Professor at Prague
Becomes professor of theoretical physics at the German University in Prague.
Follow Albert Einstein through 240 dated historical records for United States of America.
A chronological timeline drawn from matching World History Database records.
Becomes professor of theoretical physics at the German University in Prague.
Begins work as professor of theoretical physics at ETH Zurich.
Collaborates closely with Marcel Grossmann, who guides him toward Ricci and Levi-Civita tensor calculus as the mathematical language for gravitation.
Develops field equations for a restricted static gravitational problem while searching for a theory that can extend relativity beyond inertial reference frames.
Works with Marcel Grossmann to master tensor calculus for a relativistic theory of gravitation.
Realises that gravitation may require non-Euclidean geometry, redirecting the search for a relativistic gravity theory toward curved spacetime mathematics.
Explores a formulation in which the coordinate speed of light varies with gravitational potential, an intermediate step toward a geometric theory of gravity.
Fills the Zurich Notebook with tensor calculations while testing candidate gravitational field equations and learning the differential geometry needed for a covariant theory.
Uses the Zurich Notebook to explore candidate gravitational field equations and differential geometry.
Encourages astronomical testing of gravitational light deflection during a solar eclipse.
Works with Michele Besso on applying the developing gravitational theory to Mercury's orbit, creating calculations that later help solve the perihelion anomaly.
Collaborates closely with Marcel Grossmann on the mathematical framework of gravitation.
Publishes the Entwurf gravitational theory with Marcel Grossmann as an intermediate step toward general relativity.
Moves to Berlin for a senior research appointment and membership of the Prussian Academy of Sciences.
Publishes work refining the mathematical and covariance problems of his developing gravitational theory.
Continues with Grossmann to examine covariance properties of their gravitational equations, exposing problems that eventually drive Einstein back toward general covariance.
Publishes a detailed formal treatment of the developing gravitational theory, presenting its mathematical structure before he restores fully general covariance.
Co-signs a pacifist appeal opposing wartime nationalism among European intellectuals.
With Adriaan Fokker, reformulates Nordstrom's competing gravitation theory using tensor methods, clarifying how relativistic gravity could be expressed geometrically.
Lectures in Gottingen on his gravitational theory, presenting the unfinished framework to leading mathematicians while he approaches the final generally covariant equations.
Presents revised gravitational field equations to the Prussian Academy during his final push toward general relativity.
Presents improved gravitational equations to the Prussian Academy and moves substantially closer to the generally covariant form completed later that month.
Presents another formulation of gravitation using a restricted coordinate condition with unit determinant.
Explains Mercury's anomalous perihelion advance using the emerging general theory of relativity.
Presents the final generally covariant gravitational field equations to the Prussian Academy, completing the mathematical core of general relativity.
Presents the final generally covariant gravitational field equations to the Prussian Academy.
Using the completed theory, obtains the full gravitational deflection predicted for starlight grazing the Sun, approximately twice his earlier 1911 estimate.
Elected a corresponding member of the Royal Society of Sciences at Göttingen.
Publishes experimental work with Wander de Haas linking magnetism to angular momentum.
Lectures on gravitation in Göttingen, stimulating intense discussion with leading mathematicians.
Communicates Karl Schwarzschild's exact solution of the new field equations to the Prussian Academy, demonstrating that general relativity admits important exact solutions.
Predicts gravitational waves as propagating disturbances in spacetime within general relativity.
Publishes his popular introduction to special and general relativity.
Develops the treatment of energy and momentum in the gravitational field, addressing how conservation laws operate within the generally covariant theory.
Publishes a systematic presentation of the general theory of relativity and its field equations.
Serves as president of the German Physical Society during the consolidation of general relativity.
Formulates general relativity using Hamilton's variational principle, providing a compact mathematical route to the gravitational field equations and their conservation properties.
Responds to Friedrich Kottler's criticism of the equivalence hypothesis, defending the conceptual basis on which his route from special to general relativity depended.
Develops a quantum theory of radiation introducing transition probabilities later represented by Einstein coefficients.
Einstein adds the cosmological constant to his gravitational field equations to permit a static universe, creating the mathematical term later associated with dark energy.
These dates and descriptions come from the historical_events database. Exact duplicate records have been collapsed. Names are grouped by the country, Name 2 and Name 1 fields; records with missing Name 2 cannot be reliably assigned to an individual biography. Check the underlying sources before formal citation.