Space, Time and Gravitation: An Outline of the General Relativity Theory

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Cambridge University Press, 1987/02/26 - 218 ページ
This classic book is essential reading for all those interested in the development of modern physics. Sir Arthur Eddington's account of the general theory of relativity, 'without,' as he says in his preface, 'introducing anything very technical in the way of mathematics, physics or philosophy', was first published in the exciting days of 1920 soon after the first objective tests of the theory had demonstrated its validity. The book was at once received with acclamation by reviewers and remains today one of the simplest and most straightforward accounts in print. The reviewer in the Athenaeum described it as 'a masterly book. The arrangement, the vigour and ease of the reasoning, the felicity of illustration, the clear, flexible prose and (we must mention it) the wit, make this book one of the most adequate and engaging attempts at the non-technical exposition of a scientific theory that it has ever been our good fortune to encounter.' This reissue includes a foreword by Sir Hermann Bondi, FRS, giving a brief appraisal of the book, and placing it in its historical and scientific context.
 

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THE FITZGERALD CONTRACTION
17
RELATIVITY
30
THE WORLD OF FOUR DIMENSIONS
45
FIELDS OF FORCE
63
KINDS OF SPACE
77
THE NEW LAW OF GRAVITATION AND THE OLD LAW
93
WEIGHING LIGHT
110
OTHER TESTS OF THE THEORY
123
MOMENTUM AND ENERGY
136
TOWARDS INFINITY
152
ELECTRICITY AND GRAVITATION
167
ON THE NATURE OF THINGS
180
MATHEMATICAL NOTES
202
HISTORICAL NOTE
210
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v ページ - Rather admire; or if they list to try Conjecture, he his fabric of the Heavens Hath left to their disputes, perhaps to move His laughter at their quaint opinions wide Hereafter, when they come to model Heaven And calculate the stars, how they will wield The mighty frame; how build, unbuild, contrive To save appearances; how gird the sphere With centric and eccentric scribbled o'er, Cycle and epicycle, orb in orb...
14 ページ - Thus mathematics may be defined as the subject in which we never know what we are talking about, nor whether what we are saying is true.
9 ページ - Lobatchewsky's geometry is true, the parallax of a very distant star will be finite. If Riemann's is true, it will be negative. These are results which seem within the reach of experiment, and it is hoped that astronomical observations may enable us to decide between the two geometries.

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