Unified Field Theory Publication
Publishes a widely publicized unified-field theory based on teleparallel geometry.
Follow Albert Einstein through 240 dated historical records for United States of America.
A chronological timeline drawn from matching World History Database records.
Publishes a widely publicized unified-field theory based on teleparallel geometry.
Publishes a unified field formulation based on distant parallelism and Hamilton's principle, continuing his search for equations joining gravitational and electromagnetic fields.
Receives an honorary Doctor of Science degree from ETH Zurich.
Begins an extended visit to Caltech where relativity, cosmology and unified-field questions form an important part of his discussions with American physicists and astronomers.
Publishes work with Walther Mayer giving exact static solutions of unified-field equations, testing whether the programme can represent physically meaningful configurations.
Begins an extended academic visit to the California Institute of Technology.
Further develops spaces combining a Riemann metric with distant parallelism, refining the geometric machinery behind his teleparallel unified-field theory.
Attends the sixth Solvay Conference and continues discussions on quantum theory and field physics.
Examines the compatibility of equations in the unified-field programme, addressing mathematical consistency before the theory can be regarded as physically viable.
Visits Mount Wilson and discusses observational cosmology, confronting evidence that distant galaxies exhibit the redshift-distance relation associated with cosmic expansion.
Receives an honorary Doctor of Science degree from the University of Oxford.
Adopts an expanding cosmological model and abandons the need for his earlier static-universe construction.
Publishes a non-static cosmological model within general relativity, accepting cosmic expansion and dispensing with the static balance that motivated his cosmological constant.
Receives the Prix Jules Janssen for distinguished work in astronomy and astrophysics.
Einstein abandons the need for a static cosmological model after cosmic expansion becomes established, leaving the cosmological constant without its original motivation.
Abandons his earlier static cosmological model as expanding-universe observations and relativistic cosmology make a dynamical universe the more credible interpretation.
Gives three Rhodes Memorial Lectures on relativity, cosmology and his latest work in theoretical physics.
Becomes a member of the German Academy of Natural Scientists Leopoldina.
With Willem de Sitter, proposes a spatially flat expanding cosmological model without a cosmological constant, providing a simple benchmark solution of general relativity.
With Willem de Sitter, proposes a simple expanding cosmological model with zero cosmological constant.
Accepts appointment to the newly founded Institute for Advanced Study.
Publishes another unified theory of gravitation and electricity, continuing to test alternative geometrical structures beyond the standard equations of general relativity.
Resigns from the Prussian Academy of Sciences after deciding not to return to Nazi Germany.
Lectures in Glasgow on the origins and development of general relativity, recounting the physical ideas that led from equivalence to curved spacetime.
Lectures at Oxford on the methods and foundations of theoretical physics.
Settles in the United States after the Nazi rise to power and joins the Institute for Advanced Study.
Renounces German citizenship after the Nazi seizure of power while retaining Swiss citizenship.
Delivers the Gibbs Lecture on an elementary proof of the equivalence of mass and energy.
Publishes reflections on how fundamental theoretical physics develops from principles and mathematical structure.
Einstein, Podolsky and Rosen publish their argument that quantum mechanics may not provide a complete description of physical reality.
Receives the Franklin Medal in recognition of his work in relativity and the photoelectric effect.
The Einstein-Rosen construction joined two copies of a spacetime solution through a geometric bridge, creating an early mathematical example of what later literature called a wormhole.
Einstein and Nathan Rosen constructed a bridge geometry from solutions of the gravitational field equations while exploring whether particles could be represented without ordinary singularities.
With Nathan Rosen, studies bridge solutions in general relativity connecting two sheets of spacetime.
Files a declaration of intention to become a citizen of the United States.
Publishes a calculation of the lens-like action of a star's gravitational field, describing how general relativity can produce multiple or magnified images of a background source.
Einstein showed that exact alignment of source, lens and observer produces a circular image geometry, the configuration later widely known as an Einstein ring.
Publishes a calculation showing how a foreground star can gravitationally lens light from a background star.
Einstein published a short analysis of the lens-like action of a foreground star, giving a compact treatment of image formation and magnification caused by gravitational light bending.
After discussions with Rudi Mandl, Einstein returned to the lensing calculation he had explored in 1912 and agreed to publish the optical effect of gravitational light bending.
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.