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Lecture 4: The Characteristics Of Space A. The Geometry Of The Gravitational Field

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FieldValue
SourceFour Lectures on Relativity and Space
Year1923
Section IDfour-lectures-relativity-space-lecture-04
Locationlines 3595-6820
Statuscandidate
Word Count18408
Equation Candidates In Section66
Figure Candidates In Section8
Quote Candidates In Section0
LECTURE IV THE CHARACTERISTICS OF SPACE A. THE GEOMETRY OF THE GRAVITATIONAL FIELD The starting point of the relativity theory is that the laws of nature, including the velocity of light in empty space, are the same everywhere and with regard to any system to which they may be referred — whether on the revolving platform of the earth or in the speeding railway train or in the space between the fixed stars. From this it follows that the length of a body is not a fixed property of it, but is relative, depending on the conditions of obser- vation— the relative velocity of the observer with regard to the body. It also is shown that the laws of motion of bodies in a gravitational field are identical with the laws of inertial motion with
LECTURE IV THE CHARACTERISTICS OF SPACE A. THE GEOMETRY OF THE GRAVITATIONAL FIELD The starting point of the relativity theory is that the laws of nature, including the velocity of light in empty space, are the same everywhere and with regard to any system to which they may be referred — whether on the revolving platform of the earth or in the speeding r ...
LECTURE IV THE CHARACTERISTICS OF SPACE A. THE GEOMETRY OF THE GRAVITATIONAL FIELD The starting point of the relativity theory is that the laws of nature, including the velocity of light in empty space, are the same everywhere and with regard to any system to which they may be referred — whether on the revolving platform of the earth or in the speeding railway train or in the space between the fixed stars. From this it follows that the length of a body is n ...
... ARACTERISTICS OF SPACE A. THE GEOMETRY OF THE GRAVITATIONAL FIELD The starting point of the relativity theory is that the laws of nature, including the velocity of light in empty space, are the same everywhere and with regard to any system to which they may be referred — whether on the revolving platform of the earth or in the speeding railway train or in the space between the fixed stars. From this it follows that the length of a body is not a fixed property of it, but is relative, depending on the conditions of obser- vation— the relative velocit ...
... e angles are the same, etc. Thus the characteristic constant, or the curvature of the space, remains unchanged by the bending of the space. Euclidean 2-space thus is the plane and any surface made by bending it or a part of it in any desired manner — • into cylinder, cone, wave surface, etc; elliptic 2-space is the sphere and any surface made by bending a piece of the sphere into some other shape, as a spindle; hyperbolic 2-space is the pseudo-sphere — ^not existing in Euclidean 3-space — or any surface which can be considered as made by bending a ...
Concept CandidateHits In SectionStatus
Light26seeded
Ether25seeded
Spectrum2seeded
Velocity of light2seeded
Frequency1seeded
Term CandidateHits In SectionStatus
ether25seeded
Candidate IDOCR / PDF-Text CandidateSource Location
four-lectures-relativity-space-eq-candidate-0105conditions: C = ird, > 7r(iand<7rd.line 3774
four-lectures-relativity-space-eq-candidate-0106analogy with two-dimensional spaces, or 2-spaces. We canline 4176
four-lectures-relativity-space-eq-candidate-0107the same characteristic constant as the elliptic 2-space, theline 4387
four-lectures-relativity-space-eq-candidate-01081 - C/27rr (1)line 4439
four-lectures-relativity-space-eq-candidate-0109diameter, the quantity (1) is not constant, but depends online 4445
four-lectures-relativity-space-eq-candidate-0110/vi = 1/R, (3)line 4501
four-lectures-relativity-space-eq-candidate-0111A% = I/R1R2. (4)line 4526
four-lectures-relativity-space-eq-candidate-0112It can be shown that the characteristic constant (2) ofline 4528
Candidate IDOCR / PDF-Text CandidateSource Location
four-lectures-relativity-space-fig-020R = j/VK. (15) Fig. 20. E. THE STRAIGHT LINE AND THE ELLIPTIC 2-SPACEline 4631
four-lectures-relativity-space-fig-021line between them, as Li or L2 — shown dotted in Fig. 21 — Fig. 21. is longer. Suppose we have a straight line L in the plane Fig. 21 and a point P outside of L. Any line drawn…line 4776
four-lectures-relativity-space-fig-025The mathematical n-space merely is the continuous mani- FiG. 25. fold of oo« elements which are given by the n ratios: x : y :line 5036
four-lectures-relativity-space-fig-029however, are no part of projective geometry, as they are Fig. 29. made by its relation to infinity and therefore are metric in character : The hyperbola has two infinitely dista…line 5667
four-lectures-relativity-space-fig-030with regard to a conic, then the line connecting the points Fig. 30. pi and P2 is the polar of the point of intersection of Pi andline 5703
four-lectures-relativity-space-fig-031of these six lines by e = ah, cd;f = ac, hd; g = ad, he, and Fig. 31. draw the three additional lines ef, eg and fg, we get a total of nine lines and four points on each of thes…line 5727
four-lectures-relativity-space-fig-032tant (that is, very far distant) we thus recognize by the Fig. 32. two lines of sight from our eyes to the object having the same direction.line 6025
four-lectures-relativity-space-fig-033parallels Li and Lo through a point P — that is, two lines Fig. 33. which intersect L at infinity — and these tvv^o parallels Li and L2 make an angle L1PL2 with each other. Thus L]line 6078
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