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Part 1
The Special Theory of Relativity
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1. Physical Meaning of Geometrical Propositions

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In your schooldays most of you who read this book made acquaintance with the noble building of Euclidās geometry and you remember ā perhaps with more respect than love ā the magnificent structure, on the lofty staircase of which you were chased about for uncounted hours by conscientious teachers. By reason of your past experience, you would certainly regard everyone with disdain who should pronounce even the most out-of-the-way proposition of this science to be untrue. But perhaps this feeling of proud certainty would leave you immediately if someone were to ask you: āWhat, then, do you mean by the assertion that these propositions are true?ā Let us proceed to give this question a little consideration.
Geometry sets out from certain conceptions such as āplaneā, āpointā, and āstraight lineā, with which we are able to associate more or less definite ideas, and from certain simple propositions (axioms) which, in virtue of these ideas, we are inclined to accept as ātrueā. Then, on the basis of a logical process, the justification of which we feel ourselves compelled to admit, all remaining propositions are shown to follow from those axioms, i.e. they are proven. A proposition is then correct (ātrueā) when it has been derived in the recognised manner from the axioms. The question of ātruthā of the individual geometrical propositions is thus reduced to one of the ātruthā of the axioms. Now it has long been known that the last question is not only unanswerable by the methods of geometry, but that it is in itself entirely without meaning. We cannot ask whether it is true that only one straight line goes through two points. We can only say that Euclidean geometry deals with things called āstraight linesā, to each of which is ascribed the property of being uniquely determined by two points situated on it. The concept ātrueā does not tally with the assertions of pure geometry, because by the word ātrueā we are eventually in the habit of designating always the correspondence with a ārealā object; geometry, however, is not concerned with the relation of the ideas involved in it to objects of experience, but only with the logical connection of these ideas among themselves.
It is not difficult to understand why, in spite of this, we feel constrained to call the propositions of geometry ātrueā. Geometrical ideas correspond to more or less exact objects in nature, and these last are undoubtedly the exclusive cause of the genesis of those ideas. Geometry ought to refrain from such a course, in order to give to its structure the largest possible logical unity. The practice, for example, of seeing in a ādistanceā two marked positions on a practically rigid body is something which is lodged deeply in our habit of thought. We are accustomed further to regard three points as being situated on a straight line, if their apparent positions can be made to coincide for observation with one eye, under suitable choice of our place of observation.
If, in pursuance of our habit of thought, we now supplement the propositions of Euclidean geometry by the single proposition that two points on a practically rigid body always correspond to the same distance (line-interval), independently of any changes in position to which we may subject the body, the propositions of Euclidean geometry then resolve themselves into propositions on the possible relative position of practically rigid bodies.1 Geometry, which has been supplemented in this way, is then to be treated as a branch of physics. We can now legitimately ask as to the ātruthā of geometrical propositions interpreted in this way, since we are justified in asking whether these propositions are satisfied for those real things we have associated with the geometrical ideas. In less exact terms we can express this by saying that by the ātruthā of a geometrical proposition in this sense we understand its validity for a construction with rule and compasses.
1. It follows that a natural object is associated also with a straight line. Three points A, B and C on a rigid body thus lie in a straight line when the points A and C being given, B is chosen such that the sum of the distances AB and BC is as short as possible. This incomplete suggestion will suffice for the present purpose.
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Of course the conviction of the ātruthā of geometrical propositions in this sense is founded exclusively on rather incomplete experience. For the present we shall assume the ātruthā of the geometrical propositions, then at a later stage (in the general Theory of Relativity) we shall see that this ātruthā is limited, and we shall consider the extent of its limitation.
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2. The System of Co-ordinates

On the basis of the physical interpretation of distance which has been indicated, we are also in a position to establish the distance between two points on a rigid body by means of measurements. For this purpose we require a ādistanceā (rod S) which is to be used once and for all, and which we employ as a standard measure. If, now, A and B are two points on a rigid body, we can construct the line joining them according to the rules of geometry. Then, starting from A, we can mark off the distance S time after time until we reach B. The number of these operations required is the numerical measure of the distance AB. This is the basis of all measurement of length.2
2. Here we have assumed that there is nothing left over, i.e. that the measurement gives a whole number. This difficulty is got over by the use of divided measuring-rods, the introduction of which does not demand any fundamentally new method.
Every description of the scene of an event or of the position of an object in space is based on the specification of the point on a rigid body (body of reference) with which that event or object coincides. This applies not only to scientific description, but also to everyday life. If I analyse the place specification āTimes Square, New York,ā3 I arrive at the following result. The earth is the rigid body to which the specification of place refers; āTimes Square, New Yorkā is a well-defined point to which a name has been assigned and with which the event coincides in space.4
3. Einstein used āPotsdamer Platz, Berlinā in the original text. In the authorised translation this was supplemented with āTrafalgar Square, Londonā. We have changed this to āTimes Square, New Yorkā, as this is the most well known/identifiable location to English speakers in the present day. [Note by the janitor.]
4. It is not necessary here to investigate further the significance of the expression ācoincidence in spaceā. This conception is sufficiently obvious to ensure that differences of opinion are scarcely likely to arise as to its applicability in practice.
This primitive method of place specification deals only with places on the surface o...
Table of contents
- Preface
- Note to the Fifteenth Edition
- Part 1
- 1. Physical Meaning of Geometrical Propositions
- 2. The System of Co-ordinates
- 3. Space and Time in Classical Mechanics
- 4. The Galileian System of Co-ordinates
- 5. The Principle of Relativity
- 6. The Theorem of the Addition of Velocities Employed in Classical Mechanics
- 7. The Apparent Incompatibility of the Law of Propagation of Light with the Principle of Relativity
- 8. On the Idea of Time in Physics
- 9. The Relativity of Simultaneity
- 10. On the Relativity of the Conception of Distance
- 11. The Lorentz Transformation
- 12. The Behaviour of Measuring Rods and Clocks in Motion
- 13. Theorem of the Addition of Velocities. The Experiment of Fizeau
- 14. The Heuristic Value of the Theory of Relativity
- 15. General Results of the Theory
- 16. Experience and the Special Theory of Relativity
- 17. Minkowskiās Four-Dimensional Space
- Part 2
- 18. Special and General Principle of Relativity
- 19. The Gravitational Field
- 20. The Equality of Inertial and Gravitational Mass as an Argument for the General Postulate of Relativity
- 21. In What Respects are the Foundations of Classical Mechanics and of the Special Theory of Relativity Unsatisfactory?
- 22. A Few Inferences from the General Principle of Relativity
- 23. Behaviour of Clocks and Measuring-Rods on a Rotating Body of Reference
- 24. Euclidean and Non-Euclidean Continuum
- 25. Gaussian Co-ordinates
- 26. The Space-Time Continuum of the Special Theory of Relativity Considered as a Euclidean Continuum
- 27. The Space-Time Continuum of the General Theory of Relativity is not a Euclidean Continuum
- 28. Exact Formulation of the General Principle of Relativity
- 29. The Solution of the Problem of Gravitation on the Basis of the General Principle of Relativity
- Part 3
- 30. Cosmological Difficulties of Newtonās Theory
- 31. The Possibility of a āFiniteā and Yet āUnboundedā Universe
- 32. The Structure of Space According to the General Theory of Relativity
- Appendices
- Appendix I
- Appendix II
- Appendix III
- Appendix IV
- Appendix V
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