gravitational field equations.”

“For his contributions to science, epistimology, mathematics and physics from subnuclear to space sciences.”

“For its role as a teaching and research institution and as a place originating fundamental physics ideas in the exploration of the universe.”

“For promoting General Relativity and Mathematics research and inventing the summer school concept.”

“For promoting General Relativity and Mathematics research and inventing the summer school concept.”

“For opening, five successive times, new highways for exploring the Universe.”

“For extending the mathematical and geometrical foundations of General Relativity.”

“For identifying and recording in discussions by the protagonists the crucial developments of physics and astrophysics in the twentieth century.”

“For his contributions to the interface between mathematics and physics leading to new fields of research of paramount importance in relativisic astrophysics and particle physics.”

“For leading the development of extremely precise space experiments utilizing superconducting technology to test General Relativity and the Equivalence Principle.”

“For its role as a cradle of Science and Humanities and for hosting the manuscripts of Albert Einstein.”

“For his contributions to the analysis of gravitational phenomena from Newton to Einstein and especially for leading the way to relativistic astrophysics with the concept of critical mass for gravitational collapse.”

“For having built on his experience in nuclear physics, thermonuclear reactions, and extensive numerical simulation to create a new testing ground for the novel concepts of relativistic astrophysics.”

“For its critical role in the direction and operation of the Hubble Space Telescope, a unique international laboratory for modern astrophysics and cosmology.”

“For participating in the pioneering work of the early sixties in X-ray astronomy and for his subsequent molding of an agile and diversified Japanese scientific space program investigating the deepest aspects of relativistic astrophysics.”

“For his contributions to the understanding of spacetime singularities and of the large scale structure of the Universe and of its quantum origins.”

“For keeping alive first in Hiroshima and then in Kyoto research in relativity, cosmology, and relativistic field theory and the development of a school of international acclaim.”

“For his contributions to research in gamma, X-ray and infrared radiation as well as cosmic rays.”

“For his contributions to geometrodynamics and Einstein's visions.”

“For its contributions to relativistic astrophysics.”

“For his work in gravitation and low temperature physics.”

“For his work in unifying fundamental interactions.”

“For its contributions to the origin and development of astrophysics.”