Einstein's scientific publications are listed below in four tables: journal articles, book chapters, books and authorized translations. Each publication is indexed in the first column by its number in the Schilpp bibliography (Albert Einstein: Philosopher–Scientist, pp. 694–730) and by its article number in Einstein's Collected Papers. Complete references for these two bibliographies may be found below in the Bibliography section. The Schilpp numbers are used for cross-referencing in the Notes (the final column of each table), since they cover a greater time period of Einstein's life at present. The English translations of titles are generally taken from the published volumes of the Collected Papers. For some publications, however, such official translations are not available; unofficial translations are indicated with a § superscript. Collaborative works by Einstein are highlighted in lavender, with the co-authors provided in the final column of the table.
There were also five volumes of Einstein's Collected Papers (volumes 1, 5, 8–10) that are devoted to his correspondence, much of which is concerned with scientific questions, but were never prepared for publication.
Chronology and major themes
The following chronology of Einstein's scientific discoveries provides a context for the publications listed below, and clarifies the major themes running through his work. Einstein's scientific career can be broadly divided into to periods. During the first period (from 1901 to 1933), Einstein published mainly in German-language journals, notably the Annalen der Physik, and, after becoming a professional physicist, worked at various German-speaking institutions in Europe, including the Prussian Academy of Sciences in Berlin. Following his permanent relocation to the United States in 1933, Einstein spent most of his time at the Institute for Advanced Study in Princeton, New Jersey, where he remained till his death in 1955. During his second period, Einstein submitted his papers in English to North American journals, such as the Physical Review.[4] Einstein first gained fame among physicists for the papers he submitted in 1905, his annus mirabilis or miraculous year in physics. His epochal contributions during this phase of his career stemmed from a single problem, the fluctuations of a delicately suspended mirror inside a radiation cavity. It led him to examine the nature of light, the statistical mechanics of fluctuations, and the electrodynamics of moving bodies.[5]
From 1901 to 1904, Einstein submitted his first scientific papers, dealing with problems in thermodynamics and statistical mechanics.[6]
In 1905, Einstein proposed that the existence of light quanta—dubbed photons by chemist Gilbert Lewis in 1926—could explain the photoelectric effect.[7] He treated electromagnetic radiation as a gas and applied thermodynamic reasoning in his "heuristic" treatment, arguing that the energy of a photon is given by Planck's relation, , where is a new constant of nature (the Planck constant), and (nu) is the frequency of the photon. Whereas Max Planck had introduced the quantum hypothesis as merely a mathematical trick to obtain the correct description of blackbody radiation (Planck's law), Einstein considered it to be an aspect of physical reality.[8]: 94–101 In one of his 1905 calculations, Einstein also used, but did not justify or explain, the equation , where is the momentum of the photon and is the speed of light in vacuum.[9] In 1909, Einstein showed that the photon carries momentum as well as energy and that electromagnetic radiation must have both particle-like and wave-like properties if Planck's law of blackbody radiation holds; this was a forerunner of the principle of wave–particle duality.[10] He would go on to receive the 1921 Nobel Prize in Physics for his investigations of light quanta.[6]
In 1905, to avoid getting into a dispute with his supervisor, Alfred Kleiner, Einstein selected a fairly conventional problem to tackle for his doctoral dissertation, namely, the determination of molecular dimensions using classical hydrodynamics.[11] Such calculations had already been done using gases. But Einstein was the first to successfully solve the problem using liquids. Einstein obtained a respectable estimate for the Avogadro constant, after incorporating better experimental data.[8]: 101–103 Einstein received his doctorate in January 1906 from the University of Zurich.[6] Einstein's doctoral dissertation remains one of his most cited papers ever, with applications in various engineering disciplines, such as concrete mixing and dairy production.[8]: 103 The month following this paper, Einstein submitted a theory of Brownian motion, named after botanist Robert Brown, in terms of fluctuations in the number of molecular collisions with an object,[12] providing further evidence that matter was composed of atoms.[6] He showed that the distance a grain of pollen suspended in a liquid traveled from its starting point was proportional to the square root of the time elapsed and determined Avogadro's number in a new way.[8]: 103–106 A few weeks earlier, he had derived the Einstein relation for diffusion, which was the first example of the general fluctuation–dissipation theorem and gave an estimate of Avogadro's constant.[13] Within months, Einstein's description of Brownian motion was experimentally verified by Henry Siedentopf.[8]: 103–106
In 1905, Einstein concluded that "The mass of a body is a measure of its energy content." In modern form, the equation he wrote down was , where is of an object, is the mass of that object, and is the speed of light in vacuum. He suggested that "bodies whose energy contents is variable to a high degree, e.g. salts of radium" be used to test his new equation.[17]: 137–139 Einstein's mass–energy equivalence was later verified by studying mass defect in atomic nuclei. The energy released in nuclear reactions[18]—which is essential for nuclear power and nuclear weapons—can be estimated from such mass defects.[19]
Between 1914 and 1915, Einstein and Wander Johannes de Haas published a series papers on their experiments showing that a change in the magnetic moment of a free body caused this body to rotate. The Einstein-de Haas effect is a consequence of the conservation of angular momentum and is a demonstration of quantum spin, not yet understood at the time. Einstein and de Haas argued that their results supported the hypothesis by André-Marie Ampère that "molecular currents" were responsible for the field of a magnet, essentially suggesting the existence of the electron.[39][40]
In 1916, Einstein predicted the existence of gravitational waves. However, this paper was full of errors and misconceptions. He corrected most of these in another paper published in 1918, but his formula for the energy flux radiated by a slow-moving source was still off by a factor of two. Arthur Stanley Eddington later noticed and corrected the error.[41] Einstein returned to the problem in 1936 with his assistant, Nathan Rosen, arguing that gravitational waves did not exist. An anonymous reviewer commented that they had misunderstood the nature of the coordinates they were using.[4] Einstein and Rosen resolved his issue and reached the opposite conclusion, exhibiting an exact solution to the Einstein field equations, the Einstein–Rosen metric, describing cylindrical gravitational waves.[4][41] Gravitational waves have been detected by observing the Hulse–Taylor pulsar[42] and directly by the Laser Interferometer Gravitational-wave Observatory (LIGO).[43]
In 1917, Einstein presented the semi-classical Einstein–Brillouin–Keller method for computing the eigenvalues of a quantum-mechanical system.[44][45] An improvement of the Bohr–Sommerfeld quantization condition,[46] it allows for the solution of a variety of problems.[45] The Bohr model of the hydrogen atom is a simple example, but the EBK method also gives accurate predictions for more complicated systems, such as the dinuclear cations H2+ and HeH2+.[47]
In 1917, Einstein began the scientific study of cosmology. In order to ensure that his field equations predict a static universe, as was commonly thought at the time, Einstein introduced the cosmological constant (capital lambda). In the early 1930s, upon learning of Edwin Hubble's confirmation of the expansion of the universe, Einstein retracted .[48]: 355–6 The current understanding is that is non-zero. As Steven Weinberg explained, "it was not easy to just drop the cosmological constant, because anything that contributes to the energy density of the vacuum acts just like a cosmological constant."[49]
In 1918, Einstein developed a general theory of the process by which atoms emit and absorb electromagnetic radiation (the Einstein coefficients), which is the basis of lasers (light amplification by stimulated emission of radiation) and shaped the development of modern quantum electrodynamics, the best-validated physical theory at present.[50]
In 1924, Einstein read a paper from Satyendra Nath Bose deriving Planck's law using a new statistical method for photons. He developed the idea further into the Bose–Einstein statistics and applied it to ensembles of particles with mass, such as atoms, and predicted the Bose–Einstein condensates, a new state of matter.[51]: 327–329 The Bose–Einstein condensation was first achieved in 1995 by Carl Edwin Wieman and Eric Allin Cornell using rubidium-87. Since then, the Bose–Einstein condensation has also been achieved using other materials, such as liquid helium-4, which becomes a superfluid at temperatures below 2.17 K.[52] Bose and Einstein's papers are seminal contributions to quantum statistical mechanics, which form the basis for superfluidity, superconductivity, and other phenomena.[53]
In 1935, together with Boris Podolsky and Nathan Rosen, Einstein put forward what is now known as the EPR paradox. Einstein and his colleagues argued that the quantum-mechanical wave function must be an incomplete description of the physical world, and that there could be "hidden variables" not accounted for in standard quantum mechanics.[54] This paper describes the phenomenon of quantum entanglement, a term coined by Erwin Schrödinger in a paper published in the same year in which Schrödinger states his cat paradox.[55] It is Einstein's most controversial paper,[4] and the most important one he published after migrating to the U.S.[55] In 1951, David Bohm reformulated he original thought experiment was reformulated in terms of spin and in 1964, John Stewart Bell proposed experiments to test the inequalities he derived. A variety of experiments conducted since the 1970s with ever improving reliability have demonstrated the reality of quantum entanglement and disproven Einstein's notion of local realism.[55][56]
In the final thirty years of his life, Einstein explored whether various classical unified field theories could account for both electromagnetism and gravitation and, possibly, quantum mechanics using increasingly sophisticated mathematics, such as distant parallelism. He was joined by a handful of researchers, notably Hermann Weyl, Theodor Kaluza, and Oskar Klein.[48] However, their efforts were ultimately unsuccessful, since those theories did not match experimental results.[59] For example, the Kaluza–Klein theory, which Einstein briefly pursued, predicted the wrong mass for the electron by a factor of about 1018.[60]
Journal articles
Most of Einstein's original scientific work appeared as journal articles. Articles on which Einstein collaborated with other scientists are highlighted in lavender, with the co-authors listed in the "Classification and notes" column. These are the total of 272 scientific articles.
Intermolecular forces.[61] The first of two papers in which Einstein proposed the (incorrect) theory that the interactions between all molecules are a universal function of distance, in analogy with the inverse-square force of gravity. Once parameterized, his theory makes reasonably accurate predictions for heavier hydrophobic molecules, but fails for lighter molecules.
Schilpp 2; CP2, 2
1902
Thermodynamische Theorie der Potentialdifferenz zwischen Metallen und vollständig dissoziierten Lösungen ihrer Salze, und eine elektrische Methode zur Erforschung der Molekularkräfte
On the Thermodynamic Theory of the Difference in Potentials between Metals and Fully Dissociated Solutions of Their Salts and on an Electrical Method for Investigating Molecular Forces
Intermolecular forces.[62] Einstein's second paper on a universal molecular energy function, this time applied to electrolytic solutions. No data are available for comparison. Einstein characterizes these two papers as "worthless" in 1907.[63]
Schilpp 3; CP2, 3
1902
Kinetische Theorie des Wärmegleichgewichtes und des zweiten Hauptsatzes der Thermodynamik
Kinetic Theory of Thermal Equilibrium and of the Second Law of Thermodynamics
Review of Nikolay Nikolayevich Schiller: "Einige Bedenken betreffend die Theorie der Entropievermehrung durch Diffusion der Gase bei einander gleichen Anfangsspannungen der letzteren"
Review of Nikolay Nikolayevich Schiller: "Some Concerns Regarding the Theory of Entropy Increase Due to the Diffusion of Gases Where the Initial Pressures of the Latter Are Equal"
Photons.[67] Proposal of the photon as a quantum of energy, supported by many independent arguments.
Remarkably, the first English translation did not appear until the sixtieth anniversary of the original work when it was published in the American Journal of Physics, Volume 33, Number 5, May 1965 (English translation by A.B. Arons and M.B. Peppard).
Special relativity.[69] This seminal paper gave birth to special relativity (SR). In particular, it stated the two postulates of SR (uniform motion is undetectable, and the speed of light is always constant) and its kinematics.
Schilpp 10; CP2, 24; Weil *10
1905
Ist die Trägheit eines Körpers von seinem Energieinhalt abhängig?
Does the Inertia of a Body Depend upon its Energy Content?
Special relativity.[70] A follow-on from his last paper, this paper derived the conclusion that mass was equivalent to an energy and vice versa, leading to the equation E = mc2.
CP2, 25
1905
Review of Heinrich Birven: Grundzüge der mechanischen Wärmetheorie
Review of Heinrich Birven: Fundamentals of the Mechanical Theory of Heat
Photons.[73] Einstein reconciles his and Planck's independent derivations of the blackbody formula E=hν. Planck's derivation of this formula ascribed it to a restriction on the energy changes possible when radiation is produced or absorbed by matter, which implied no restriction on the energies of either matter or radiation. Einstein's 1905 derivation ascribed it to a restriction on the energy of radiation alone, but in this paper, he proposes the modern idea that the energies of both matter and radiation are quantized, which led to his work on quantum specific heats, such as reference #16.
Schilpp 14; CP2, 35
1906
Prinzip von der Erhaltung der Schwerpunktsbewegung und die Trägheit der Energie
The Principle of Conservation of Motion of the Center of Gravity and the Inertia of Energy
Special relativity.[78] Einstein's discovery of the transverse Doppler effect, in which the perceived frequency is shifted even when the line between the wave source and receiver and the source's velocity are perpendicular.
Schilpp 19
1907
Bemerkung zur Notiz des Herrn P. Ehrenfest: Translation deformierbarer Elektronen und der Flächensatz
Comments on the Note of Mr. Paul Ehrenfest: The Translatory Motion of Deformable Electrons and the Area Law
Special relativity.[80] First statement that the total energy of a particle in rest equals E = mc2. Derives the transformation of energy and momentum under the influence of external forces (relativistic dynamics). Notes again the difficulty of applying Lorentz transformations to rigid bodies (see reference #19). Finally, speculates that Maxwell's equations will prove to be the limiting case for large numbers of light-quanta, just as thermodynamics is a limiting case of statistical mechanics.
CP2, 46
1907
Review of Jakob Johann Weyrauch: Grundriss der Wärmetheorie. Mit zahlreichen Beispielen und Anwendungen
Review of Jakob Johann Weyrauch: An Outline of the Theory of Heat. With Numerous Examples and Applications. Part 2.
Neue elektrostatische Methode zur Messung kleiner Elektrizitätsmengen
A New Electrostatic Method for the Measurement of Small Quantities of Electricity
Physikalische Zeitschrift, 9, 216–217
Electromagnetism.[85] Novel experimental method for measuring tiny amounts of charge, by first charging a variable capacitor at low capacitance, then changing it to high capacitance and discharging it to another capacitor. An apparatus for this amplification was constructed by two brothers, Johann Conrad Habicht and Franz Paul Habicht, in collaboration with Einstein and published in Physikalische Zeitschrift, 11, 532 (1910).
Photons.[89] Walther Ritz's joint communique with Einstein (co-author) on their differing viewpoints of the advanced and retarded solutions of Maxwell's equations. Einstein argues that the physical restriction to retarded solutions is not a law, but probabilistic; Ritz states that the same restriction is the basis of the 2nd law of thermodynamics.
Schilpp 30; CP2, 60
1909
Entwicklung unserer Anschauungen über das Wesen und die Konstitution der Strahlung
On the Development of Our Views Concerning the Nature and Constitution of Radiation
Physikalische Zeitschrift, 10, 817–825
Photons.[90] Pivotal address before the 81st assembly of the Gesellschaft Deutscher Naturforscher, held in Salzburg, where Einstein showed that photons must carry momentum and should be treated as particles. Notes that electromagnetic radiation must have a dual nature, at once both wave-like and particulate. Also published in the journal Deutsche physikalische Gesellschaft, Verhandlungen, 11, pp. 482–500. An English translation is available at the English Wikisource.
Schilpp 31; CP3, 7
1910
Über einen Satz der Wahrscheinlichkeitsrechnung und seine Anwendung in der Strahlungstheorie
On a Theorem of the Probability Calculus and Its Application in the Theory of Radiation
Specific heats.[101] Recognizing that his 1907 model of specific heats is incorrect at very low temperatures, Einstein tries to improve it. The correct answer came a year later with the Debye model.
Schilpp 42; CP3, 23; Weil *43
1911
Einfluss der Schwerkraft auf die Ausbreitung des Lichtes
On the Influence of Gravitation on the Propagation of Light
General relativity.[102] In this paper, Einstein resumes his development of general relativity, last discussed in 1907. Here, Einstein realizes that a new theory is needed to replace both special relativity and Newton's theory of gravitation. He also realizes that special relativity and the equivalence principle hold locally, not globally.
General relativity.[106] First of two papers (see next entry for second) in the continuing development of general relativity (see reference #42). These two papers are the last in which Einstein allows time to be warped while keeping space flat (uncurved). In these papers, he realizes that the Lorentz transformations of special relativity must be generalized and that the new theory of gravitation must be nonlinear, since gravitational energy can itself gravitate.[107]
Entwurf einer verallgemeinerten Relativitätstheorie und eine Theorie der Gravitation. I. Physikalischer Teil von A. Einstein II. Mathematischer Teil von M. Grossmann
Outline of a Generalized Theory of Relativity and of a Theory of Gravitation. I. Physical Part by A. Einstein II. Mathematical Part by M. Grossmann
Zeitschrift für Mathematik und Physik, 62, 225–244, 245–261
General relativity.[113] A breakthrough paper, written in collaboration with Marcel Grossmann, in which the single Newtonian scalargravitational field is replaced by ten fields, which are the components of a symmetric, four-dimensional metric tensor. However, the correct equations describing these fields are not identified. Reviewed critically in reference #68. See also references #21, 42, 46 and 47.
Schilpp 54; CP4, 11
1913
Einige Argumente für die Annahme einer molekular Agitation beim absoluten Nullpunkt
Some Arguments for the Assumption of Molecular Agitation at Absolute Zero
Specific heats.[114] Co-authored with O. Stern. Einstein and Stern attempt to explain the specific heats of diatomic gases, such as molecular hydrogen, H2. Although qualitatively correct, they are quantitatively inaccurate.[115]
Schilpp 55; CP4, 12
1913
Déduction thermodynamique de la loi de l'équivalence photochimique
Thermodynamic Deduction of the Law of Photochemical Equivalence
Journal de physique (ser. 5), 3, 277–282
Statistical mechanics.[116] Not a translation of reference #45, but rather an address before the Société Française de Physique, held on March 27, 1913.
Schilpp 56; CP4, 16
1913
Physikalische Grundlagen einer Gravitationstheorie
General relativity.[117] Address before the Swiss Society of Scientists on September 9, 1913. A résumé is printed in the Schweizerische naturforschende Gesellschaft, Verhandlungen, 1913 (part 2), pp. 137–138.
On the Present State of the Problem of Gravitation
Physikalische Zeitschrift, 14, 1249–1266
General relativity.[119] Address on September 21, 1913, to the 85th Versammlung Deutscher Naturforscher in Vienna. The discussion following Einstein's address is included in this citation. This review was also published in the Gesellschaft deutscher Naturforscher und Ärzte, Verhandlungen, 1914, pp. 3–24. A referat was also published in the journal Himmel und Erde, 26, pp. 90–93.
Schilpp 59; CP4, 28
1914
Nordströmsche Gravitationstheorie vom Standpunkt des absoluten Differentialkalküls
Nordström's Theory of Gravitation from the Point of View of the Absolute Differential Calculus
Die Formale Grundlage der allgemeinen Relativitätstheorie
The Formal Foundations of the General Theory of Relativity§
Preussische Akademie der Wissenschaften, Sitzungsberichte, 1914 (part 2), 1030–1085
General relativity.[128] An important paper in the development of general relativity. Einstein still has not derived correct field equations, but he derives the geodesic motion of point particles, relates gravitational fields to rotation, and re-derives his 1907 results about the bending of light and gravitational redshift using the new metric tensor theory.
Preussische Akademie der Wissenschaften, Sitzungsberichte, 1915 (part 2), 778–786, 799–801
General relativity.[137] Second of Einstein's four papers in November 1915 that led to the final field equations for general relativity. The first paper had corrected a fundamental misconception and had allowed Einstein to finish; however, the second introduced a serious mistake.[138]
Schilpp 84; CP6, 24; Weil *76
1915
Erklärung der Perihelbewegung des Merkur aus der allgemeinen Relativitätstheorie
Explanation of the Perihelion Motion of Mercury from the General Theory of Relativity
Preussische Akademie der Wissenschaften, Sitzungsberichte, 1915 (part 3), 831–839
General relativity.[139] Third of Einstein's four papers in November 1915. A pivotal paper in which Einstein shows that general relativity explains the anomalous precession of the planet Mercury, which had vexed astronomers since 1859. This paper also introduced the important calculational method, the post-Newtonian expansion. Einstein also calculated correctly (for the first time) the bending of light by gravity.
Schilpp 85; CP6, 25
1915
Feldgleichungen der Gravitation
The Field Equations of Gravitation
Preussische Akademie der Wissenschaften, Sitzungsberichte, 1915 (part 4), 844–847
General relativity.[140] Fourth of Einstein's four papers in November 1915. This is the defining paper of general relativity. At long last, Einstein had found workable field equations, which served as the basis for subsequent derivations.
Schilpp 88; CP6, 14
1916
Experimental proof of the existence of Ampère's molecular currents
Proceedings of the Akademie van Wetenschappen, Amsterdam, 18, 696–711,link[permanent dead link]
Strahlungs-emission und -absorption nach der Quantentheorie
Emission and Absorption of Radiation in Quantum Theory
Verhandlungen der Deutschen Physikalischen Gesellschaft, 18, 318–323
Photons.[145] Seminal paper in which Einstein showed that Planck's quantum hypothesis E=hν could be derived from a kinetic rate equation. This paper introduced the idea of stimulated emission (which led to the laser and maser), and Einstein's A and B coefficients provided a guide for the development of quantum electrodynamics, the most accurately tested theory of physics at present. In this work, Einstein begins to realize that quantum mechanics seems to involve probabilities and a breakdown of causality.[146]
Schilpp 93; CP6, 38
1916
Quantentheorie der Strahlung
On the Quantum Theory of Radiation
Mitteilungen der Physikalischen Gesellschaft, Zürich, 16, 47–62
Photons.[147] Following his 1909 address (reference #30), Einstein shows that photons must carry momentum if Planck's law is to hold. This was confirmed in 1923 by Compton scattering, for which the 1927 Nobel Prize in Physics was awarded and which led to the general acceptance to the photon concept.
Schilpp 94; CP6, 36
1916
Review of H. A. Lorentz: Théories statistiques en thermodynamique
Review of H. A. Lorentz: Statistical Theories in Thermodynamics: Five Lectures...
Report of a lecture at King's College on the development and present position of relativity, with quotations
Nation and Athenaeum, 29, 431–432
Special and general relativity. The German text is reproduced in Mein Weltbild (pp. 215–220); a full translation is found in The World as I See It. It was also reported in Nature (107, p. 504) and also in the Times (London) on June 14, p. 8.
Schilpp 159
1922
Bemerkung zur Seletyschen Arbeit: Beiträge zum kosmologischen Problem
Observation of the Paper of Selety: Contributions to the Cosmological Problem§
Photons.[193] Experiment showing that photons could carry momentum; for many physicists, this experiment was conclusive proof that photons were particles.
Schilpp 184
1924
Zum hundertjährigen Gedenktag von Lord Kelvins Geburt
Interferenzeigenschaften des durch Kanalstrahlen emittierten Lichtes
Interference Properties of Light Emitted by Canal Rays§
Sitzungsberichte der Preussischen Akademie der Wissenschaften, Physikalisch-mathematische Klasse, 1926, 334–340
Photons.[208] Supposedly verified experimentally by Rupp in the paper following it in the journal (pp. 341–351); later, it came out that Rupp was a fraud.
Schilpp 203
1926
Geometría no euclídea y física
Non-Euclidean Geometry and Physics§
Revista matemática Hispano-americana (ser. 2), 1, 72–76
History of physics. Reprinted in the Manchester Guardian (March 19, 1927); Observatory, 50, 146–153; Smithsonian Institution, Report for 1927, 201–207.
Schilpp 208
1927
Newtons Mechanik und ihr Einfluss auf die Gestaltung der theoretischen Physik
Newton's Mechanics and its Influence on the Formation of Theoretical Physics§
Special and general relativity. Einstein's discussions with RG Loyarte on mass–energy equivalence and with H Damianovich on the relevance of relativity for a proposed "chemical field".
The Problems of Space, Fields and Aether in Physics§
World power conference, 2nd, Berlin, 1930. Transactions, 19, 1–5
Special and general relativity. A widely reported address, e.g., in Dinglers polytechnisches journal, 345, p. 122.
Schilpp 234
1930
Raum, Äther und Feld in der Physik
Space, Aether and Field in Physics§
Forum Philosophicum, 1, 173–180
Special and general relativity.[227] An English translation by ES Brightman was provided in the same volume, pp. 180–184. Similar to #233, but different from the article "Das Raum-, Äther-, und Feld-problem der Physik" reprinted in Mein Weltbild (The World as I See It), pp. 229–248.
Special and general relativity.[235] A survey of relativity theory (special and general) and of field theory in general. A précis of the talk was published in Nature, 125, pp. 897–898, under the title "Concept of space".
Schilpp 243
1930
Über den gegenwärtigen Stand der allgemeinen Relativitätstheorie
On the Present Status of the General Theory of Relativity§
Yale University Library, Gazette, 6, 3–6
General relativity.[236] An English translation by Prof. Leigh Page of Yale University was provided on pages 7–10. This was neither a scientific talk nor a typical scientific paper; rather, a Yale graduate convinced Einstein to write the summary by longhand; the manuscript is still housed at Yale.
Schilpp 247
1931
Theory of Relativity: Its Formal Content and Its Present Problems
Quantum mechanics.[258] An English translation (by J Picard) is provided on pages 349–382. Also reprinted in Zeitschrift für freie deutsche Forschung, 1, no. 1, pp. 5–19 and no. 2, pp. 1–14 (1938).
Special relativity.[275] Novel, simplified derivation in the Yearbook of American Society for Advancement of the Hebrew Institute of Technology in Haifa. Also published in Hebrew in 1947, in the Scientific Publications of Hebrew Technical College (Institute of Technology) in Haifa.
With the exception of publication #288, the following book chapters were written by Einstein; he had no co-authors. Given that most of the chapters are already in English, the English translations are not given their own columns, but are provided in parentheses after the original title; this helps the table to fit within the margins of the page. These are the total of 31.
Special and general relativity. The first edition of this book is listed as publication #102. Editions of this work were published until 1922 (the 14th edition). Editions 10–14 contained an additional section "Rotverschiebung der Spectrallinien" (Redshift of spectral lines) in the appendix.
Schilpp 131
1920
Äther und Relativitätstheorie: Rede gehalten am 5. Mai 1920 an der Reichs-Universität zu Leiden
Aether and Relativity Theory: A Talk Given on May 5, 1920, at the University of Leiden§
Springer Verlag (Berlin)
Special and general relativity.[303] The French, English, and Italian translations are listed as publications #145, 152, and 153, respectively. An undated Polish translation by L. Freundenheim, Eter a teorja wzglednosci, was published in Lviv. Also published with variant subtitle in Dutch (although the text is German), Aether und Relativitaetstheorie: Rede Uitgesproken bij de Aanvaarding van het Ambt van Bijzonder Hoogleerar aan de Rijks-Universiteit te Leiden.
Schilpp 143
1921
Geometrie und Erfahrung, Erweiterte Fassung des Festvortrages gehalten an der Preussischen Akademie
Geometry and Experience: Expanded Edition of the Celebratory Lecture Given at the Prussian Academy§
Springer Verlag (Berlin)
General relativity.[304] The original paper is found as (journal) publication #148. French, English and Italian translations are listed as publications #144, 152, and 153. An undated Polish translation, Geometrja a doswiadczenie, was published in Lviv.
Schilpp 156
1922
Vier Vorlesungen über Relativitätstheorie, gehalten im Mai 1921, an der Universität Princeton
Four Lectures on Relativity Theory, Given in May 1921 at Princeton University§
Statistical mechanics. A re-issue of publications #8, 11, 12, 22, and 26 with notes and derivations from the editor, R. Fürth. Released as Nr. 199 of Oswalds Klassiker der exacten Wissenschaften. An English translation appeared as publication #198.
Schilpp 168
1923
Grundgedanken und Probleme der Relativitätstheorie
Fundamental Ideas and Problems of Relativity Theory§
Special and general relativity.[305] Nobel prize lecture, delivered before the Nordische Naturforscherversammlung in Göteborg. Reprinted in Nobelstiftelsen, Les prix Nobel en 1921–22.
Les fondements de la théorie de la relativité générale
Foundations of the General Theory of Relativity§
Hermann (Paris)
General relativity. French translations of publications #89 and 251 by Maurice Solovine, together with a new essay by Einstein, "Sur la structure cosmologique de l'espace", which discusses the cosmological implications of general relativity, together with its historical antecedents.
Special and general relativity.[308] Second edition of publication #142, with a long appendix covering various topics such as the cosmological implications of general relativity. The appendix was translated by Ernst G. Straus. A "third edition" was published in 1946 by Methuen (London), but it is identical except for a change in pagination. The true third, fourth and fifth editions appeared in 1950, 1953 and 1956, respectively. In the 3rd, Einstein added Appendix II on a generalized theory of gravitation, which was substantially revised for the fifth and final edition.
Authorized translations
The following translations of his work were authorized by Einstein.
Special and general relativity. Authorized translation of the 5th German edition of Ueber die spezielle und die allgemeine Relativitaetstheorie, gemeinverstaendlich (cf. publications #102, 110, 129). The text also includes Dr. Lawson's biographical sketch of Albert Einstein, a short bibliography on relativity theory and an appendix written for this edition entitled "Experimental confirmation of the general theory of relativity". Up to 10 editions were published by Methuen, the last in 1931.
Special and general relativity. Effectively the same as publication #130. Later imprints were Smith (New York, 1931) and Hartsdale House, Inc. (New York, 1947).
Special and general relativity.[310] Reprinted in 1922 and 1923. Also released in 1922 and 1924 under the imprint Methuen (London). Translations are found in publications #166, 167, and 179, whereas the German text is listed as publication #156. A second edition was also released; see publication #297.
Schilpp 144
1921
La géometrie et l'expérience
Maurice Solovine
Gauthier (Paris)
General relativity. French translation of publication #143. A second edition was also published by Gauthier in 1934.
Sidelights on Relativity: I. Ether and Relativity. II. Geometry and Experience
GB Jeffrey and W Perrett
Methuen (London)
Special and general relativity. Translation of publications #131 and 143. Republished in 1923 by Dutton (New York) imprint. The second part, Geometry and Experience, was published separately in 1947 as chapter 8 of Methods of the sciences from the Chicago University.
Schilpp 153
1922
Prospettive Relativistiche dell'Etere e della Geometria
^ abcdThese Index numbers are taken from: 1. Schilpp reference cited in the Bibliography, pp. 694–730. 2. The Collected Papers of Albert Einstein published by Princeton University Press, which are indicated by a CP in italic type, the volume number in boldface type, and by the article number within that volume. 3. Albert Einstein: A Bibliography of His Scientific Papers, 1901–1954, by Ernst Weil, which are indicated by "Weil #" where # is the article number within that reference. A “principal work” is marked by an asterisk (*), for example, Weil *235.
^ abcdThe translations of article titles are generally taken from the published volumes of Einstein's collected papers. For some articles, however, such official translations are not available; unofficial translations are indicated with a § superscript.
^The volume number is given in boldface type. Terms such as "ser. 4" in the journal name refer to the series of the journal, which is a grouping of volumes. For example, a journal may appear in yearly volumes for 60 years (volumes 1–60), then start its volume numbering anew in a second series.
^ abcdThe subject classification of Einstein's articles are the first item, and are indicated in boldface type. Any co-authors are always indicated by the second item.
References
The following references are drawn from Abraham Pais' biography of Albert Einstein, Subtle is the Lord; see the Bibliography for a complete reference.
^Muhlfelder, B., Mac Keiser, G., and Turneaure, J., Gravity Probe B Experiment Error, poster L1.00027 presented at the American Physical Society (APS) meeting in Jacksonville, Florida, on April 14–17, 2007, 2007.
^Isaacson, Walter (2007). "Chapter Eleven: Einstein's Universe". Einstein: His Life and Universe. New York: Simon & Schuster. pp. 250–1. ISBN978-0-7432-6473-0.
^Landau, Elizabeth (April 10, 2019). "Black Hole Image Makes History". Jet Propulsion Laboratory, California Institute of Technology. Retrieved May 17, 2023.
^ abWill, Clifford (2016). "Did Einstein Get It Right? A Centennial Assessment". Proceedings of the American Philosophical Society. 161 (1): 18–30. JSTOR45211536.
^Knudson SK (2006). "The Old Quantum Theory for H2+: Some Chemical Implications". Journal of Chemical Education. 83 (3): 464–472. Bibcode:2006JChEd..83..464K. doi:10.1021/ed083p464. Strand MP, Reinhardt WP (1979). "Semiclassical quantization of the low lying electronic states of H2+". Journal of Chemical Physics. 70 (8): 3812–3827. Bibcode:1979JChPh..70.3812S. doi:10.1063/1.437932.
Einstein, Albert (1989). The Collected Papers of Albert Einstein, Volume 2: The Swiss Years: Writings, 1900–1909 (English translation supplement; translated by Anna Beck, with Peter Havas, consultant ed.). Princeton, New Jersey: Princeton University Press. ISBN978-0-691-08549-4.
Einstein, Albert (1994). The Collected Papers of Albert Einstein, Volume 3: The Swiss Years: Writings, 1909–1911 (English translation supplement; translated by Anna Beck, with Don Howard, consultant ed.). Princeton, New Jersey: Princeton University Press. ISBN978-0-691-10250-4.
Einstein, Albert (1996). The Collected Papers of Albert Einstein, Volume 4: The Swiss Years: Writings, 1912–1914 (English translation supplement; translated by Anna Beck, with Don Howard, consultant ed.). Princeton, New Jersey: Princeton University Press. ISBN978-0-691-02610-7.
Einstein, Albert (1997). The Collected Papers of Albert Einstein, Volume 6: The Berlin Years: Writings, 1914–1917 (English translation supplement; translated by Alfred Engel, with Engelbert Schucking, consultant ed.). Princeton, New Jersey: Princeton University Press. ISBN978-0-691-01734-1.
Einstein, Albert (2002). The Collected Papers of Albert Einstein, Volume 7: The Berlin Years: Writings, 1918–1921 (English translation supplement; translated by Alfred Engel, with Engelbert Schucking, consultant ed.). Princeton, New Jersey: Princeton University Press. ISBN978-0-691-05718-7.
Schilpp, Paul Arthur, ed. (1951). Albert Einstein: Philosopher-Scientist, Volume II. New York: Harper and Brothers Publishers (Harper Torchbook edition).