276 books for « c b wheeler »Edit

‎Forces in molecules [Feynman] (+) The mechanism of nuclear fission [N. Bohr. & J. A. Wheeler] ""On continued gravitational contraction"" [J. R. Oppenheimer & H. Snyder]. - [FEYNMAN'S UNDERGRADUATE THESIS & THE FIRST THEORETICAL DESCRIPTION OF A SINGULARITY]‎

‎[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.].‎

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‎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)).‎

‎The mechanism of nuclear fission [N. Bohr. & J. A. Wheeler] ""On continued gravitational contraction"" [J. R. Oppenheimer & H. Snyder]. - [THE FIRST THEORETICAL DESCRIPTION OF A SINGULARITY]‎

‎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)).‎

‎Mathématique dans l'enseignement élémentaire / modèles patrons et situations de 6 à 12 ans‎

‎O.c.d.l 1970 IN8. 1970. Relié jaquette. 373 pages. Bon Etat intérieur propre? JAQUETTE LEGEREMENT USAG2E‎

‎Le drame de l'armée allemande‎

‎Gallimard/ l'air du temps 1955 in8. 1955. broché. 589 pages. Bon Etat‎

‎L'art romain‎

‎Librairie larousse 1965 in8. 1965. Cartonné jaquette. 250 pages. Bon Etat‎

‎Les grandes aventures de l'archéologie‎

‎Laffont 1960 16x18. 1960. Reliure editeur. 310 pages. Bon Etat‎

‎Bali Lombok‎

‎Lonely Planet 1997 in8. 1997. Broché. 375 pages. Bon Etat‎

‎Les grandes aventures de l'archéologie‎

‎Laffont 1960 in8. 1960. Broché. 250 pages. Etat Correct‎

‎Business Process Reengineering: Breakpoint Strategies for Market Dominance‎

‎John Wiley & Sons 1993 23x16x3cm. 1993. Relié. 256 pages. Très Bon Etat‎

‎Les influences romaines au-delà des frontières impériales.‎

‎ 1960 Plon 1960, collection "Civilisations d'Hier et d'Aujourd'hui", IX+232pp., petit in-8, 16 cartes in texte, broché. ‎

‎Bon État ‎

‎Un Mystère de Peter Duluth : Puzzle de Mort. ( Avec jaquette et dédicaces autographes signées des auteurs, Richard Wilson Webb et Hugh Callingham Wheeler et du traducteur, Maurice-Bernard Endrèbe ).‎

‎ Editions Presses de la Cité / Collection Cosmopolis ( ancêtre de la collection " Un Mystère " ) 1949. In-12 broché de 250 pages au format 12 x 19 cm. Couverture avec titre imprimé. Dos carré. Plats et intérieur parfaits. Exemplaire non coupé. Complet de la belle jaquette illustrée. Rarissime édition originale surtout dans un tél état de fraicheur. Précieux exemplaire orné de 3 dédicaces autographes signées, non nominatives, de Patrick Quentin alias, Richard Wilson Webb et Hugh Callingham Wheeler et du traducteur, Maurice-Bernard Endrèbe.‎

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‎. Site Internet : Http://librairie-victor-sevilla.fr.Vente exclusivement par correspondance. Le libraire ne reçoit, exceptionnellement que sur rendez-vous. Il est préférable de téléphoner avant tout déplacement.Forfait de port pour un livre 7 €, sauf si épaisseur supérieure à 3 cm ou valeur supérieure ou égale à 100 €, dans ce cas expédition obligatoire au tarif Colissimo en vigueur. A partir de 2 livres envoi en colissimo obligatoire. Port à la charge de l'acheteur pour le reste du monde.Les Chèques ne sont plus acceptés.Pour destinations extra-planétaire s'adresser à la NASA.Membre du Syndicat Lusitanien Amateurs Morues‎

‎The Ants of North Dakota.‎

‎1963 viii, 326 p., num. figs & maps, paperbound. Library stamps, else good copy of the original, not a low quality modern print on demand reprint.‎

‎Les champignons, connaître et cuisiner.‎

‎Paris, Larousse, 1996, 1 volume, in-4, cartonnage rigide éditeur, 286 p.. Très nombreuses photographies couleur, glossaire, index des champignons et index des recettes en fin de volume. Un angle légèrement accidenté à la couverture.‎

‎ Très bel exemplaire. ************* Remise 20 % pour toute commande supérieure à 100 €, envoi gratuit en courrier suivi et assurance à partir de 30 € d'achat (France seulement).‎

‎Les Fruits. - Connaître - Utiliser - Savourer. ‎

‎sl, Editions Du May, 1996, 1 volume, in-4, cartonnage souple remplié, 159 p.. Nombreuses illustrations noir et couleur (photographies, dessins, documents), bibliographie en fin de volume.‎

‎Plusieurs recettes sur les eaux-de-vie et liqueurs. A l'état de neuf. ************* Remise 20 % pour toute commande supérieure à 100 €, envoi gratuit en courrier suivi et assurance à partir de 30 € d'achat (France seulement).‎

‎GRANDES AVENTURES DE L'ARCHEOLOGIE" ‎

‎ LAFFONT 1960 IN8 br.,couv.ill;leg.accroc 2eme plat,249p.;ht;n.c. ‎

‎TISSUS IMPRIMES‎

‎ P , Carrousel, 1999 , in4° br , 174 pp , abondantes illustrations Langue: Français ‎

‎Papiers fantaisie.‎

‎Paris, L'Aventurine, 1997, 1 volume, in-4, cartonnage souple éditeur, 175 p. Très nombreuses illustrations en couleur.‎

‎ Exemplaire à l'état de neuf. ************* Remise 20 % pour toute commande supérieure à 100 €, envoi gratuit en courrier suivi et assurance à partir de 30 € d'achat (France seulement).‎

‎The Awakening of the Laurentians. / A Fabulous woman Lucille Wheeler and her family who made the Laurentians famous. ‎

‎New York, Vantage Press, (1958). In-16 (20.2 cm) 93, (3) pages. Reliure toile bleue d'édition en très bel état. Jaquette défraîchie de petits accrocs, dont 2 réparés au ruban gommé, coin supérieur du rabat coupé. Édition originale signée par l'auteure au titre.‎

‎Frances Wheeler, née à St-Jovite dans les Laurentides, fille de pionniers du Mont Tremblant, première femme à gravir cette montagne.‎

‎The Letters of Private Wheeler.. Edited and with a foreword by Captain B. H. Liddell Hart‎

‎Boston, Houghton Mifflin Company, 1952 in-8, VIII-342 pp., index, bradel toile grise et rouge sous jaquette illustrée (reliure de l'éditeur). Jaquette défraîchie.‎

‎125 lettres écrites entre 1809 et 1828. - - VENTE PAR CORRESPONDANCE UNIQUEMENT‎

‎Guide de Voyage‎

‎Lonely Planet Broché D'occasion bon état 30/08/1996 426 pages ‎

‎NEPAL. 2ème édition‎

‎Lonely Planet Broché D'occasion état correct 01/02/1997 452 pages ‎

‎Cambodge‎

‎Lonely Planet Relié D'occasion bon état 28/02/1997 186 pages ‎

‎Foundations of Accounting Theory - Papers Given at the Accounting Theory Symposium, University of Florida, March 1970 , (Information, business, and society - Varieties of accounting theory - The commercial foundations of accounting theory - The balance sheet embodiment of the most fundamental elements of accounting theory - What is the measure of A statement of basic accounting - The past's future)‎

‎University of Florida Press , University of Florida Accounting Series, n° 7 Malicorne sur Sarthe, 72, Pays de la Loire, France 1971 Book condition, Etat : Bon hardcover, editor's full blue printed binding, no dust-jacket grand In-8 1 vol. - 175 pages‎

‎a photography of Bill Paton 1st edition, 1971 "Contents, Chapitres : Foreword, Contributors, Contents, Introduction by William A. Paton, xi, Text, 164 pages - Norton M. Bedford : Information, business, and society - John T. Wheeler : Discussion on Norton Bedford paper, Information, business, and society - Louis Goldberg : Varieties of accounting theory - Stephen A. Zeff : Comments on Varieties of Accounting Theory - R.J. Chambers : The commercial foundations of accounting theory - Kermit D. Larson : Are there commercial foundations of accounting theory ? - Robert T. Sprouse : The balance sheet embodiment of the most fundamental elements of accounting theory - Alfred Rapaport : Discussion of the ""Balance sheet-embodiment..."" - Harvey T. Deinzer : What is the measure of A statement of basic accounting - Robert R. Sterling : A response - C. West Chruchman : The past's future - Robert E. Jensen : Discussion on the Past's future" editor's binding in very good condition, minor wear on the top of the spine, inside is fine, no markings‎

‎Lady Wheeler. Les Grandes aventures de l'archéologie : . Traduit de l'anglais par Eliette Vasseur‎

‎R. LaffontLagny-sur-Marne impr. E. Grevin et fils 1960 253 pages 1960. 253 pages.‎

‎Corse - plus de 100 pages sur la plongee et la randonnee‎

‎Lonely Planet. 1999. In-8. Broché. Bon état, Couv. convenable, Dos satisfaisant, Intérieur frais. 335 pages - texte sur deux colonnes - quelques illustrations noir/blanc et couleurs, dans et hors texte, dont cartes.. . . . Classification Dewey : 53-Guide‎

‎Tony Wheeler, Jean-Bernard Carillet, Olivier Cirendini, Christophe Corbel, Laurence Billiet Classification Dewey : 53-Guide‎