OPPENHEIMER, J. Robert. “On continued gravitational contraction” and many other papers offered in one monumental year of the Physical Review for 1939.
American Physical Society, Lancaster Pa., January-December 1939. Two volumes: x, 1294pp & x,1300pp. The two volumes, complete. Finely and sturdily rebound in cloth and marbled boards. Very stout, readable volumes. Fine condition. Few scant ownership stamps on some of the individual issues' first page. $2250
This is a remarkable volume for one of the most electrifying years in the history of modern phsyics, ranking alongside the great years of 1859, 1932, and 1948 for the sheer weight of highly significant papers from many sources. Included are papers by Oppenheimer, Gamow, Feynman, Szilard, Bethe, Rabi, Anderson, Tolman, Morrison, Kusch, Abelson, and many others. Astonishing, really.
Some of the most significant papers include:
OPPENHEIMER, Robert and Hartland Snyder, “On continued gravitational contraction”, September 1, 1939, Vol. 56, #5, pp. 426-50 The Oppenheimer and Snyder (a graduate assistant) paper is one of the most prescient in the history of modern physics, correctly physically describing (where Chandrasekhar and Eddington in their discussions did not) what happens in a particular collapse of a neutron star, and still today reads as fresh and and brightly as it did in 1939. Really, it is an extraordinary work, and a foundation paper in the history of gravitation, the application of RT, singularity, and astrophysics. (The Southampton GR Explorer site nicely states it this way: "This paper has strong claims to being one of the most prophetic ever written in this field of research. Today, 60 years later, this paper needs little revision - even the terminology is undated!")
In an often-repeated quotation, they write, somewhat in irony and in a certain and understated manner on page 456: "The star thus tends to close itself off from any communication with a distant observer; only its gravitational field persists". And later: "When all thermonuclear sources of energy are exhausted, a sufficiently heavy star will collapse. Unless fission due to rotation, the radiation of mass, or the blowing off of mass by radiation, reduce the star's mass to the order of that of the sun, this contraction will continue indefinitely", they wrote.
BOHR, Niels and J.A. Wheeler, “The mechanism of nuclear fission”, September 1, 1939, Vol. 56, pp. 455-459. This is the experimental foundation stone (on the basis of the liquid drop model of atomic nuclei) of nuclear fission and the great leap forward in the construction of the atomic bomb.
From the abstract: "On the basis of the liquid drop model of atomic nuclei, an account is given of the mechanism of nuclear fission. In particular, conclusions are drawn regarding the variation from nucleus to nucleus of the critical energy required for fission, and regarding the dependence of fission cross section for a given nucleus on energy of the exciting agency. A detailed discussion of the observations is presented on the basis of the theoretical considerations. Theory and experiment fit together in a reasonable way to give a satisfactory picture of nuclear fission".
BOHR, Niels. “Resonance in Uranium and Thorium Disintegrations and the Phenomenon of Nuclear Fission”;
BETHE, Hans. "Meson Theory of Nuclear Forces." Vol 55, 2nd series, number 12; June 15, 1939, 1261-1264
BETHE, Hans. “Energy Production in Stars” no 1. January 1, 1939 -and- "Energy Production in Stars II", no. 5 March 1, 1939). Awarded the Nobel Prize (the first time the award was given for astrophysics) 1967 "for his contributions to the theory of nuclear reactions, especially his discoveries concerning the energy production in stars")
OPPENHEIMER, J. Robert and G.M. Volkhoff in the 15 February 1939 issue. Here (along with a preceding paper by Richard C. Tolman, issued in the same issue just above Oppenheimer, which were the analytic analysis used by O+V to base their estimates of nuclear forces) was established the Tolman-Oppenheimer-Volkhoff limit, which stated that if the state of evolution of neutrons forming a degenerate Fermi gas of extremely dense masses in neutron stars was more massive than .07 solar masses that it would collapse into a black hole or exotic/quark star; if the mass was below that limit, the star would not collapse due to the degeneracy pressure of neutrons and the strong force. The black hole part was left really to a second paper of 1 September 1939 (the day that the Nazis attacked Poland and the fighting began in World War II in Europe) .
GAMOW, George and Edward Teller, "On the Origin of Great Nebulae", volume 55, number 7, April 1, 1939, pp 654-657, in the weekly issue of pp 609-671.
FEYNMAN, Richard. “Forces in Molecules”, pp. 340-43. Feynman's undergraduate thesis at MIT, know known as Feynman-Hellmann theorem - "This work treated the problem of molecular forces from a thoroughly quantum-mechanical point of view, arriving at a simple means of calculating the energy of a molecular system that continues to guide quantum chemists." (Complete DSB online)
SLIZARD, Leo and ZINN's landmark "Instantaneous Emission of Fast Neutrons in the Interaction of Slow Neutrons with Uranium" confirmed 'instantaneous' neutron multiplication, showing that it meets the requirement for nuclear bombs. Some argue this is one of the most important papers in atomic/nuclear physic
ANDERSON, Herbert L, Fermi, Enrico & Hanstein, H. B. “Production of Neutrons in Uranium Bombarded by Neutrons”, vol 55, pp. 415-419;
TOLMAN, Richard, “Static Solutions of Einstein's Field Equations for Spheres of Fluid”, vol 55, pp. 799-800;
RABI, I, Millman, S., Kusch, P. & Zacharias J. R. “The Molecular Beam Resonance Method for Measuring Nuclear Magnetic Moments ()”, vol 55, pp 526-535;
WEISSKOPF, Viktor. “On the Self-Energy and the Electromagnetic Field of the Electron”, 56 No. 1 pp. 72–85, July 1, 1939 . Also bound in the same issue with: “Weisskopf demonstrates that QED diverges at all levels of perturbation theory.” --This paper reproduced in full as paper 6 in Julian Schwinger’s Selected Papers on Quantum Electrodynamics. See also Jo Bovy (Ghent University),
ABELSON, Philip. “Investigation of the Products of the Disintegration of Uranium by Neutrons”, July 1, 1939, pp 1-9.
RABI, I.I., Kellogg, J. M. B. “The magnetic moment of the proton and the deuteron. The radiofrequency spectrum of H2 in various magnetic fields” , vol. 56, No. 8., pp 728-743.