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Berlin

123 Einstein records associated with Berlin.

Albert Einstein in a 1912 portrait
Albert Einstein, 1912. Photograph by J. F. Langhans โ€” public domain. Wikimedia Commons source.

Berlin Notebook Gravitational Lens Calculation

1912 ยท Berlin ยท Germany ยท Astronomy

During work recorded in a 1912 notebook, Einstein calculated how a foreground mass could bend light from a background source and produce the geometry of a gravitational lens.

Double-Image Lens Geometry Derived

1912 ยท Berlin ยท Germany ยท Astronomy

Einstein's notebook analysis showed that gravitational deflection could allow light from one distant source to reach an observer along two paths, producing two apparent images.

Lens Magnification Formula First Calculated

1912 ยท Berlin ยท Germany ยท Astronomy

Einstein worked out a magnification relation for the gravitational-lens configuration, anticipating formulae he would publish when he returned to the subject decades later.

Berlin Academy Appointment

1914 ยท Berlin ยท United States of America ยท Physics

Moves to Berlin for a senior research appointment and membership of the Prussian Academy of Sciences.

Covariance Problem in Gravitation

1914 ยท Berlin ยท United States of America ยท Physics

Publishes work refining the mathematical and covariance problems of his developing gravitational theory.

Covariance Restrictions Defended

1914 ยท Berlin ยท Germany ยท Physics

Einstein defended the restricted covariance of his provisional gravitational equations, believing at the time that broader coordinate freedom would prevent a unique physical description.

Einstein-Grossmann Covariance Analysis

1914 ยท Berlin ยท United States of America ยท Physics

Continues with Grossmann to examine covariance properties of their gravitational equations, exposing problems that eventually drive Einstein back toward general covariance.

Formal Entwurf Theory Presented in Berlin

1914 ยท Berlin ยท Germany ยท Physics

Einstein gave a systematic mathematical presentation of the Entwurf gravitational theory after moving to Berlin, clarifying its field equations, coordinate restrictions and physical assumptions.

Formal Foundations of General Relativity

1914 ยท Berlin ยท United States of America ยท Physics

Publishes a detailed formal treatment of the developing gravitational theory, presenting its mathematical structure before he restores fully general covariance.

Gravitational Conservation Laws Reconsidered

1914 ยท Berlin ยท Germany ยท Physics

Einstein investigated how energy and momentum conservation should be formulated when the gravitational field itself participates in the dynamics of spacetime.

Manifesto to Europeans

1914 ยท Berlin ยท United States of America ยท Physics

Co-signs a pacifist appeal opposing wartime nationalism among European intellectuals.

Nordstrom Gravitation Recast with Fokker

1914 ยท Berlin ยท United States of America ยท Physics

With Adriaan Fokker, reformulates Nordstrom's competing gravitation theory using tensor methods, clarifying how relativistic gravity could be expressed geometrically.

Rotating Coordinates Test the Entwurf Theory

1914 ยท Berlin ยท Germany ยท Physics

Einstein examined rotating coordinate systems as a demanding consistency test for the Entwurf equations, exposing difficulties that contributed to his later rejection of the provisional theory.

Einstein-de Haas Effect

1915 ยท Berlin ยท United States of America ยท Physics

Publishes experimental work with Wander de Haas linking magnetism to angular momentum.

Return to General Covariance

1915 ยท Berlin ยท Germany ยท Physics

Einstein abandoned key restrictions of the Entwurf approach and returned to generally covariant tensor equations, beginning the final rapid reconstruction of his gravitational theory.

Revised Solar Deflection Reaches Full Relativistic Value

November 1915 ยท Berlin ยท Germany ยท Astronomy

With the completed geometric treatment of gravity, Einstein obtained a solar light-deflection prediction approximately twice the value produced by his earlier equivalence-principle calculation.

Revised Solar Light-Bending Value

November 1915 ยท Berlin ยท United States of America ยท Astronomy

Using the completed theory, obtains the full gravitational deflection predicted for starlight grazing the Sun, approximately twice his earlier 1911 estimate.

November 4 Covariant Gravity Equations

4 November 1915 ยท Berlin ยท Germany ยท Physics

Einstein presented new gravitational field equations to the Prussian Academy that restored much broader covariance and marked the first of his decisive November 1915 communications.

Restricted Covariance Equations

4 November 1915 ยท Berlin ยท United States of America ยท Physics

Presents revised gravitational field equations to the Prussian Academy during his final push toward general relativity.

November 11 Vacuum Field Equations

11 November 1915 ยท Berlin ยท Germany ยท Physics

Einstein refined his field equations under a trace condition and showed how the revised framework could approach fully covariant gravitation in regions outside matter.

Second November Field Equations

11 November 1915 ยท Berlin ยท United States of America ยท Physics

Presents improved gravitational equations to the Prussian Academy and moves substantially closer to the generally covariant form completed later that month.

Unimodular Gravitation Equations

11 November 1915 ยท Berlin ยท United States of America ยท Physics

Presents another formulation of gravitation using a restricted coordinate condition with unit determinant.

Mercury Anomaly Reproduced without Adjustable Parameters

18 November 1915 ยท Berlin ยท Germany ยท Astronomy

The relativistic Mercury calculation matched the anomalous perihelion advance using the gravitational theory itself rather than introducing an additional planet or an adjustable correction to Newtonian gravity.

Mercury Perihelion

18 November 1915 ยท Berlin ยท United States of America ยท Astronomy

Explains Mercury's anomalous perihelion advance using the emerging general theory of relativity.

November 18 Mercury Advance Calculation

18 November 1915 ยท Berlin ยท Germany ยท Astronomy

Einstein used the emerging general theory to account for Mercury's unexplained perihelion advance, obtaining the observed residual shift that earlier gravitational models had failed to reproduce.

Final Generally Covariant Field Equations

25 November 1915 ยท Berlin ยท United States of America ยท Physics

Presents the final generally covariant gravitational field equations to the Prussian Academy, completing the mathematical core of general relativity.

General Relativity Field Equations

25 November 1915 ยท Berlin ยท United States of America ยท Physics

Presents the final generally covariant gravitational field equations to the Prussian Academy.

November 25 Matter-Coupled Field Equations

25 November 1915 ยท Berlin ยท Germany ยท Physics

Einstein presented the final generally covariant field equations including their coupling to matter, completing the mathematical core of general relativity.

Zangger Letter Revisits Gravitational Lensing

15 December 1915 ยท Berlin ยท Germany ยท Astronomy

Einstein mentioned the possibility of gravitational lensing in a letter to Heinrich Zangger, revisiting the double-image effect he had calculated in his 1912 notebook.

Absorption Probability Coefficient Defined

1916 ยท Berlin ยท Germany ยท Physics

Einstein represented the probability of an atom absorbing incident radiation and moving to a higher energy state with a coefficient proportional to the surrounding radiation density.

Atomic Transition Probabilities Introduced

1916 ยท Berlin ยท Germany ยท Physics

Einstein formulated radiation processes in terms of probabilities for transitions between atomic energy states, creating a statistical framework for absorption and emission.

Detailed Balance Applied to Matter and Radiation

1916 ยท Berlin ยท Germany ยท Physics

Einstein required upward and downward atomic transitions to balance in thermal equilibrium, using that condition to connect transition probabilities with the equilibrium radiation spectrum.

Energy Conservation in General Relativity

1916 ยท Berlin ยท United States of America ยท Physics

Develops the treatment of energy and momentum in the gravitational field, addressing how conservation laws operate within the generally covariant theory.

Foundation of General Relativity

1916 ยท Berlin ยท United States of America ยท Physics

Publishes a systematic presentation of the general theory of relativity and its field equations.

General Relativity Review Article Published

1916 ยท Berlin ยท Germany ยท Physics

Einstein published a comprehensive exposition of general relativity that assembled the geometric framework, field equations and physical consequences into a systematic theory.

Geodesic Motion Described in Curved Spacetime

1916 ยท Berlin ยท Germany ยท Physics

Einstein's mature theory described freely falling bodies as following the straightest possible world-lines through curved spacetime rather than being pulled by a Newtonian gravitational force.

German Physical Society Presidency

1916 ยท Berlin ยท United States of America ยท Physics

Serves as president of the German Physical Society during the consolidation of general relativity.

Gravitational Energy Flux Treated with Pseudotensor

1916 ยท Berlin ยท Germany ยท Physics

Einstein developed a gravitational energy-momentum construction to discuss how changing gravitational fields can transport energy despite the special conservation difficulties of general relativity.

Gravitational Waves Propagate at Light Speed

1916 ยท Berlin ยท Germany ยท Physics

Einstein's wave analysis showed that physical gravitational disturbances in the relativistic theory propagate through empty space at the speed of light.

Hamilton Principle for General Relativity

1916 ยท Berlin ยท United States of America ยท Physics

Formulates general relativity using Hamilton's variational principle, providing a compact mathematical route to the gravitational field equations and their conservation properties.

Kottler Equivalence Hypothesis Response

1916 ยท Berlin ยท United States of America ยท Physics

Responds to Friedrich Kottler's criticism of the equivalence hypothesis, defending the conceptual basis on which his route from special to general relativity depended.

Nonlinearity of Gravitational Field Established

1916 ยท Berlin ยท Germany ยท Physics

Einstein's field equations made gravity nonlinear, so the gravitational field contributes to the dynamics instead of behaving as a simple superposition of independent Newtonian forces.

Planck Spectrum Recovered from Transition Statistics

1916 ยท Berlin ยท Germany ยท Physics

Einstein showed that his statistical rules for absorption, spontaneous emission and induced emission can reproduce Planck's black-body radiation law under thermal equilibrium.

Quantum Theory of Radiation

1916 ยท Berlin ยท United States of America ยท Physics

Develops a quantum theory of radiation introducing transition probabilities later represented by Einstein coefficients.

Spontaneous Emission Probability Defined

1916 ยท Berlin ยท Germany ยท Physics

Einstein introduced a coefficient describing the probability that an excited atom will emit radiation spontaneously and fall to a lower energy state.

Stimulated Emission Probability Coefficient Defined

1916 ยท Berlin ยท Germany ยท Physics

Einstein introduced a second radiation-dependent transition probability in which incident radiation stimulates an excited atom to emit additional radiation.

Stress-Energy Identified as Source of Curvature

1916 ยท Berlin ยท Germany ยท Physics

General relativity connected spacetime curvature with the energy, momentum and stresses of matter, making the physical contents of the universe sources of the gravitational geometry.

Weak-Field Gravitational Waves Derived

1916 ยท Berlin ยท Germany ยท Physics

Einstein linearised the gravitational field equations in the weak-field limit and identified wave-like disturbances capable of propagating through spacetime.

Schwarzschild Solution Presented to Academy

13 January 1916 ยท Berlin ยท United States of America ยท Physics

Communicates Karl Schwarzschild's exact solution of the new field equations to the Prussian Academy, demonstrating that general relativity admits important exact solutions.

Gravitational Waves

June 1916 ยท Berlin ยท United States of America ยท Astronomy

Predicts gravitational waves as propagating disturbances in spacetime within general relativity.

Atomic Recoil Required by Photon Momentum

1917 ยท Berlin ยท Germany ยท Physics

By assigning momentum to individual radiation quanta, Einstein concluded that atoms must recoil when they emit or absorb directed packets of light.

Cosmological Term Added to Field Equations

1917 ยท Berlin ยท Germany ยท Astronomy

To support a static cosmological solution, Einstein modified the gravitational field equations with an additional cosmological term that could counterbalance large-scale attraction.

Machian Motivation Shapes Einstein Cosmology

1917 ยท Berlin ยท Germany ยท Astronomy

Einstein designed his early relativistic cosmology partly around the hope that inertia would be determined by the overall distribution of matter, reflecting his interpretation of Mach's ideas.

Random Emission Directions Linked to Molecular Motion

1917 ยท Berlin ยท Germany ยท Physics

Einstein showed that randomly directed quantum emission events contribute to molecular momentum fluctuations and must be balanced statistically in thermal equilibrium.

Relativistic Cosmology

1917 ยท Berlin ยท United States of America ยท Astronomy

Applies general relativity to the universe and introduces the cosmological constant in a static cosmological model.

Static Closed Universe Model Proposed

1917 ยท Berlin ยท Germany ยท Astronomy

Einstein applied general relativity to the universe as a whole and proposed a spatially closed, homogeneous model intended to remain static on cosmic scales.

Stimulated Emission

1917 ยท Berlin ยท United States of America ยท Physics

Formulates stimulated emission in his quantum theory of radiation, a principle later fundamental to lasers.

Stimulated Emission Predicted from Thermal Equilibrium

1917 ยท Berlin ยท Germany ยท Physics

Einstein's equilibrium analysis required an induced emission process in which incident radiation increases the probability that an excited atom emits matching radiation.

Gravitational Wave Energy Calculation Corrected

1918 ยท Berlin ยท Germany ยท Physics

Einstein revisited his gravitational-wave analysis and corrected the treatment of radiated energy, removing misleading wave modes from the earlier calculation.

Mach Principle Formulation

1918 ยท Berlin ยท United States of America ยท Physics

Publishes a foundational discussion of general relativity in which he explicitly names Mach's principle and distinguishes it from the equivalence and relativity principles.

Mass Quadrupole Identified as Leading Radiation Source

1918 ยท Berlin ยท Germany ยท Physics

Einstein showed that the leading gravitational radiation from an isolated slow-moving system is governed by changes in its mass quadrupole moment rather than by a simple mass dipole.

Quadrupole Radiation Formula

1918 ยท Berlin ยท United States of America ยท Physics

Derives the quadrupole formula for gravitational radiation, relating emitted wave power to changing mass distributions in accelerating systems.

International Scientific Fame

1919 ยท Berlin ยท United States of America ยท Physics

Becomes internationally famous after eclipse observations are widely reported as confirming general relativity.

Anti-Relativity Campaign

1920 ยท Berlin ยท United States of America ยท Physics

Publicly confronts organized attacks on relativity amid growing political and antisemitic hostility.

General Relativity Foundation Supplement

1921 ยท Berlin ยท United States of America ยท Physics

Publishes a proposed addition to the foundations of general relativity, continuing his effort to strengthen the conceptual and mathematical basis of gravitational field theory.

Nobel Prize in Physics

1921 ยท Berlin ยท United States of America ยท Physics

Awarded the 1921 Nobel Prize in Physics for theoretical physics, especially the law of the photoelectric effect.

Geometry and Experience Lecture

January 1921 ยท Berlin ยท United States of America ยท Physics

Explains how geometry acquires physical meaning through measurement and discusses the relationship between mathematical geometry and the spacetime structure of general relativity.

Early Unified Field Program

1922 ยท Berlin ยท United States of America ยท Physics

Begins sustained attempts to combine gravitation and electromagnetism within a single field framework.

Photoelectric Law Highlighted in Nobel Citation

1922 ยท Berlin ยท Germany ยท Physics

The Nobel citation singled out Einstein's quantitative law of the photoelectric effect, giving formal recognition to a result rooted in his 1905 light-quantum hypothesis.

Nobel Award Announced for Photoelectric Law

9 November 1922 ยท Berlin ยท Germany ยท Physics

The Royal Swedish Academy of Sciences announced Einstein as the recipient of the reserved 1921 Nobel Prize in Physics, emphasizing his discovery of the law of the photoelectric effect.

Affine Field Theory

1923 ยท Berlin ยท United States of America ยท Physics

Explores an affine field theory as a possible extension of general relativity, seeking a unified geometric description of gravitation and electromagnetism.

General Relativity Academy Paper

1923 ยท Berlin ยท United States of America ยท Physics

Publishes a further Prussian Academy paper on general relativity, revisiting technical aspects of the theory after its rapid international acceptance.

Bose Counting Recasts Planck Radiation Law

1924 ยท Berlin ยท Germany ยท Physics

Einstein recognized that Bose's counting method obtained Planck's spectrum by treating light quanta statistically without relying on the classical independent-particle counting used for ordinary gases.

Bose Light-Quantum Manuscript Reaches Einstein

1924 ยท Berlin ยท Germany ยท Physics

Satyendra Nath Bose sent Einstein a manuscript deriving Planck's radiation law by a new statistical counting method applied directly to indistinguishable light quanta.

Bose Paper Translation

1924 ยท Berlin ยท United States of America ยท Physics

Translates Satyendra Nath Bose's paper on Planck's law into German and arranges its publication.

Bose-Einstein Condensation Prediction

1924 ยท Berlin ยท United States of America ยท Physics

Predicts that ideal bosonic particles can accumulate in the lowest quantum state at low temperature.

Bose-Einstein Statistics

1924 ยท Berlin ยท United States of America ยท Physics

Extends Bose's statistical method from photons to particles of an ideal gas.

Einstein Translates Bose Photon Statistics Paper

1924 ยท Berlin ยท Germany ยท Physics

Einstein translated Bose's manuscript on the quantum statistics of radiation into German after recognizing the importance of its treatment of light quanta.

Photon Indistinguishability Gains Statistical Role

1924 ยท Berlin ยท Germany ยท Physics

Bose's method, promoted by Einstein, treated light quanta as statistically indistinguishable objects, an idea that became fundamental to quantum statistics.

BKS Statistical Conservation Challenged by Photon Picture

1925 ยท Berlin ยท Germany ยท Physics

Einstein continued to favour exact energy and momentum conservation in individual radiation processes rather than the merely statistical conservation proposed by the Bohr-Kramers-Slater approach.

Einstein Extends Radiation Duality Analogy to Matter

1925 ยท Berlin ยท Germany ยท Physics

Einstein drew an analogy between the wave-particle duality he had identified for radiation and the emerging wave description of material particles, reinforcing the broader quantum duality concept.

Quantum Mechanics Critique Begins

1925 ยท Berlin ยท United States of America ยท Physics

Engages critically with the emerging matrix and wave formulations of quantum mechanics.

Second Quantum Gas Paper

1925 ยท Berlin ยท United States of America ยท Physics

Publishes further work on the quantum theory of the ideal monatomic gas.

Unified Gravitation and Electromagnetism Paper

1925 ยท Berlin ยท United States of America ยท Physics

Publishes a unified field theory of gravitation and electricity, beginning a long programme to extend relativity into a single classical field framework.

Canal-Ray Radiation Coherence Test Proposed

1926 ยท Berlin ยท Germany ยท Physics

Einstein proposed experiments on light emitted by moving canal-ray atoms to test how quantum emission events could coexist with the coherence properties expected from wave optics.

Einstein-Szilard Refrigerator Work

1926 ยท Berlin ยท United States of America ยท Technology

Works with Leo Szilard on safer refrigerator designs without moving mechanical parts.

Kaluza Five-Dimensional Theory Reconsidered

1926 ยท Berlin ยท United States of America ยท Physics

Reconsiders Theodor Kaluza's five-dimensional approach after developments by Oskar Klein, seeing new possibilities for unifying gravitation and electromagnetism geometrically.

Rupp Radiation Experiments

1926 ยท Berlin ยท United States of America ยท Physics

Collaborates with Emil Rupp on proposed tests of whether atomic radiation behaves as waves or quanta.

Schrodinger Wave Mechanics Discussion

1926 ยท Berlin ยท United States of America ยท Physics

Studies and discusses Schrรถdinger's wave mechanics while questioning its physical interpretation.

General Relativity and Law of Motion

1927 ยท Berlin ยท United States of America ยท Physics

With Jakob Grommer, investigates whether the motion of particles can be derived from the gravitational field equations rather than imposed as a separate law.

Motion from Field Equations

1927 ยท Berlin ยท United States of America ยท Physics

Investigates with Jakob Grommer whether particle motion can follow directly from gravitational field equations.

Kaluza Theory Academy Papers

February 1927 ยท Berlin ยท United States of America ยท Physics

Presents Academy papers on Kaluza's connection between gravitation and electricity, deriving important aspects of the five-dimensional unified-field framework.

Distant Parallelism Geometry

1928 ยท Berlin ยท United States of America ยท Physics

Introduces a geometry that preserves distant parallelism, adopting teleparallel structures as a new mathematical basis for attempts to unify gravity and electromagnetism.

Einstein-Szilard Refrigerator Patent

1928 ยท Berlin ยท United States of America ยท Technology

Patent work with Leo Szilard advances an absorption refrigerator using electromagnetic pumping concepts.

Teleparallel Unified Field Programme

1928 ยท Berlin ยท United States of America ยท Physics

Develops the teleparallel unified-field programme, replacing ordinary Riemannian geometry with tetrad-based structures intended to encompass gravitation and electromagnetism together.

Teleparallel Unified Field Theory

1928 ยท Berlin ยท United States of America ยท Physics

Develops a unified-field approach using distant parallelism, also called teleparallel geometry.

Tetrad Fields Introduced for Unified Gravitation

1928 ยท Berlin ยท Germany ยท Physics

Einstein adopted tetrad fields and distant parallelism as a new geometric language in an attempt to place gravitation and electromagnetism inside one unified classical field theory.

Helen Dukas Becomes Assistant

13 April 1928 ยท Berlin ยท United States of America ยท Physics

Employs Helen Dukas as his secretary and assistant, beginning a long professional association.

Unified Field Theory and Hamilton Principle

1929 ยท Berlin ยท United States of America ยท Physics

Publishes a unified field formulation based on distant parallelism and Hamilton's principle, continuing his search for equations joining gravitational and electromagnetic fields.

Unified Field Theory Publication

1929 ยท Berlin ยท United States of America ยท Physics

Publishes a widely publicized unified-field theory based on teleparallel geometry.

Max Planck Medal

28 June 1929 ยท Berlin ยท United States of America ยท Physics

Receives the inaugural Max Planck Medal for outstanding achievement in theoretical physics.

Space and Ether Harnack House Lecture

December 1929 ยท Berlin ยท United States of America ยท Physics

Lectures at Harnack House on the problem of space and ether, revisiting how relativity changes the physical interpretation of spacetime and field structure.

Exact Static Unified-Field Solutions

1930 ยท Berlin ยท United States of America ยท Physics

Publishes work with Walther Mayer giving exact static solutions of unified-field equations, testing whether the programme can represent physically meaningful configurations.

Riemann Metric and Distant Parallelism

1930 ยท Berlin ยท United States of America ยท Physics

Further develops spaces combining a Riemann metric with distant parallelism, refining the geometric machinery behind his teleparallel unified-field theory.

Unified Field Equation Compatibility

1930 ยท Berlin ยท United States of America ยท Physics

Examines the compatibility of equations in the unified-field programme, addressing mathematical consistency before the theory can be regarded as physically viable.

Expanding Universe Paper

1931 ยท Berlin ยท United States of America ยท Astronomy

Adopts an expanding cosmological model and abandons the need for his earlier static-universe construction.

Expanding-Universe Cosmology Paper

1931 ยท Berlin ยท United States of America ยท Astronomy

Publishes a non-static cosmological model within general relativity, accepting cosmic expansion and dispensing with the static balance that motivated his cosmological constant.

Unified Gravitation and Electricity Theory

1932 ยท Berlin ยท United States of America ยท Physics

Publishes another unified theory of gravitation and electricity, continuing to test alternative geometrical structures beyond the standard equations of general relativity.