Princeton Stafford Little Lectures
Delivers four Stafford Little Lectures explaining special and general relativity.
Albert Einstein ยท Place
53 Einstein records associated with Princeton.

Delivers four Stafford Little Lectures explaining special and general relativity.
The Meaning of Relativity is published from the four lectures Einstein delivered at Princeton in May 1921.
Publishes The Meaning of Relativity from his Princeton lectures, giving a systematic account of special relativity, tensor methods, gravitation and cosmological applications.
Receives an invitation to accept a research professorship at Princeton University.
Accepts appointment to the newly founded Institute for Advanced Study.
Settles in the United States after the Nazi rise to power and joins the Institute for Advanced Study.
Publishes reflections on how fundamental theoretical physics develops from principles and mathematical structure.
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.
With Nathan Rosen, studies bridge solutions in general relativity connecting two sheets of spacetime.
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.
Einstein, Podolsky and Rosen publish their argument that quantum mechanics may not provide a complete description of physical reality.
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 and Nathan Rosen initially question whether exact gravitational waves exist, then recognise that a troublesome singularity is a coordinate effect rather than a physical obstruction.
With Nathan Rosen, submits a manuscript questioning gravitational waves, then revises the analysis after recognising that a problematic singularity arose from the coordinates used.
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.
Einstein quantified the magnification produced by gravitational deflection in a simple stellar-lens geometry, linking image brightness to the angular alignment of source and lens.
Einstein's lensing note described how imperfect alignment can produce two apparent images of a background star because its light reaches the observer along different curved paths.
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.
Works with Leopold Infeld and Banesh Hoffmann on deriving equations of motion from general relativity.
Einstein and Rosen publish a corrected paper showing cylindrical gravitational-wave solutions.
Einstein and Rosen publish a corrected treatment of cylindrical gravitational waves, demonstrating that exact wave solutions can exist within general relativity.
With Leopold Infeld and Banesh Hoffmann, Einstein developed an approximation in which the motion of gravitating bodies follows from the relativistic field equations rather than from a separately imposed force law.
Publishes work deriving approximate equations of motion for gravitating bodies from general relativity.
Publishes The Evolution of Physics with Leopold Infeld for a broad readership.
With Leopold Infeld, publishes The Evolution of Physics, explaining the conceptual transition from classical mechanics and fields to relativity and modern physics.
Studies a stationary spherical system of gravitating particles and argues that such configurations do not naturally form the Schwarzschild-type singular surface then under discussion.
Writes again to President Roosevelt urging stronger attention to uranium research developments.
Sends another letter to Roosevelt concerning the need for effective action on uranium research.
With Wolfgang Pauli, proves a restrictive result on non-singular stationary solutions of the relativistic gravitational field equations with nonzero total mass.
Publishes a generalization of the relativistic theory of gravitation, continuing his attempt to construct a unified classical field theory extending general relativity.
After the atomic bombings, speaks publicly about the political and ethical dangers of nuclear weapons.
Signs a letter drafted by Leo Szilard seeking a presidential meeting on nuclear policy; Roosevelt dies before receiving it.
Publishes an elementary derivation of the equivalence of mass and energy, revisiting one of the central physical consequences that emerged from special relativity.
Helps form and chairs the Emergency Committee of Atomic Scientists to promote public education and international control.
Presents a new draft of field equations for his continuing general field theory program.
Supports public education campaigns on atomic energy, disarmament and international control.
Publishes a generalized theory of gravitation in Reviews of Modern Physics, presenting another stage of his sustained search for a unified geometric field theory.
Publishes Autobiographical Notes, reflecting on the development of his scientific ideas and philosophy.
In his Autobiographical Notes, reconstructs the intellectual path from special relativity through the equivalence principle to general relativity and later unified-field research.
Comments on Kurt Godel's rotating cosmological solution, acknowledging that general relativity permits global spacetime structures with profound consequences for the concept of time.
Presents and revises his mature attempts to construct a unified classical field theory.
Publishes a collection of essays on science, society, philosophy and public affairs.
A revised English edition of his relativity exposition appears, updating the presentation of special and general relativity for a postwar scientific readership.
Explains his latest generalized theory of gravitation in Scientific American, placing the work within his long search for a unified foundation of field physics.
Refines asymmetric-field approaches intended to combine gravitation and electromagnetism.
Declines the offer to become president of Israel, citing lack of aptitude and experience for official duties.
Publishes a response to criticism of unified field theory, defending the mathematical programme through which he hoped to extend relativistic field physics.
With Bruria Kaufman, studies algebraic properties of the asymmetric field in a relativistic unified theory, refining the mathematical structure of his late programme.
With Bruria Kaufman, develops a new form of general relativistic field equations, one of the final technical products of Einstein's lifelong geometric programme.
Signs Bertrand Russell's appeal warning of nuclear war and urging peaceful resolution of international disputes.
Albert Einstein dies in Princeton, New Jersey, aged 76.