The astronomical contributions of Sir Arthur Eddington have sometimes been distracted by his philosophy and his derivation of ~1079 for the total number of elementary particles in the universe. However, assumptions employed to obtain the universal mass in a volume of ~1079 m3 produce values remarkably commensurate with ~1079 protons. The congruence between the calculated gravitational forces for rest mass photons separated by Planck’s length and potassium ions separated by the distance that maintains a neuron’s resting plasma membrane potential is also consistent with his assumption that universal structure is mirrored within consciousness and its extensions through sensitive instrumentation. Recent measurements of photon emissions during c...
Arthur Eddington traveled to Principe in Africa in 1919 with the express purpose of proving Einstein...
40-42Sir Arthur Stanley Eddington, the ‘best measuring man’, the founder of theoretical astrophysic...
Eddington’s prediction for general relativity (GR) is exemplified by three cases: a static spherical...
Eddington believed that the number of particles in the universe was equal to the fine structure cons...
Abstract. Considering that the Large Eddington Number has correctly predicted the number of atoms in...
Abstract. Considering that the Large Eddington Number has correctly predicted the number of atoms in...
Arthur S. Eddington, FRS, (1882-1944) was one of the most prominent British scientists of his time. ...
Unanimement considéré comme l’astronome le plus influent de l’entre-deux guerres, Arthur S. Eddingto...
In 1919, mathematician and physicist Hermann Weyl puzzled why the ratio of the electromagnetic force...
Published by and copyright by the Astronomical Society of the Pacific.Arthur Stanley Eddington domin...
A previously derived mass relation has been extended to seven equidistant fundamental masses coverin...
Quantitative solutions involving classical methods indicated that the numbers of quantum foci within...
Quantitative solutions involving classical methods indicated that the numbers of quantum foci within...
Eddington in 1923, first identified four dimensionless numbers, derived from combinations of the bas...
This work is licensed under the Creative Commons Attribution International License (CC BY)The paramo...
Arthur Eddington traveled to Principe in Africa in 1919 with the express purpose of proving Einstein...
40-42Sir Arthur Stanley Eddington, the ‘best measuring man’, the founder of theoretical astrophysic...
Eddington’s prediction for general relativity (GR) is exemplified by three cases: a static spherical...
Eddington believed that the number of particles in the universe was equal to the fine structure cons...
Abstract. Considering that the Large Eddington Number has correctly predicted the number of atoms in...
Abstract. Considering that the Large Eddington Number has correctly predicted the number of atoms in...
Arthur S. Eddington, FRS, (1882-1944) was one of the most prominent British scientists of his time. ...
Unanimement considéré comme l’astronome le plus influent de l’entre-deux guerres, Arthur S. Eddingto...
In 1919, mathematician and physicist Hermann Weyl puzzled why the ratio of the electromagnetic force...
Published by and copyright by the Astronomical Society of the Pacific.Arthur Stanley Eddington domin...
A previously derived mass relation has been extended to seven equidistant fundamental masses coverin...
Quantitative solutions involving classical methods indicated that the numbers of quantum foci within...
Quantitative solutions involving classical methods indicated that the numbers of quantum foci within...
Eddington in 1923, first identified four dimensionless numbers, derived from combinations of the bas...
This work is licensed under the Creative Commons Attribution International License (CC BY)The paramo...
Arthur Eddington traveled to Principe in Africa in 1919 with the express purpose of proving Einstein...
40-42Sir Arthur Stanley Eddington, the ‘best measuring man’, the founder of theoretical astrophysic...
Eddington’s prediction for general relativity (GR) is exemplified by three cases: a static spherical...