Aperçu avant impression Fermer

Affichage de 158 résultats

Description archivistique
30 résultats avec objets numériques Afficher les résultats avec des objets numériques
EDDN/A/4/9 · Pièce · 21 June and 2 July 1919
Fait partie de Papers of Sir Arthur Eddington

Transcript

S.S. “Zaire”
1919 June 21

My very dear Mother

I will write a little to tell you about the rest of my experiences in Principe; but it is doubtful if you will receive this before I arrive. I have only had two letters from you—the second written about March 28 reached me about May 11. Since then there have been no mails from Europe, and in fact we expect to pass tomorrow (at S. Vincent) the outward boat which will be taking the next batch of letters to Principe.

We stayed just a week at Sundy on our first visit, then returned to S. Antonio for a week, and finally returned to Sundy on May 13 and stayed there until our steamer sailed on June 12. Nothing much happened during the week at S. Antonio except that most afternoons we played tennis, generally with the Curador and Judge.

We were ready to take the first photographs about May 16, and as the nights were generally clear we had no difficulty in getting the check photographs. These had to be taken between 12∙30 and 1 a.m; we took them on three different nights. The developing also had to be done at night and, owing to the special difficulties due to the high temperature of the water (78°), was a slow business. So we were often up pretty late during this period. In the day time I had a good deal of work measuring these check photographs.

The last heavy rain fell about May 9 and shortly afterwards the Gravana or cool season began. There was practically no rain, but a good deal of cloud in the day-time, and the conditions seemed rather less favourable for the eclipse than during the rainy season. However there were a number of beautifully clear days, and usually at least part of the day was clear. The two days before the eclipse were about the most unfavourable we had.

On the morning of the eclipse Mr Carneiro, the Curador, Judge, Mr Wright and three Doctors came over. Just as they arrived a tremendous rain-storm came on, the heaviest we have seen. It was most unusual at that time of the year; but it was favourable for the eclipse as it helped to clear the sky. The rain stopped about no[o]n (the eclipse was at 2∙15). There were a few gleams of sunshine after the rain, but it soon clouded over again. About 1∙30 when the partial phase was well advanced, we began to get glimpses of the sun, at 1∙55 we could see the crescent (through cloud) almost continuously, and there were large patches of clear sky appearing. We had to carry out our programme of photographs in faith. I did not see the eclipse, being too busy changing plates, except for one glance to make sure it had begun, and another half-way through to see how much cloud there was. We took 16 photographs (of which 4 are not yet developed). They are all good pictures of the sun, showing a very remarkable prominence; but the cloud has interfered very much with the star-images. The first 10 photographs show practically no stars. The last 6 show a few images which I hope will give us what we need; but it is very disappointing. Everything shows that our arrangements were quite satisfactory, and with a little clearer weather we should have got splendid results. Ten minutes after the eclipse the sky was beautifully clear, but it soon clouded again.

We developed the photographs 2 each night for 6 nights after the eclipse, and I spent the whole day measuring. The cloudy weather upset my plans and I had to treat the measures in a different way from what I had intended; consequently I have not been able to make any preliminary announcements of the result. But the one good plate that I measured gave a result agreeing with Einstein and I think I have got a little confirmation from a second plate.

We had a number of excursions to different places on the island chiefly on Sundays. We had a monkey-hunting expedition, but did not see any except in the distance. We were singularly unfortunate in not seeing monkeys because there are enormous crowds of them about and numbers of men are employed simply in scaring them away from the cocoa. Another interesting expedition was to Lola, a dependency of Sundy where there was a specially fine crop of cocoa. It was a very fine sight to see the large golden pods in such numbers—almost as though the forest had been hung with Chinese lanterns.

Another day we went to Lapa in the estate of the Sociedade Agricultura Colonial and had lunch on the beach off fish which we watched being caught. Lapa is a very beautiful spot at the foot of a fine sugar-loaf mountain. All the beaches are very pretty—a strip of golden sand between the cocoanut palms and the blue sea. I had a good bathe at Lapa—the only time in Principe,—a black man went with me to see that I did not go too near the sharks.

Another time we went to near Bombom to see the ruins of the palace of Marie Corelli (that was not quite her name, but it was something very near it). She was a famous slave dealer about ninety years ago. Her palace on the beach is all in ruins but it must have been a huge place. Her church is there also—quite a fine ruin.

We liked Mr Atalia immensely. He was very lively and amusing and extremely good to us in every way. After dinner we used to sit out in front of the house and there was generally a succession of natives came up to interview him on all sorts of matters. They evidently have great respect and confidence in him.

We had to return by this boat the “Zaire” (although it was rather earlier than I liked) because there will not be another boat leaving Principe until about August 1. There has been a dispute between the company and the government about passage rates, and no boats have left Lisbon for a long while. This boat is tremendously crowded and we should not have got a passage on it; but for the help of the Governor who managed to get places commandeered for us.

I got a bit of fever two days before starting (otherwise I have had splendid health all the time) and was feeling rather bad when I got on board but the sea-air has soon set me right again. It left me a bit weak for the first three or four days—in fact I fainted one night—but it has quite gone now.

Mr. Carneiro is on the ship—returning to Portugal for three months. There are also 4 English missionaries from Angola. They knew about us from Mrs Williams the missionary we met on the Portugal. One of them Mrs Stober is a friend (a Williamson of Cockermouth) related to John Hall. Her husband (who is not a Friend) is a very nice fellow; he was the founder of the mission.

It has been a little rougher this voyage than when we came out; but nothing to speak of. Of course, a lot of passengers have been ill; it is very bad for them being so crowded on the boat. There are lots of children and in some cabins there are as many as seven people. There are three in our cabin—a Portuguese and Cottingham & myself.

We reached Praia last night after 8¼ days from Principe. This is a slow boat and I do not expect we shall reach Lisbon until June 30.

We were very delighted to receive a telegram from Dyson saying that the Brazil party had been successful; we often wondered how they were getting on.

I suppose I shall be back about July 10. I shall look forward to the strawberries, which are better than anything they have in the tropics.

With very dear love to both
Your affectionate son
Stanley

Lisbon, July 2. I expect we shall reach Liverpool about July 15 by R.M.S.P. Line. Ships very crowded and scarce.

—————

The postscript was written in pencil. Two passages have been marked off in pencil by a later hand.

EDDN/A/5/1 · Pièce · 9 Nov. 1909
Fait partie de Papers of Sir Arthur Eddington

Transcript

Victoria Park, Manchester
Novr 9. 1909

Dear Mr Eddington,

May I ask you—in confidence—whether you consider yourself definitely fixed to “Astronomy” or whether you would at all consider a return to Physics as possible.—I am not at liberty to go into details but the question arises whether in case a chair of Theoretical Physics were founded here or elsewhere and suitable conditions were offered you would be prepared to accept the chair.—Also in that case it might help matters if you wd let me know what conditions you would consider acceptable.

You may take it for granted that the duties wd leave you plenty of time for private work and that nothing wd prevent you continuing to prosecute the line of research on which you have entered with such success

I remain
Yours sincerely
Arthur Schuster.

EDDN/A/5/2 · Pièce · 15 Nov. 1909
Fait partie de Papers of Sir Arthur Eddington

Transcript

(copy)

Royal Observatory, Greenwich, London, S.E.
1909 Nov. 15

Dear Dr. Schuster

You will, I am sure, not be surprised that I have delayed a little replying to your important letter. I had not at all thought of such a change, and it was a matter requiring very careful consideration. Whilst the idea of returning to Physics, and perhaps especially to academic work, was in many respects attractive, I have however decided that it is best for me not to leave my present work. I need not trouble you with the reasons that have led me to this difficult decision; rightly or wrongly I have concluded that the suggestion and opportunities that I meet with in a large observatory are more likely to lead to good research work on my part {1} than any I could hope for elsewhere.

With many thanks
yours sincerely
A. S. Eddington

—————

The letter is headed ‘copy’ but, since it contains a correction, it is probably a draft.

{1} ‘the suggestion …. on my part’ has been altered from ‘the suggestion and opportunities of research work that I meet with in a large observatory are more likely to lead to good results on my part’.

EDDN/A/5/3 · Pièce · 21 May 1936
Fait partie de Papers of Sir Arthur Eddington

Transcript

Observatory, Cambridge
21 May 1936

Dr W. M. Smart’s application for the Chair of Regius Professor of Astronomy in the University of Glasgow has my warmest support. He is a man of established reputation in astronomical circles who would fill the office with distinction; and he has proved himself very successful as a lecturer and teacher. He would be much missed from this Observatory and from the University; but promotion to a professorial chair would be a fitting recognition of his work.

Dr Smart has been Chief Assistant in the Observatory and John Couch Adams Astronomer since 1921. There is only one other Assistant. The policy of the Observatory has been to avoid routine undertakings and to develop new methods. Two main lines of work have been developed during his tenure—an improved method of determining photographic proper motions of stars, and measurement of stellar magnitudes with a photo-electric cell. As regards the former it may, I think, be claimed that the Cambridge results set a new standard of accuracy for large series of proper motions. Photo-electric work is still confined to two or three observatories (Cambridge being the only British one). After a long struggle with pioneer difficulties the work is now proceeding with great success, and astonishing accuracy is obtained. A large share of the credit for these results is due to Dr Smart.

On the theoretical side his earlier work was in celestial mechanics. But in connection with the practical work above-mentioned his more recent interests have {1} been mainly in proper motions and other branches of stellar statistics, to which he is one of the most active contributors. He is a member of the Commission of the International Astronomical Union on Stellar Parallaxes and Proper Motions.

His teaching work covers elementary lectures on astronomy, advanced lectures on celestial mechanics and on stellar motions and a practical class at the observatory. Judging from the response of the students he is a stimulating lecturer. He normally supervises one or two research students.

An important part of his experience is his work as Secretary of the Royal Astronomical Society during the last five years. This brings him into touch with astronomers in all parts of the world, so that he is in full contact with all modern developments. It is perhaps not irrelevant to mention that he is Treasurer of the Royal Astronomical Society Dining Club—an office (of which the duties are by no means confined to the care of money) which is a tribute to his popularity with his colleagues.

To sum up:—He has shown himself able to make the most of the resources of a small observatory; he is well-known and esteemed internationally; he is successful with students; and is well used to administrative activity.

—————

The various cancelled words and passages in this letter have not been recorded, except for the mistaken deletion noted below.

{1} Struck through by mistake.

Chapter VIII: Double Frames
EDDN/B/1/10 · Pièce · Aug. 1944
Fait partie de Papers of Sir Arthur Eddington

§ 79. The EF-frame.
§ 80. Chirality of a double frame.
§ 81. The interchange operator.
§ 82. Duals.
§ 83. The CD-frame.
§ 84. Double-wave vectors.
§ 85. The 136-dimensional phase space.
§ 86. Uranoid and aether.
§ 87. The Riemann-Christoffel tensor.
§ 88. The de Sitter universe.
§ 89. The tensor identities.
§ 90. The contracted Riemann-Christoffel tensor.
§ 91. States and interstates.
§ 92. The recalcitrant terms.

Chapter IX: Simple Applications
EDDN/B/1/11 · Pièce · Aug. 1944
Fait partie de Papers of Sir Arthur Eddington

§ 93. The metastable states of hydrogen.
§ 94. Neutrium and deuterium.
§ 95. Mass of the neutron.
§ 96. Double intracules.
§ 97. Comparison with field theory.
§ 98. Mass of the deuterium atom.
§ 99. Mass of the helium atom.
§ 100. The separation constant of isobaric doublets.
§ 101. Isotopic spin.
§ 102. Radii of nuclei.
§ 103. The nuclear planoid.
§ 104. Mass of the mesotron.

Chapter X: The Wave Equation
EDDN/B/1/12 · Pièce · Sept. 1944
Fait partie de Papers of Sir Arthur Eddington

§ 105. Field momentum.
§ 106. The gradient operator.
§ 107. Isostatic compensation.
§ 108. Wave equation of the hydrogen intracule.
§ 109. Solution of the wave equation.
§ 110. The interchange momentum.
§ 111. The two-frame transformation.
§ 112. Electromagnetic potentials.

EDDN/B/1/13 · Pièce · Sept. 1944
Fait partie de Papers of Sir Arthur Eddington

§ 113. Gauge transformations (molar theory).
§ 114. Action invariants.
§ 115. Gauge transformations (microscopic theory).
§ 116. Indices of wave tensors.
§ 117. Magnetic moments.
§ 118. Magnetic moment of the hydrogen atom.
§ 119. Magnetic moment of the neutron.

(There is no § 120.)

EDDN/B/1/15 · Pièce · [Sept. 1944 and 1946]
Fait partie de Papers of Sir Arthur Eddington

Chapter XII [continued].
§ 125. Symbolic occupation.
§ 126. Einstein-Bose particles.
§ 127. Photons.
§ 128. Life-time of the mesotron.

Chapter XIII: Epistemological Theory.
[§§ 129–136.] As in Proceedings of the Cambridge Philosophical Society, vol. xl (1944), p. 37, expanded.

Chapter XIV. Summary.
§ 137. The principles of fundamental theory.

EDDN/B/1/3 · Pièce · June 1944
Fait partie de Papers of Sir Arthur Eddington

§ 1. The uncertainty of the origin.
§ 2. The physical origin.
§ 3. The Bernoulli fluctuation.
§ 4. The standard of length.
§ 5. Range of nuclear forces and the recession of the galaxies.
§ 6. Spherical space.
§ 7. Uranoids.
§ 8. The extraneous standard.
§ 9. Scale-free physics.
§ 10. Pseudo-discrete states.
§ 11. Stabilisation.

Chapter II: Multiplicity Factors
EDDN/B/1/4 · Pièce · June 1944
Fait partie de Papers of Sir Arthur Eddington

§ 12. Complementary fields.
§ 13. The rigid-field convention.
§ 14. Separation of field and particle energy.
§ 15. Application of scale-free systems.
§ 16. The ‘top particle’.
§ 17. Standard carriers.
§ 18. Mass-ratio of the proton and electron.
§ 19. Rigid coordinates.
§ 20. The fine-structure constant.
§ 21. The inversion of energy.
§ 22. Mutual and self energy.
§ 23. Comparison particles.

Chapter III: Interchange
EDDN/B/1/5 · Pièce · June 1944
Fait partie de Papers of Sir Arthur Eddington

§ 24. The phase dimension.
§ 25. Interchange of suffixes.
§ 26. The two-particle transformation.
§ 27. Hydrocules.
§ 28. Separation of electrical energy.
§ 29. Current masses of the proton and electron.
§ 30. Molarly controlled charge.
§ 31. Secondary anchors.
§ 32. Calculated values of the microscopic constants.
§ 33. The Coulomb energy.

Chapter IV: Gravitation and Exclusion
EDDN/B/1/6 · Pièce · July 1944
Fait partie de Papers of Sir Arthur Eddington

§ 34. Unsteady states.
§ 35. Under-observation.
§ 36. Structural and predictive theory.
§ 37. Physical and geometrical distribution functions.
§ 38. The weight function.
§ 39. The genesis of proper mass.
§ 40. Absolute determination of m0.
§ 41. Exclusion.
§ 42. The negative energy levels.
§ 43. Determination of m0 by exclusion theory.
§ 44. Super-dense matter.
§ 45. The degeneracy pressure.

Chapter V: The Planoid
EDDN/B/1/7 · Pièce · July 1944
Fait partie de Papers of Sir Arthur Eddington

§ 46. Uranoid and planoid.
§ 47. Interchange of extracules.
§ 48. The special planoid.
§ 49. The energy of two protons.
§ 50. Non-Coulombian energy.
§ 51. The constant of gravitation.
§ 52. Molar and nuclear constants.

Chapter VI: The Complete Momentum Vector
EDDN/B/1/8 · Pièce · July 1944
Fait partie de Papers of Sir Arthur Eddington

§ 53. The symbolic frame.
§ 54. Miscellaneous properties of E-symbols.
§ 55. Equivalence and chirality.
§ 56. Rotations.
§ 57. Five-dimensional theory.
§ 58. Ineffective relativity transformations.
§ 59. Strain vectors.
§ 60. Real and imaginary E-symbols.
§ 61. Reality conditions.
§ 62. Distinction between space and time.
§ 63. Neutral space-time.
§ 64. Congruent spaces.
§ 65. Determinants and eigenvalues.

Chapter VII: Wave Vectors
EDDN/B/1/9 · Pièce · July 1944
Fait partie de Papers of Sir Arthur Eddington

§ 66. Idempotency.
§ 67. Standard form of idempotent vectors.
§ 68. Spectral sets.
§ 69. Catalogue of symbolic coefficients.
§ 70. The wave identities.
§ 71. Matrix representation of E-numbers.
§ 72. Factorisation of E-numbers.
§ 73. Wave tensors of the second rank.
§ 74. Wave tensors of the fourth rank.
§ 75. Phase space.
§ 76. Relative space.
§ 77. Vectors in micro space.
§ 78. The quantum-classical analogy.

EDDN/B/2 · Dossier · early 1940s
Fait partie de Papers of Sir Arthur Eddington

These manuscripts are all in Eddington’s own hand, with the exception of the ringed pencil number on the first page of each and the foliation (in red biro, except B2/20), which were added by Slater, the former in June 1945, the latter about the end of 1947. Other notes by Slater indicate that there is a sheet missing from B2/22 between ff. 4 and 5, and that B2/29 f. 14 is a modification of f. 4.

Chapter II: Multiplicity Factors
EDDN/B/2/10 · Pièce · Dec. 1942–Aug. 1943
Fait partie de Papers of Sir Arthur Eddington

§ 12. Object-fields.
§ 13. The rigid field convention.
§ 14. Separation of particle and field energy.
§ 15. Application to scale-free systems.
§ 16. Standard carriers.
§ 17. Mass-ratio of the proton and electron.
§ 18. The fine-structure constant.
§ 19. Rigid coordinates.
§ 20. Unsteady states.
§ 21. The inversion of energy.

(Drafted Dec. 1942; revised Aug. 1943.)

EDDN/B/2/13 · Pièce · Dec. 1942–Aug. 1943
Fait partie de Papers of Sir Arthur Eddington

§ 1. The uncertainty of the origin.
§ 2. The Gaussian distribution.
§ 3. The Bernoulli fluctuation.
§ 4. The standard of length.
§ 5. Range of nuclear forces and the recession of the galaxies.
§ 6. Non-uniform curvature.
§ 7. Uranoids.
§ 8. The extraneous standard.
§ 9. Scale-free physics.
§ 10. Pseudo-discrete distributions.
§ 11. Stabilisation.

(Drafted Dec. 1942; revised Aug. 1943.)

Chapter IX: two sections
EDDN/B/2/14 · Pièce · [1943]
Fait partie de Papers of Sir Arthur Eddington

(i) Chapter IX: The Molar Electromagnetic Field.
Gauge transformations.

(ii) Chapter IX: The Molar Electromagnetic Field.
Affine field theory.

Chapter VII: Double Frames
EDDN/B/2/15 · Pièce · May 1943
Fait partie de Papers of Sir Arthur Eddington

§ 61. The EF-frame.
§ 62. Chirality of the double frame.
§ 63. The interchange operator.
§ 64. Duals.
§ 65. The CD-frame.
§ 66. Double phase space.
§ 67. The uranoid and the aether.
§ 68. The tensor identities.
§ 69. The quantum-classical analogy.
§ 70. Recoil rotations.
§ 71. Transformation to a relative frame.