Einstein

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EINSTEIN, ALBERT - EINSTEINS FOURTH PAPERBiblio.com

Eine Theorie der Grundlagen der Thermodynamik;

1903ref. 47072Leipzig Johann Ambrosius Barth 1903. Contemp. hcloth. Handwritten paperlabel on spine. In: "Annalen der Physik. Vierte Folge. Band 11. Herausgegeben von Paul Drude.". VIII1144pp. and 6 plates. Entire volume offered. The Einstein paper: pp. 170-187. Faint signs of dampstains in outer margins on a few leaves. First edition of Einsteins fourth paper. In his paper from 1902 Einstein "says in his introduction that nobody has yet succeeded in deriving the conditions of thermal equilibrium and of the second law of thermodynamics from probability considerations although Maxwell and Boltzmann came near to it. Willard Gibbs is not mentioned. In fact Einstein's paper was written in ignorance of Gibbs paper published 1901. In the present paper Einstein builds the theory on another basis not used by Gibbs namely on the consideration of a single system in course of time later called "Zeit-Gesamtheit" time assembly and proves that this is equivalent to a certain virtual assembly of many systems Gibb's micro-canonical assembly.Einstein at once proceeded to apply his theorems to a case of utmost importance namely to systems of a size suited for demonstrating the reality of molecules and the correctness of the kinetic theory of matter."Walter Alicke. First edition of Einsteins fourth paper. In his paper from 1902 Einstein "says in his introduction that nobody has yet succeeded in deriving the conditions of thermal equilibrium and of the second law of thermodynamics from probability considerations although Maxwell and Boltzmann came near to it. Willard Gibbs is not mentioned. In fact Einstein's paper was written in ignorance of Gibbs paper published 1901. In the present paper Einstein builds the theory on another basis not used by Gibbs namely on the consideration of a single system in course of time later called "Zeit-Gesamtheit" time assembly and proves that this is equivalent to a certain virtual assembly of many systems Gibb's micro-canonical assembly.Einstein at once proceeded to apply his theorems to a case of utmost importance namely to systems of a size suited for demonstrating the reality of molecules and the correctness of the kinetic theory of matter."Walter Alicke. - Weil No. 4 - Boni No 4. hardcover

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EINSTEIN, ALBERT (+) L HOPFBiblio.com

Über einen Satz der Wahrscheinlichkeitsrechnung und seine Anwendung in der Strahlentheorie. Statistische Untersuchung der Bewegung eines Resonators in einem Strahlungsfeld Theorie der Opaleszenz von hogenen Flüssigkeitsgemischen in der Nähe de.

1910ref. 49714Leipzig Barth 1910. 8vo. Bound in contemporary half cloth with gilt lettering to spine. In "Annalen der Physik" Bd. 33 1910. Entire volume offered. Library stamp to verso of title page light wear to extremities. Otherwise fine and clean. pp. 1096-1104 and pp. 1105-1115; Pp. 1275-1298 Entire volume: VIII 1584 pp. 6 plates. First appearance of all three papers. The purpose of "A theorem in probability and its application in the Theory of radiation" is to demonstrate that the failure of statistical mechanics with respect to the radiation law Rayleigh - Jeans law contradicted by experience cannot be removed by the conjecture that perhaps the individual statistical events should not follow the usual law of independence product of probabilities instead of assuming a certain interdependence between them. Lanczos. The second paper "Statistical investigation on of the motion of an oscillator in a radiation field" makes use of the results of the previous investigation. Einstein's aim is to demonstrate that the Rayleigh-jeans law of radiation contracdicted by the physical facts is an unavoidable consequence of statistics even if we avoid any kind of assumption which may be suspected of needing correction. Lanczos. The third paper "Theory of the opalescence of homogenous fluids and fluid mixtures near the critical state" is an importent investigation and one of the most difficult of all his papers to understand. The aim of the paper is to complement the work of Smoluchovski Ann. d. Physik25 1908 who gave a general explanation of the strong density fluctuations - and the opalescence thus generated - of two fluids near the critical state of mixture or a single fluid near the critical state of condensation on the basis of the kinetic theory of heat. he did notgive howeverthe quantitative details concerning the scattered light associated with this phenomenon. Lanczos. - Weil Nos 34 35 and 36 with an asterix denoting major work.Weil No. 34 35 & 36. hardcover

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EINSTEIN, ALBERTBiblio.com

Einheitliche Feldtheorie von Gravitation und Elektrizität Neue Möglichkeit für eine einheitliche Feldtheorie von Gravitation und Elektrizität Zur einheitlichen Feldtheorie Einheitliche Feldtheorie und Hamiltonsches Prinzip Über den ge. - PMM 416 - A NEW THEORY OF GRAVITATION

1925ref. 52559Berlin Königlich Akademie der Wissenschaften 1925-1929. 1. Einheitliche Feldtheorie von Gravitation und Elektrizität. Offprint: S. B. preuss. Akad. Wiss. 1925 pp.414-419. Original wrappers. Mint. Weil 147 / Boni 155.2. Neue Möglichkeit für eine einheitliche Feldtheorie von Gravitation und Elektrizität. Offprint: S. B. preuss. Akad. Wiss. 1928 pp.235-245. Original wrappers. Mint. Weil 162/ Boni 175.3. Zur einheitlichen Feldtheorie. Offprint: S. B. preuss. Akad. Wiss. 1929 pp.2-7. Original wrappers. Mint. Weil 165/ Boni 183.4. Einheitliche Feldtheorie und Hamiltonsches Prinzip. Offprint: S. B. preuss. Akad. Wiss. 1929 pp.156-159. Original wrappers. Mint. Weil 166/ Boni 184.5. Über den gegenwärtigen Stand der Feldtheorie. In: Festschrift Dr. A. Stodola Zürich Füssli 1929 pp.126-132. Publishers full cloth. Spine slightly faded. Otherwise mint. Weil 168 / Boni 178.All in all a very fine set. Offprint of all four papers and first edition of the final essay constituting Einstein's attempt toward creating a unified field theory: "a new theory of space with a view to unification of all forms of activity that fall within the sphere of physics giving them a common explanation" PMM416. The task of unifying nuclear electromagnetic and gravitational force is nowadays by many considered the holy grail of theoretical physics.Maxwell was the first to develop such a theory when he described the forces of electricity and magnetism as the single force electromagnetism. After Einstein had completed his general theory of relativity a field theory for gravitation he turned his attention towards generalizing his theory even further to include Maxwell's theory. Even though Einstein never succeeded in completing this task in the way that he finished his earlier theories he pioneered and explored many areas of this subject. "It had been repeatedly observed that Einstein's general theory of relativity necessitated a pluralistic explanation of the universe. In 1925 he announced that he had resolved this difficulty but the announcement was premature. In 1928 he attacked the problem once more only to find that Riemann's conception of space on which the general theory was based would not permit of a common explanation of electromagnetic and gravitational phenomena. In a series of papers the present devoted to the development of 'A Uniform Theory of Gravitation and Electricity' he outlined a new theory of space with a view to unification of all forms of activity that fall within the sphere of physics giving them a common explanation. All that would then remain to complete a scientific unison is the correlation of the organic and inorganic".PMM 416Barchas 586 hardcover

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EINSTEIN, ALBERT - THE FIRST EXPLICIT STATEMENT OF THE ENERGY-MASS EQUATION !!Biblio.com

Über die vom Relativitätsprincip geforderte Trägheit der Energie. On the Inertia of Energy Required by the Relativity Principle.

1907ref. 53408Leibzig Johann Ambrosius Barth 1907. 8vo. Contemp. hcalf. Spine gilt and with gilt lettering. Slightly rubbed and light wear to spineends. In "Annalen der Physik" Vierte Folge Band 23. VIII1000 pp. a. 4 plates. The entire volume offered. Einstein's paper: pp.371-384. Stamps on titlepage Allgemeine Electricitäts-Gesellschaft a. AEG Forschungsinstitut. Internally clean. First edition of the first explicit statement of Einstein's energy-mass equation E=mc2.Nearly all descriptions of Einstein's scientific work state that the mass-energy equivalence E=mc2 was first formulated in Einstein's 1907 review paper 'Über das Relativitätsprinzip und die aus demselben gezogenen.' published in 'Jahrbuch der Radioaktivität und Elektronik' see Weil no. 21 and Dictionary of Scientific Biography vol. 4 pp.323 for examples. However in his paper 'Über die von Relativitätsprincip geforderte Trägheit der Energie' the offered paper which predates the former mentioned by six months Einstein gave a clear statement of the mass-energy equivalence E=mc2. See Lanczos: The Einstein Decade pp.149-150 and 153 as well as Volume 2 of 'The Collected Papers of Albert Einstein' pp. 428.Einstein's first paper regarding the relation E=mc2 is his fourth 1905 paper 'Ist die Trägheit eines Körpers von seinem Energieinhalt abhängig'. In this short paper Einstein showed that a body releasing the energy E in the form of radiation will have its mass decreased by E/c2 and concluded that the mass of a body is a measure of its energy content e.g. that all energy has mass. The next time Einstein returns to the subject is in his 1906 paper 'Das Prinzip von der Erhaltung der Schwerpunkts Bewegung und die Trägheit der Energie.'. Here Einstein concluded that one must either ascribe the inertial mass E/c2 to any form of energy E or else give up the fundamental law mechanics regarding conservation of the motion of the center of gravity. Then finally in the 1907 paper 'Über die von Relativitätsprincip geforderte Trägheit der Energie.' the offered paper Einstein makes the decisive step of assuming that all mass has energy. On page 382 Einstein considers the total energy of a moving mass point as the sum of its kinetic energy and its rest energy. In classical mechanics it is most convenient to set the second term to zero but in relativistic mechanics one obtains the simplest expression by setting the rest energy equal to mc2. Einstein then continues to show that this stipulation cannot lead to a contradiction in any relativistic argument. In a footnote on page 382 Einstein states for the first time the equation E=mc2 and mentions that this equation is the expression of the principle of the equivalence of mass and energy - see Volume 2 of 'The Collected Papers of Albert Einstein' pp. 428.The volume contains another paper by Einstein "Bemerkungen zu der Notiz von Hrn. Paul Ehrenfest: "Die Translation deformierbarer Elektronen und der Flächensatz"" pp.206-208. - Weil No. 18. Further with 2 importent papers by Max v. Laue.Collected Works Doc. 45. Weil 19. Boni 19. unknown

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FRIEDMANN, ALEXANDER (+) ALBERT EINSTEINBiblio.com

Über die Krümmung des Raumes Über die Möglichkeit einer Welt mit konstanter negativer Krümmung des Raumes Friedman Bemerkung zu der Arbeit von A. Friedmann "Über die Krümmung des Raumes" Notiz zu der Arbeit von A. Friedmann "Über die Krümm. - THE CURVATURE OF SPACE

1922ref. 49429Berlin Julius Springer 1922-24. 8vo. 4 contemporary half cloth binding: two in uniform half green cloth and two en uniform grey/blue half cloth. In "Zeitschrift für Physik" Bd. 10 11 16 & 21. Entire volumes offered. All volumes with stamp to title page and front free end paper otherwise a fine and clean set. Friedmann: Bd. 10: Pp. 377-386; Bd. 21: P.p. 326-332. Einstein: Bd. 11:P. 326; Bd. 16: P. 228. First printing of these four landmark paper in which Friedman "introduced into cosmology two concepts of revolutionary importance the age og the world and the creation of the world" Kragh Cosmology and Controversy. "In his paper of 1922 Friedmann offered a complete analysis of the solutions of Einstein's cosmological field equations that went beyond the earlier solutions of Einstein and de Sitter as it also included nonstatic solutions. Friedmann did so clearly and explicitly: "The purpose of this note" he wrote "is firstly to show that the cylindrical Einsteinand spherical de Sitter worlds are special cases of more general assumptions and secondly to demonstrate the possibility of a world in which the curvature of space is independent of the three spatial coordinates but does on time".Ibid.In 'Über die Krümmung des Raumes' Friedman derived the non-stationary solutions to Einstein's field equations. Einstein quickly responded in a short comment 'Bemerkung' in which he expressed his suspicion of such a model of the Universe and apparently pointed out an error in Friedman's calculations. However Friedman now wrote a letter to Einstein in which he enclosed his full calculations. Shortly after this Einstein submitted a short notice Notiz in which he admitted that he himself had performed a calculation error and that Friedman's solutions which shed new light on the matter were valid. Friedman's expanding universe model was corroborated by Edwin Hubble's red-shift observations in 1929. In 'Über die Möglichkeit einer Welt mit konstanter negativer Krümmung des Raumes' Friedman derived the Friedman-equations and demonstrated that he had command of all three Friedman-models describing positive zero and negative curvature respectively nearly a decade before the independent discoveries of the same models by Lemaître Robertson and Walker. "Friedmann made a valuable contribution to Einstein's general theory of relativity. As always his interest was not limited simply to familiarizing himself with this new field of science but led to his own remarkable investigations. Friedmann's work on the theory of relativity dealt with one of its most difficult questions the cosmological problem. In his paper "Über die Krümmung des Raumes" 1922 he outlined the fundamental ideas of his cosmology: the supposition concerning the homogeneity of the distribution of matter in space and the consequent homogence of "world" time for which at any moment in time the metrics of space will be identical at all points and in all directions. This theory is especially important because it leads to a sufficiently correct explanation of the fundamental phenomenon known as the "red shift." This solution of the Einstein field equations obtained from the above propositions is the model for any homogeneous and isotropic cosmological theory. It is interesting to note that Einstein thought that the cosmological solution to the equations of a field had to be static and had to lead to a closed model of the universe. Friedmann discarded both conditions and arrived at an independent solution. Einstein welcomed Friedmann's results because they showed the dispensability of the ad hoc cosmological term Einstein had been forced to introduce into the basic field equation of general relativity". DSB. Weil 122 & 130. hardcover

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EINSTEIN, ALBERT - THE PHOTOELECTRIC EQUATIONBiblio.com

Zur Theorie der Lichterzeugung und Lichtsabsorption; withbound: Das princip von der Erhaltung der Schwerpunktsbewegung und die Trägheit der Energie; 2 papers.

1906ref. 46962Leipzig Johann Ambrosius Barth 1906. Bound together in one contemp. halfcalf. Spine gilt. Minor scratches to spine. A stamp to titlepage and htitle. "Annalen der Physik. Vierte Folge. Band 20. Herausgegeben von Paul Drude." Portrait Paul Drude VIII1048 pp. and 6 plates. Einstein papers: pp. 199-206 and 627-33. The entire volume offered. Both papers first edition. It was for the papers "Ueber einen die Erzeugung und Verwandlung des Lichtes betreffenden heuristischen Gesichtspunkt" of 1905 and "Zur Theorie der Lichterzeugung. Theory of light emission and absorption the offered item that Einstein was awarded the Nobel Prize in 1921."The quantum theory has affected virtually every branch of physics. Its earliest and one of its most significant developments was Einstein's application of the theory to what is known as the 'photo-electrical effect'.Einstein explained this effext by suggesting that the classical view that light is emitted in the form of continous waves must be abandoned. The photo-electrical effect could be explained only as an example of quantum action where the waves of light or X-rays are emitted in minute particles or bullets. It is he size of the bullet the wave-lenght of the radiation which determines the number of electrons ejected. It was for this and not for the theory of relativity that Einstein was awarded the Nobel Prize in 1921. Einstein's two fundamental papers on this subject are "Ueber einem Erzeugung." 1905 and Zur Theorie der Lichterzeugung the paper offered here" PMM the note to 391. In the second paper Principle of the conservation of the centre of mass motion and the inertia of energy he shows that the conservation of mass is a special application of his energy principle E= Mc2 - Weil: 12 & 13.Among the many papers in this volume we have Max von Laue: Zur Thermodynamik der Inteferenzerscheinungen. pp. 365-378. unknown

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Einstein

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