"FEYNMAN, R. P. (+) N. BOHR (+) J. A. WHEELER (+) J. R. OPPENHEIMER (+) H. SNYDER.
Reference : 46900
(1939)
[Lancaster], American Institute of Physics, 1939. Royal8vo. Bound in contemporary full red cloth with gilt lettering to spine. Entire volume of ""The Physical Review"", Volume 56, Second Series, July 1 - December 15, 1939. ""Development Department"" in small gilt lettering to lower part of spine. A very fine and clean copy. [Feynman:] Pp. 340-43. [Bohr & Wheeler:] Pp. 426-50. [Oppenheimer & Snyder:] Pp. 455-59. [Entire volume: X, 1264 pp.].
First printing of three landmark papers, all of seminal importance in history of physics: Feynman's undergraduate thesis at MIT, the intricacies of the fission process, the groundwork for atomic and hydrogen bombs and the forgotten birth of black holes: The first theoretical description of a black hole, the production of a singularity when a sufficiently large neutron star collapses.First printing of ""FORCES IN MOLECULES"" - know known as Feynman-Hellmann theorem - is Feynman's undergraduate thesis at MIT, published when he was just twenty-one, which helped to establish his name in the world of physics. ""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."" (DSB). ""As Feynman conceived the structure of molecules, forces were the natural ingredients. He saw springlike bonds with varying stiffness, atoms attracting and repelling one another. The usual energy-accounting methods seemed secondhand and euphemistic: [He demonstrated that] the force on an atom's nucleus is no more or less than the electrical force from the surrounding field of charged electrons-the electrostatic force. Once the distribution of charge has been calculated quantum mechanically, then from that point forward quantum mechanics disappears from the picture. The problem becomes classical"" the nuclei can be treated as static points of mass and charge. Feynman's approach applies to all chemical bonds"" (Gleick, The Life and Science of Richard Feynman, P. 54).Oppenheimer and Snyder's ""ON CONTINUED GRAVITATIONAL CONTRACTION"" constitute the very first theoretical prediction of a singularity when a sufficiently large neutron star collapses. This phenomenon was later to be coined as a black hole. ""Had J. Robert Oppenheimer not led the US effort to build the atomic bomb, he might still have been remembered for figuring out how a black hole could form."" (American Physical Society). The paper has by several physics historians been described as the forgotten birth of black holes. ""Oppenheimer and his graduate student George Volkoff presented the first analysis of the formation of a neutron star in a 1939 Physical Review paper titled, ""On Massive Neutron Stars"". Oppenheimer wondered what would happen to a very massive neutron star. The Schwartzschild analysis of General Relativity has a theoretical limit, called the ""Schwartzschild limit"", when the ratio of mass-to-radius of a star is 236,000 times greater than the ratio for our sun. When this limit is exceeded, the Schwartzschild analysis does not yield a solution. Oppenheimer believed that a neutron star could have sufficient mass to exceed this limit. What would happen to it? Oppenheimer and his graduate student Hartland Snyder applied General Relativity theory to a star with sufficient mass and density to exceed the Schwartzschild limit. The Schwartzschild analysis assumed that the size of the star stays constant with time. Oppenheimer and Snyder found that they could achieve a real solution from General Relativity when the Schwartzschild limit is exceeded by assuming that the diameter of the star decreases with time. They presented their analysis in a 1939 Physical Review paper, titled, ""On Continual Gravitational Contraction,"" which concluded with: ""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."" This analysis concluded that when the Schwartzschild limit is exceeded, the star must collapse indefinitely until it reaches a singularity having an infinite density of matter"" (Bjornson, Singularity Predictions of General Relativity, P. 4).The Chandrasekhar / Eddington controvery in the mid 30ies did discuss the fate of neutron stars but the first thoroughly theoretical desciption was first published here. ""THE MECHANISM OF NUCLEAR FISSION"" is the first fully worked out theory of nuclear fission, which laid the groundwork for atomic and hydrogen bombs.""Wheeler's technical mastery of physics is best seen in the classic paper of Bohr and Wheeler. Bohr and Wheeler wrote the paper in Princeton, where Bohr was visiting in the spring of 1939, a few months after the discovery of fission. The paper is a masterpiece of clear thinking and lucid writing. It reveals, at the center of the mystery of fission, a tiny world where everything can be calculated and everything understood. The tiny world is a nucleus of uranium 236, formed when a neutron is freshly captured by a nucleus of uranium 235. The uranium 236 nucleus sits precisely on the border between classical and quantum physics. Seen from the classical point of view, it is a liquid drop composed of a positively charged fluid. The electrostatic force that is trying to split it apart is balanced by the nuclear surface tension that is holding it together. The energy supplied by the captured neutron causes the drop to oscillate in various normal modes that can be calculated classically. Seen from the quantum point of view, the nucleus is a superposition of a variety of quantum states leading to different final outcomes. The final outcome may be a uranium 235 nucleus with a re-emitted neutron, or a uranium 236 nucleus with an emitted gamma-ray, or a pair of fission-fragment nuclei with one or more free neutrons. Bohr and Wheeler calculate the cross-section for fission of uranium 235 by a slow neutron and get the right answer within a factor of two. Their calculation is a marvelous demonstration of the power of classical mechanics and quantum mechanics working together. By studying this process in detail, they show how the complementary views provided by classical and quantum pictures are both essential to the understanding of nature. Without the combined power of classical and quantum concepts, the intricacies of the fission process could never have been understood. Bohr's notion of complementarity is triumphantly vindicated"" (John Archibald Wheeler, Proceedings of the American Philosophical Society 154 (2010)).
"BOHR, N. (+) J. A. WHEELER (+) J. R. OPPENHEIMER (+) H. SNYDER.
Reference : 54015
(1939)
Lancaster, American Institute of Physics, 1939. Royal8vo. In the original green printed wrappers. In ""The Physical Review"", Volume 56, Second Series, Number 5, September 1. With cloth back-strip. A quire, affecting both papers, detached but without any loss of paper. A few minor tear throughout, far from affecting text. [Bohr & Wheeler:] Pp. 426-50. [Oppenheimer & Snyder:] Pp. 455-59. [Entire volume: Pp. 387-486].
First printing of two landmark papers, all of seminal importance in history of physics: The intricacies of the fission process, the groundwork for atomic and hydrogen bombs and the forgotten birth of black holes: The first theoretical description of a black hole, the production of a singularity when a sufficiently large neutron star collapses.Oppenheimer and Snyder's ""ON CONTINUED GRAVITATIONAL CONTRACTION"" constitute the very first theoretical prediction of a singularity when a sufficiently large neutron star collapses. This phenomenon was later to be coined as a black hole. ""Had J. Robert Oppenheimer not led the US effort to build the atomic bomb, he might still have been remembered for figuring out how a black hole could form."" (American Physical Society). The paper has by several physics historians been described as the forgotten birth of black holes. ""Oppenheimer and his graduate student George Volkoff presented the first analysis of the formation of a neutron star in a 1939 Physical Review paper titled, ""On Massive Neutron Stars"". Oppenheimer wondered what would happen to a very massive neutron star. The Schwartzschild analysis of General Relativity has a theoretical limit, called the ""Schwartzschild limit"", when the ratio of mass-to-radius of a star is 236,000 times greater than the ratio for our sun. When this limit is exceeded, the Schwartzschild analysis does not yield a solution. Oppenheimer believed that a neutron star could have sufficient mass to exceed this limit. What would happen to it? Oppenheimer and his graduate student Hartland Snyder applied General Relativity theory to a star with sufficient mass and density to exceed the Schwartzschild limit. The Schwartzschild analysis assumed that the size of the star stays constant with time. Oppenheimer and Snyder found that they could achieve a real solution from General Relativity when the Schwartzschild limit is exceeded by assuming that the diameter of the star decreases with time. They presented their analysis in a 1939 Physical Review paper, titled, ""On Continual Gravitational Contraction,"" which concluded with: ""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."" This analysis concluded that when the Schwartzschild limit is exceeded, the star must collapse indefinitely until it reaches a singularity having an infinite density of matter"" (Bjornson, Singularity Predictions of General Relativity, P. 4).The Chandrasekhar / Eddington controvery in the mid 30ies did discuss the fate of neutron stars but the first thoroughly theoretical desciption was first published here. ""THE MECHANISM OF NUCLEAR FISSION"" is the first fully worked out theory of nuclear fission, which laid the groundwork for atomic and hydrogen bombs.""Wheeler's technical mastery of physics is best seen in the classic paper of Bohr and Wheeler. Bohr and Wheeler wrote the paper in Princeton, where Bohr was visiting in the spring of 1939, a few months after the discovery of fission. The paper is a masterpiece of clear thinking and lucid writing. It reveals, at the center of the mystery of fission, a tiny world where everything can be calculated and everything understood. The tiny world is a nucleus of uranium 236, formed when a neutron is freshly captured by a nucleus of uranium 235. The uranium 236 nucleus sits precisely on the border between classical and quantum physics. Seen from the classical point of view, it is a liquid drop composed of a positively charged fluid. The electrostatic force that is trying to split it apart is balanced by the nuclear surface tension that is holding it together. The energy supplied by the captured neutron causes the drop to oscillate in various normal modes that can be calculated classically. Seen from the quantum point of view, the nucleus is a superposition of a variety of quantum states leading to different final outcomes. The final outcome may be a uranium 235 nucleus with a re-emitted neutron, or a uranium 236 nucleus with an emitted gamma-ray, or a pair of fission-fragment nuclei with one or more free neutrons. Bohr and Wheeler calculate the cross-section for fission of uranium 235 by a slow neutron and get the right answer within a factor of two. Their calculation is a marvelous demonstration of the power of classical mechanics and quantum mechanics working together. By studying this process in detail, they show how the complementary views provided by classical and quantum pictures are both essential to the understanding of nature. Without the combined power of classical and quantum concepts, the intricacies of the fission process could never have been understood. Bohr's notion of complementarity is triumphantly vindicated"" (John Archibald Wheeler, Proceedings of the American Philosophical Society 154 (2010)).
- Klickmann F.Henri,Williams Spencer,Pinkard Maceo,White James,Garrett Lloyd,Warfield Chas.,Stewart Paul,Keithley E. Clinton,Wand Hart A.,Speroy Robert,Frost Jack,Neander Harold,Snyder Chas. - Williams Spencer,Graham Roger,Armstrong Paul B.,White James,Garrett Lloyd,Frost Jack,Warfield Chas.,Stewart Paul,Snyder Chas.,Nesbit Wilbur D.
Reference : 92158
(1918)
New York. Liveright, 1979. In-4 reliure pleine toile éditeur, jaquette illustrée en couleurs. Textes en anglais de Gerard Malanga et Angus MacLise. Nombreuses photos en couleurs, vision très psychédélique des années 60. E.O. Bel envoi autographe de Don Snyder.
1969 A New Directions Paperbook (1969) - In-8 broché de 144 pages - Couverture illustrée en noir et blanc - Bon état
1974 Los Angeles : Nash Publishing, 1974 - grand format (21,1x27,6 cm) sous couverture illustrée en deux tons, 126 pages illustrées en noir - texte en anglais - Exemplaire enrichi d'un envoi autographe signé de Robert Snyder -
Allen Cohen, Bruce Conner, Rick Griffin, Allen Ginsberg, Gary Snyder, Lawrence Ferlinghetti, Michael McClure
Reference : 104419
n°1, septembre 1966 - n°12, février 1968; Format de 280x280mm à 445x929mm, 12 à 32 pages, en feuilles.Collection complète (104419)
Également connu sous le nom de San Francisco Oracle, the Oracle of the city of San Francisco était un journal clandestin publié en 12 numéros du 20 septembre 1966 à février 1968 dans le quartier Haight-Ashbury de cette ville. Allen Cohen (1940-2004), rédacteur en chef pendant la période la plus dynamique du journal, et Michael Bowen, directeur artistique, comptent parmi les fondateurs de la publication. L'Oracle a été l'un des premiers membres de l'Underground Press Syndicate. L'Oracle combinait poésie, spiritualité et intérêts multiculturels avec un design psychédélique, reflétant et façonnant la communauté contre-culturelle telle qu'elle se développait à Haight-Ashbury. Sans doute l'exemple exceptionnel de psychédélisme dans la presse « underground », la publication était connue pour son design multicolore expérimental. Les contributeurs d'Oracle comprenaient de nombreux artistes importants de la région de San Francisco de l'époque, notamment Bruce Conner et Rick Griffin. Il mettait en vedette des auteurs de beat tels qu'Allen Ginsberg, Gary Snyder, Lawrence Ferlinghetti et Michael McClure. Bel état dans un boîte de Pierre Mercier (1928-2014) signée et datée (19)89.
Phone number : +33 1 48 01 02 37
Allen Ginsberg, Jack Kerouac, William Burroughs, Mezz Mezzrow, Charles Olson, Allan Kaprow, Harold Norse, Rexroth, Lawrence Durrel, Robert Creeley, Diane di Prima, Dick Higgins, Henri Miller, Gary Snyder, LeRoi Jones, Douglas Woolf, Larry Eigner, Michael McClure, Barbara Moraff
Reference : 103283
(1961)
1961-1969 5 numéros en 4 volumes, collection complète en édition de luxe.New Orleans, Louisiana et Tucson, Arizona, 1961-1969, volumes 1 à 3 brochés couvertures photographiques 233x155mm, n°4/5 cartonné couverture photographique, 260x185mm , jaquette translucide en papier végétal imprimé.Publié et imprimé à la main au Loujon’s Desert Workshop Printery, Arizona par Jon Edgar et Louise "Gypsy Lou" Webb avec un soin et des matériaux délicatement choisis, The Outsider n'en resta pas moins scrupuleusement fidèle à l'esprit de la "mimeograph revolution" par son attachement à des auteurs comme Charles Bukowski et Kenneth Patchen.Contributions de Allen Ginsberg, Jack Kerouac, William Burroughs, Mezz Mezzrow, Charles Olson, Allan Kaprow, Harold Norse, Rexroth, Lawrence Durrel, Robert Creeley, Diane di Prima, Dick Higgins, Henri Miller, Gary Snyder, LeRoi Jones, Douglas Woolf, Larry Eigner, Michael McClure, Barbara Moraff et beaucoup d’autres. Le dernier numéro 4/5 est luxueusement imprimé en plusieurs couleurs et comporte une section de 46 pages d’hommage au poète Kenneth Patchen à qui il est dédié; il est ici en édition limitée comportant en outre une nature morte hors texte réalisée à partir d’une fleur cueillie sur l’ancien territoire apache près de la tombe de Geronimo et réputée permettre d'exaucer un vœu. Clay/ Phillips p.50, 190. (103283)
Phone number : +33 1 48 01 02 37
Graves (Alvin Cushman) and Froman (Darol Kennedy), eds. - R.W. Dodson, A.C. Graves, L. Helmholz, D.L. Hufford, R.M. Potter and J.G. Povelites - A.C. Graves, R.L. Walker, R.F. Taschek, A.O. Hanson, J.H. Williams and H.M. Agnew - Donald Kerst - B.D. McDaniel, Leo S. Lavatelli and Elizabeth Graves - Thomas Snyder and David Lipkin - J.E. Mack
Reference : 100390
(1952)
McGraw-Hill Book Company, Inc. , National Nuclear Energy Series Malicorne sur Sarthe, 72, Pays de la Loire, France 1952 Book condition, Etat : Bon hardcover, editor's binding, full blue printed clothes, no dust-jacket, red title-piece on the spine grand In-8 1 vol. - 336 pages
many black and white illustrations and text-figures 1st edition, 1952 Contents, Chapitres : Foreword by Gordon Dean, Acknowledgments, Preface, Preface to the Experimental Techniques volumes, Contents, xiii, Text,323 pages - 1. R.W. Dodson, A.C. Graves, L. Helmholz, D.L. Hufford, R.M. Potter and J.G. Povelites : Preparation of Foils - A.C. Graves, R.L. Walker, R.F. Taschek, A.O. Hanson, J.H. Williams and H.M. Agnew : Neutron Sources - Donald Kerst : The Modulated Betatron - B.D. McDaniel, Leo S. Lavatelli and Elizabeth Graves : Modulation and other Techniques Used with Ion Accelerators - Thomas Snyder and David Lipkin : Topics on Vacuum Technique - J.E. Mack : Optical Methods and Instruments - Index - Alvin Cushman Graves (né le 4 novembre 1909 mort le 19 juillet 1965) est un physicien nucléaire américain ayant travaillé au Metallurgical Laboratory du projet Manhattan ainsi qu'au Laboratoire national de Los Alamos lors de la Seconde Guerre mondiale. Après la guerre, il est nommé à la tête de la division J à Los Alamos. Il a été le directeur ou l'assistant directeur de nombreux essais nucléaires au cours des années 1940 et 1950. - Au cours des années 1950, Alvin Graves est directeur des essais nucléaire au Nevada Test Site. Il devient critique envers ceux qui soulignent les risques liés à ces derniers, affirmant que ces derniers sont de « faibles tire-au-flanctrad ». Porte-parole du site, il fait le tour des environs pour rassurer la population sur les activités qui s'y tiennent et sur l'absence de dangers. À la tête de la division J du Laboratoire national de Los Alamos5, Graves gère la plupart des essais nucléaires de la fin des années 1940 et des années 1950, incluant les exercices Desert Rock et Castle Bravo. - Darol Kenneth Froman (October 23, 1906 September 11, 1997) was the Deputy Director of the Los Alamos National Laboratory from 1951 to 1962. He served as a group leader from 1943 to 1945, and a division head from 1945 to 1948. He was the scientific director of the Operation Sandstone nuclear tests at Enewetak Atoll in the Pacific in 1948, and Assistant Director for Weapons Development from 1949 to 1951. ex-library copy, track on sticker and numer on the bottom of the spine, editor's binding remains in rather very good condition, text is clean, but few ex-library markings, stamps, bookplate, number, with the cancellation stamp
Partitions sur la Danse Salabert Edouard 1911
Très bon état Grand format Piano
Partitions sur l'Amérique du Nord,Partitions sur le Train Snyder Ted 1909
Etat moyen Grand format Piano
Snyder Ted 1910
Bon état Grand format Piano
[Armengol H. Langlois] - - Berlin Irving,Snyder Ted,Salabert Francis -
Reference : 92143
(1911)
Partitions sur la Danse Salabert 1911
Bon état Grand format Piano
Princeton (U.S.A.), The Pyne Press, 1971 Bound, blue leather hardcover with goldprint, 23.3x15.7 cm., pages not numbered, illustrated catalog in b/w with historical introduction.
Editions Francis Salabert. 1921. In-Folio. En feuillets. Etat d'usage, Couv. légèrement passée, Dos satisfaisant, Intérieur bon état. 4 pages, 1er plat illustré par R. de Valerio, tampon.. . . . Classification Dewey : 0-GENERALITES
Le Sheik, dans l'immense Sahara, chanson du célèbre film Paramount Le Cheik, paroles françaises par Lucien Boyer, musique par Ted Snyder. E.A.S2333. Classification Dewey : 0-GENERALITES
Belin.1993.In-8 carré,caronnage en couleurs éditeur.229 p.Ills.en couleurs.TBE.
Arché, Bibliotheca Hermetica, 1977, 157 p., petit in-8, broché, bon état.
TraduCtion française de la Commentation de pharmaco Catholico (1665) par Pierre Pascal. Merci de nous contacter à l'avance si vous souhaitez consulter une référence au sein de notre librairie.
New York, Lamber Snyder, ( n.d. ca. 1910). 4 pp. Flyer, 9,4 x 15,5 pp. With 2 illustrations.
A folded advertisement sheet for the portable Exhilarator and a brief introduction regarding exhilaration by means of vibration. The company claimed: "There is only one disease - Congestion", "There is only one cure - Circulation".
Ed. Seuil, 1981, format poche, 179pp. , bon état.
Coll. Points- Actuels, A40.
DC Comics. 2012. In-8. Cartonné. Etat d'usage, Couv. convenable, Dos satisfaisant, Intérieur frais. 150 pages environ de bandes dessinées en couleurs.. . . . Classification Dewey : 843.067-Comics
Classification Dewey : 843.067-Comics
BELLES LETTRES EDITIONS -LES-
LIVRE A L’ETAT DE NEUF. EXPEDIE SOUS 3 JOURS OUVRES. NUMERO DE SUIVI COMMUNIQUE AVANT ENVOI, EMBALLAGE RENFORCE. EAN:9782251451831
CASTOR ASTRAL EDITEUR
LIVRE A L’ETAT DE NEUF. EXPEDIE SOUS 3 JOURS OUVRES. NUMERO DE SUIVI COMMUNIQUE AVANT ENVOI, EMBALLAGE RENFORCE. EAN:9791027803132
WILDPROJECT ED
LIVRE A L’ETAT DE NEUF. EXPEDIE SOUS 3 JOURS OUVRES. NUMERO DE SUIVI COMMUNIQUE AVANT ENVOI, EMBALLAGE RENFORCE. EAN:9782381140421
Snyder, Scott; Soule, Charles; Camuncoli, Giuseppe
Reference : SVALIVCN-9782413041092
Delcourt (11/2023)
LIVRE A L’ETAT DE NEUF. EXPEDIE SOUS 3 JOURS OUVRES. NUMERO DE SUIVI COMMUNIQUE AVANT ENVOI, EMBALLAGE RENFORCE. EAN:9782413041092
Delcourt (5/2024)
LIVRE A L’ETAT DE NEUF. EXPEDIE SOUS 3 JOURS OUVRES. NUMERO DE SUIVI COMMUNIQUE AVANT ENVOI, EMBALLAGE RENFORCE. EAN:9782413049715