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Meaning of Relativity (Princeton Science Library)
 
 
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Meaning of Relativity (Princeton Science Library) [Englisch] [Taschenbuch]

Albert Einstein , Brian Greene
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Taschenbuch, 17. September 1992 --  

Produktinformation

  • Taschenbuch: 176 Seiten
  • Verlag: Princeton University Press; Auflage: Reissue (17. September 1992)
  • Sprache: Englisch
  • ISBN-10: 0691023522
  • ISBN-13: 978-0691023526
  • Größe und/oder Gewicht: 20,2 x 12,7 x 1,2 cm
  • Durchschnittliche Kundenbewertung: 5.0 von 5 Sternen  Alle Rezensionen anzeigen (2 Kundenrezensionen)
  • Amazon Bestseller-Rang: Nr. 1.016.617 in Englische Bücher (Siehe Top 100 in Englische Bücher)
  • Komplettes Inhaltsverzeichnis ansehen

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Albert Einstein
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Produktbeschreibungen

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In 1921, a young Albert Einstein travelled to America to give four lectures at Princeton University, paving the way for a more complete acceptance of his theory of general relativity. These lectures are published together as The Meaning of Relativity, and were revised with each new edition until Einstein's death. Despite Einstein's profession that he thought without using words, his examples and descriptions of the relativistic world he perceived are clear and easy to follow. Unfortunately for non-technical readers, his presentation requires deep diversions into mathematics often enough to break up the flow of his narrative and they may find this rough terrain. But for the mathematically sophisticated or the devoted scientific historian, these lectures are profoundly illuminating-- Einstein's bright, quiet genius shines through in the simplicity and economy of his writing. Two appendices follow the lectures: The first covers advances and experimental verifications after 1921; the second, "Relativistic theory of the non-symmetric field", was Einstein's last scientific paper. The Meaning of Relativity documents a revolution in progress and yields to the careful student deeper truths than those found in physics textbooks. --Rob Lightner, Amazon.com

Amazon.com

In 1921, a young Albert Einstein traveled to America to give four lectures at Princeton University, paving the way for a more complete acceptance of his theory of general relativity. These lectures are published together as The Meaning of Relativity, and were revised with each new edition until Einstein's death. Despite Einstein's profession that he thought without using words, his examples and descriptions of the relativistic world he perceived are clear and easy to follow. Unfortunately for nontechnical readers, his presentation requires deep diversions into mathematics often enough to break up the flow of his narrative, and they may find this rough terrain. But for the mathematically sophisticated or the devoted scientific historian, these lectures are profoundly illuminating--Einstein's bright, quiet genius shines through in the simplicity and economy of his writing. Two appendices follow the lectures: the first covers advances and experimental verifications after 1921; the second, "Relativistic Theory of the Non-Symmetric Field," was Einstein's last scientific paper. The Meaning of Relativity documents a revolution in progress and yields to the careful student deeper truths than those found in physics textbooks. --Rob Lightner

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THE theory of relativity is intimately connected with the theory of space and time. Lesen Sie die erste Seite
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Format:Taschenbuch
In this presentation Einstein communicated a remarkable set of identities for the equation of motion, obtaining on page 102 or so a form like F = m[ E + (v x B)] + higher-order_terms for GR's geodesic equation of motion. The electromagnetic- like nature of the motion is quite evident in this Lorentz-force type of equation. Einstein complexified it a bit by using identities like E = - grad(phi) - dA/dt and B = curl A, but there it was, really a monument to his powers of analysis. However, in general relativity, we then have B four times too strong, which leads to a violation of the equation of continuity prominently featuring the factor of 4 as the problem term. This is the basis of my first non-self-consistency theorem for classical general relativity, the so-called 1st overthrow theorem. I have also been able to show that the problem comes up again when exact solutions are used, in particular, when the Kerr metric is employed. Einstein's solution in Cartesian coordinates is very useful not only for general relativity's overthrow, but for figuring out the kind of a theory most likely to succeed. Apart from the factor of 4, the linearized solutions look like Maxwell's equations for the electromagnetic field with the source-coupling reversed for like-charges-attract fields with consequently left-hand rule symmetry. They are mirror-image Maxwell's equations. A study of the electroweak model in Cottingham and Greenwood's INTRODUCTION TO NUCLEAR

PHYSICS suggested that a generalization of elementary particle theory's vector-boson field equations could contain all forces in local coordinates, including gravitation, electromagnetism, and the nuclear forces. This approach to unified field theory, which emphasizes the local validity of special relativity and the wave-operator identities of quantum mechanics, provides the right answers if we include the principle of equivilance in a way that produces gravitational time-dialation only, for the synchronization of clocks. This approach is far more direct with respect to the derivation of field equations than Einstein's, and produces a superbly unified picture of force field theory firmly grounded on conservative assumptions. Classical GR effects of higher-order can be derived from this theory. For details, see GRAVITATION & THE ELECTROFORM MODEL by James A. Green and THERMONUCLEAR FUSION IN STARS, also by James A. Green.

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Von Ein Kunde
Format:Taschenbuch
The first half (special relativity) is an exelent resource for beginners on relativity who heve a confident handle of real variable and vector differetial calculus. The seconth half is an introductory text on Generla Relativity which is good. For this part is necesary to have also handle of differential geometry, and I recomend you to read before the article "Space and Time" by H. Minkowski in which some how the conection between the mathematical background (diff. geom.) and the physical theory is set. --- Enrique Castro Student of Physics (National University of México)---
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41 von 44 Kunden fanden die folgende Rezension hilfreich
Will never collect dust.... 2. Februar 2002
Von Dr. Lee D. Carlson - Veröffentlicht auf Amazon.com
Format:Taschenbuch
There are numerous books on general relativity currently on the market, and these range in difficulty from those written for the beginner or the layman, those written for graduate students in physics, and research monographs covering specialized topics. It is always refreshing to go back to the originator of the subject, and take part in his special insights on the topic. Philosophers and historians of science can definitely benefit from a perusal of this book.

The author begins this book with a discussion of the origin of the concepts of space-time, the emphasis being partly philosophical and partly psychological, and the reader can see the origin of the author's operationalism in reading this introduction. He is clearly against the philosophers who attempt to remove concepts from experience and put them in his words "in the intangible heights of the a priori". The motion of rigid bodies is used to set up a discussion of Euclidean geometry and linear orthogonal transformations. The author emphasizes the role of the physicist in discerning whether a system of geometry is true or not, contrary to the pure mathematician. Examples of geometrical invariants, such as the Cartesian line element and the volume element are discussed, along with the role of vectors and tensors. Both of these are used as means by which one can give expression to the independence of Cartesian coordinates. Maxwell's equations are put in tensor notation as an example of covariance with respect to Cartesian coordinate transformations. All of this is done to motivate the theories of special and general relativity.

The theory of spectial relativity is treated in chapter 2, the author introducing his famous principle of special relativity. The author poses the problem of calculating the coordinates and time in an inertial system moving with uniform translation relative to another. He shows how this problem is solved by assuming that time and space are absolute, and if the coordinate axes of the systems are parallel to one another, the Galilean transformations result. Newton's equations of motion are covariant under these transformations, but Maxwell equations are not (but the author chooses not to show this explicitly). He then gives an in-depth discussion of how the Lorentz transformations arise as being those that guarantee the covariance of the Maxwell equations. The author also discusses the signature of the Lorentz metric and how it is related to the light cone. He ends the chapter by developing the energy tensor of the electromagnetic field and matter.

The author's rejection of inertial frames as being priveleged leads him in the beginning of the next chapter to a short philosophical critique of the principle of inertia. This leads to a discussion of the principle of equivalence and to the origin of the general theory of relativity, a theory which the author developed, amazingly, single-handedly, and which he clearly believes is very much superior to classical mechanics. The intuition to be gained by reading this chapter is invaluable for serious students of general relativity. One can see the simplicity and power of the author's arguments, relying on keen physical intuition and sound use of mathematics. In particular, the author's heuristic derivation of the gravitational field equations from Poisson's equation is briliant. In addition, he is not ashamed to interject philosophical argumentation into his writing, particularly in his discussion of Mach's principle. Such discussions are becoming more rare among physicists at the present time.

16 von 18 Kunden fanden die folgende Rezension hilfreich
Good reference on medium level Relativity 11. Juni 1999
Von Ein Kunde - Veröffentlicht auf Amazon.com
Format:Taschenbuch
The first half (special relativity) is an exelent resource for beginners on relativity who heve a confident handle of real variable and vector differetial calculus. The seconth half is an introductory text on Generla Relativity which is good. For this part is necesary to have also handle of differential geometry, and I recomend you to read before the article "Space and Time" by H. Minkowski in which some how the conection between the mathematical background (diff. geom.) and the physical theory is set. --- Enrique Castro Student of Physics (National University of México)---
25 von 31 Kunden fanden die folgende Rezension hilfreich
Einstein goes deeper. 27. Dezember 2001
Von henrique fleming - Veröffentlicht auf Amazon.com
Format:Taschenbuch
The Meaning of Relativity is an advanced book. The title should have made it clear. Einstein delves here into what his theory
actually MEANS. That is, what must we change (if anything...) in our world conception, in the way we think, as a consequence of his immense discovery. Just think that he meddled with time, a concept static since so long that it is registered deep in our DNA: our concept of time goes back to the epoch where our main purpose was to survive the day
(sounds familiar? No, no, it was different! It was permanent. What you experience now is transient...)
So what? Read it! It is a marvellous book. Perhaps you will have to reach for other, more elementary, books, in this enterprise. All right! That almost characterizes a book worth reading. So... go on! It will repay your efforts. It IS doable. You will come out, for instance, with a precise CONSTRUCTION OF SPACE! Your brains will be enriched.You deserve that!
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