61. The Nobel Prize For Physics (1901-1996) The following is a complete listing of nobel Prize awards, from the firstaward in 1901. 1913, heike Kamerlingh Onnes, Matter at low temperature. http://physics.hallym.ac.kr/education/faq/nobel_html.html

The Nobel Prize for Physics (1901-1996) The following is a complete listing of Nobel Prize awards, from the first award in 1901. Prizes were not awarded in every year. The description following the names is an abbreviation of the official citation. Wilhelm Konrad Roentgen X-rays Hendrik Antoon Lorentz Pieter Zeeman Magnetism in radiation phenomena Antoine Henri Bequerel Pierre Curie Marie Sklodowska-Curie Spontaneous radioactivity Lord Rayleigh (a.k.a. John William Strutt) Density of gases and discovery of argon Pilipp Eduard Anton von Lenard Cathode rays Joseph John Thomson Conduction of electricity by gases Albert Abraham Michelson Precision meteorological investigations Gabriel Lippman Reproducing colors photographically based on the phenomenon of interference Guglielmo Marconi Carl Ferdinand Braun Wireless telegraphy Johannes Diderik van der Waals Equation of state of fluids Wilhelm Wien Laws of radiation of heat Nils Gustaf Dalen Automatic gas flow regulators Heike Kamerlingh Onnes Matter at low temperature Max von Laue Crystal diffraction of X-rays William Henry Bragg William Lawrence Bragg X-ray analysis of crystal structure no award Charles Glover Barkla Characteristic X-ray spectra of elements Max Planck Energy quanta Johannes Stark Splitting of spectral lines in E fields Charles-Edouard Guillaume Anomalies in nickel steel alloys Albert Einstein Photoelectric Effect Niels Bohr Structure of atoms Robert Andrew Millikan Elementary charge of electricity Karl Manne Georg Siegbahn

62. Nobel Prize Winners In Physics lighthouses. 1913, heike Kamerlingh Onnes, 18531926, for his work on theproperties of matter at low temperatures and for liquefying helium. http://empl.ksc.nasa.gov/nobelwin.htm

Year Winner Lifetime Contribution Wilhelm Konrad Rontgen for the discovery of x-rays Hendrik Antoon Lorentz Pieter Zeeman for their work on the influence of magnetism on radiation. Antoine Henri Becquerel Pierre Curie Marie Sklowdowska-Curie for his discovery of radioactivity. for their joint research on nuclear radiation phenomena. Lord Rayleigh (John William Strutt) for his research on the densities of the gases and for his discovery of argon Philipp Eduard Anton von Lenard for his work on cathode rays. Joseph John Thomson for his research on the conduction of electricity by gases. Albert Abraham Michelson for his optical instruments and for measuring the speed of light. Gabriel Lippmann for his method of reproducing colors photographically based on the interference techiniques. Guglielmo Marconi Carl Ferdinand Braun for their development of wireless telegraphy. Johannes Diderik van der Waals for his research on the equation of state for gases and liquids.

63. Nobel Prize Winners In Physics, 1901-2000 nobel Prize Winners in Physics, 19012000. 1913, heike Kamerlingh Onnes, 1853-1926,for his work on the properties of matter at low temperatures and for liquefying http://empl.ksc.nasa.gov/nobelwintext.htm

Electromagnetic Physics Laboratory NASA/Kennedy Space Center Local Site Navigation: Home About Services Fundamentals ... Search Kennedy Space Center Links: KSC Home KSC Site Search FAQ's Site Survey ... Headlines Nobel Prize Winners in Physics, 1901-2000 Year Winner Lifetime Contribution Wilhelm Konrad Rontgen for the discovery of x-rays Hendrik Antoon Lorentz Pieter Zeeman for their work on the influence of magnetism on radiation. Antoine Henri Becquerel Pierre Curie Marie Sklowdowska-Curie for his discovery of radioactivity. for their joint research on nuclear radiation phenomena. Lord Rayleigh (John William Strutt) for his research on the densities of the gases and for his discovery of argon Philipp Eduard Anton von Lenard for his work on cathode rays. Joseph John Thomson for his research on the conduction of electricity by gases. Albert Abraham Michelson for his optical instruments and for measuring the speed of light. Gabriel Lippmann for his method of reproducing colors photographically based on the interference techiniques.

64. A Short History Of Leiden University s first university lowtemperature laboratory, professor heike Kamerlingh Onnesachieved temperatures of Kamerlingh Onnes was awarded the nobel Prize for http://www.etcl.nl/ip/index.php?module_id=22

65. Www.npac.syr.edu/textbook/kidsweb/physics/nobel.txt I. Chase The following is a complete listing of nobel Prize awards 1912 Nils GustafDalen Automatic gas flow regulators 1913 heike Kamerlingh Onnes Matter at http://www.npac.syr.edu/textbook/kidsweb/physics/nobel.txt

The Nobel Prize for Physics (1901-1993) updated 15-OCT-1993 by SIC - original by Scott I. Chase The following is a complete listing of Nobel Prize awards, from the first award in 1901. Prizes were not awarded in every year. The description following the names is an abbreviation of the official citation. 1901 Wilhelm Konrad Rontgen X-rays 1902 Hendrik Antoon Lorentz Magnetism in radiation phenomena Pieter Zeeman 1903 Antoine Henri Bequerel Spontaneous radioactivity Pierre Curie Marie Sklowdowska-Curie 1904 Lord Rayleigh Density of gases and (a.k.a. John William Strutt) discovery of argon 1905 Pilipp Eduard Anton von Lenard Cathode rays 1906 Joseph John Thomson Conduction of electricity by gases 1907 Albert Abraham Michelson Precision meteorological investigations 1908 Gabriel Lippman Reproducing colors photographically based on the phenomenon of interference 1909 Guglielmo Marconi Wireless telegraphy Carl Ferdinand Braun 1910 Johannes Diderik van der Waals Equation of state of fluids 1911 Wilhelm Wien Laws of radiation of heat 1912 Nils Gustaf Dalen Automatic gas flow regulators 1913 Heike Kamerlingh Onnes Matter at low temperature 1914 Max von Laue Crystal diffraction of X-rays 1915 William Henry Bragg X-ray analysis of crystal structure William Lawrence Bragg 1917 Charles Glover Barkla Characteristic X-ray spectra of elements 1918 Max Planck Energy quanta 1919 Johannes Stark Splitting of spectral lines in E fields 1920 Charles-Edouard Guillaume Anomalies in nickel steel alloys 1921 Albert Einstein Photoelectric Effect 1922 Niels Bohr Structure of atoms 1923 Robert Andrew Millikan Elementary charge of electricity 1924 Karl Manne Georg Siegbahn X-ray spectroscopy 1925 James Franck Impact of an electron upon an atom Gustav Hertz 1926 Jean Baptiste Perrin Sedimentation equilibrium 1927 Arthur Holly Compton Compton effect Charles Thomson Rees Wilson Invention of the Cloud chamber 1928 Owen Willans Richardson Thermionic phenomena, Richardson's Law 1929 Prince Louis-Victor de Broglie Wave nature of electrons 1930 Sir Chandrasekhara Venkata Raman Scattering of light, Raman effect 1932 Werner Heisenberg Quantum Mechanics 1933 Erwin Schrodinger Atomic theory Paul Adrien Maurice Dirac 1935 James Chadwick The neutron 1936 Victor Franz Hess Cosmic rays Carl D. Anderson The positron 1937 Clinton Joseph Davisson Crystal diffraction of electrons George Paget Thomson 1938 Enrico Fermi New radioactive elements 1939 Ernest Orlando Lawrence Invention of the Cyclotron 1943 Otto Stern Proton magnetic moment 1944 Isador Isaac Rabi Magnetic resonance in atomic nuclei 1945 Wolfgang Pauli The Exclusion principle 1946 Percy Williams Bridgman Production of extremely high pressures 1947 Sir Edward Victor Appleton Physics of the upper atmosphere 1948 Patrick Maynard Stuart Blackett Cosmic ray showers in cloud chambers 1949 Hideki Yukawa Prediction of Mesons 1950 Cecil Frank Powell Photographic emulsion for meson studies 1951 Sir John Douglas Cockroft Artificial acceleration of atomic Ernest Thomas Sinton Walton particles and transmutation of nuclei 1952 Felix Bloch Nuclear magnetic precision methods Edward Mills Purcell 1953 Frits Zernike Phase-contrast microscope 1954 Max Born Fundamental research in QM Walther Bothe Coincidence counters 1955 Willis Eugene Lamb Hydrogen fine structure Polykarp Kusch Electron magnetic moment 1956 William Shockley Transistors John Bardeen Walter Houser Brattain 1957 Chen Ning Yang Parity violation Tsung Dao Lee 1958 Pavel Aleksejevic Cerenkov Interpretation of the Cerenkov effect Il'ja Mickajlovic Frank Igor' Evgen'evic Tamm 1959 Emilio Gino Segre The Antiproton Owen Chamberlain 1960 Donald Arthur Glaser The Bubble Chamber 1961 Robert Hofstadter Electron scattering on nucleons Rudolf Ludwig Mossbauer Resonant absorption of photons 1962 Lev Davidovic Landau Theory of liquid helium 1963 Eugene P. Wigner Fundamental symmetry principles Maria Goeppert Mayer Nuclear shell structure J. Hans D. Jensen 1964 Charles H. Townes Maser-Laser principle Nikolai G. Basov Alexander M. Prochorov 1965 Sin-Itiro Tomonaga Quantum electrodynamics Julian Schwinger Richard P. Feynman 1966 Alfred Kastler Study of Hertzian resonance in atoms 1967 Hans Albrecht Bethe Energy production in stars 1968 Luis W. Alvarez Discovery of many particle resonances 1969 Murray Gell-Mann Quark model for particle classification 1970 Hannes Alfven Magneto-hydrodynamics in plasma physics Louis Neel Antiferromagnetism and ferromagnetism 1971 Dennis Gabor Principles of holography 1972 John Bardeen Theory of superconductivity Leon N. Cooper J. Robert Schrieffer 1973 Leo Esaki Tunneling in superconductors Ivar Giaever Brian D. Josephson Super-current through tunnel barriers 1974 Antony Hewish Discovery of pulsars Sir Martin Ryle Pioneering radioastronomy work 1975 Aage Bohr Structure of the atomic nucleus Ben Mottelson James Rainwater 1976 Burton Richter Discovery of the J/Psi particle Samual Chao Chung Ting 1977 Philip Warren Anderson Electronic structure of magnetic and Nevill Francis Mott disordered solids John Hasbrouck Van Vleck 1978 Pyotr Kapitsa Liquifaction of helium Arno A. Penzias Cosmic Microwave Background Radiation Robert W. Wilson 1979 Sheldon Glashow Electroweak Theory, especially Steven Weinberg weak neutral currents Abdus Salam 1980 James Cronin Discovery of CP violation in the Val Fitch asymmetric decay of neutral K-mesons 1981 Kai M. Seigbahn High resolution electron spectroscopy Nicolaas Bleombergen Laser spectroscopy Arthur L. Schawlow 1982 Kenneth G. Wilson Critical phenomena in phase transitions 1983 Subrahmanyan Chandrasekhar Evolution of stars William A. Fowler 1984 Carlo Rubbia Discovery of W,Z Simon van der Meer Stochastic cooling for colliders 1985 Klaus von Klitzing Discovery of quantum Hall effect 1986 Gerd Binning Scanning Tunneling Microscopy Heinrich Rohrer Ernst August Friedrich Ruska Electron microscopy 1987 Georg Bednorz High-temperature superconductivity Alex K. Muller 1988 Leon Max Lederman Discovery of the muon neutrino leading Melvin Schwartz to classification of particles in Jack Steinberger families 1989 Hans Georg Dehmelt Penning Trap for charged particles Wolfgang Paul Paul Trap for charged particles Norman F. Ramsey Control of atomic transitions by the separated oscillatory fields method 1990 Jerome Isaac Friedman Deep inelastic scattering experiments Henry Way Kendall leading to the discovery of quarks Richard Edward Taylor 1991 Pierre-Gilles de Gennes Order-disorder transitions in liquid crystals and polymers 1992 Georges Charpak Multiwire Proportional Chamber 1993 Russell A. Hulse Discovery of the first binary pulsar Joseph H. Taylor and subsequent tests of GR

66. Zeal.com - United States - New - Library - Sciences - Physics - Physicists - Phy 13. Kamerlingh Onnes, heike 1913 nobel Prize http//www.nobel.se/physics/laureates/1913/Read about how this Dutch scientist's studies of matter at low http://www.zeal.com/category/preview.jhtml?cid=331341

67. Nobel Prizes In Physics [UWA Physics] The following is a complete listing of nobel Prize awards in Physics 1912 Nils GustafDalen Automatic gas flow regulators 1913 heike Kamerlingh Onnes Matter at http://www.physics.uwa.edu.au/Misc/nobel.html

Nobel Prizes in Physics The following is a complete listing of Nobel Prize awards in Physics, from the first award in 1901. Prizes were not awarded in every year. The description following the names is an abbreviation of the official citation:

68. Premio Nobel De Física - Wikipedia Translate this page 1917 Charles Glover Barkla 1915 Sir William Henry Bragg, William Lawrence Bragg 1914Max von Laue 1913 heike Kamerlingh Onnes 1912 Nils See also Premio nobel, http://es.wikipedia.org/wiki/Premio_Nobel/Física

Portada Cambios Recientes Edita esta página Historia Páginas especiales Preferencias de usuario Mi lista de seguimiento Cambio Recientes Subir una imagen Lista de imágenes Usuarios registrados Estadísticas del sitio Artículo aleatorio Artículos huérfanos Imágenes huérfanas Artículos populares Artículos más solicitados Artículos cortos Artículos largos Artículos nuevos Todas las páginas (alfabético) Direcciones IP bloqueadas Página de mantención Fuentes externas de libros Versión para imprimir Discusión Registrase/Entrar Ayuda Otros idiomas: Dansk(Danés) English (Inglés) Esperanto Nederlands (Holandés) Premio Nobel de Física (Redirigido desde Premio Nobel/Física Ver enlace: http://www.nobel.se/physics/laureates/index.html Raymond Davis, Masatoshi Koshiba, Riccardo Giacconi Eric A. Cornell, Wolfgang Ketterle, Carl E. Wieman Zhores I. Alferov, Herbert Kroemer, Jack S. Kilby Gerardus 't Hooft Martinus J.G. Veltman Robert B. Laughlin, Horst L. Störmer, Daniel C. Tsui Steven Chu, Claude Cohen-Tannoudji, William D. Phillips David M. Lee, Douglas D. Osheroff, Robert C. Richardson Martin L. Perl, Frederick Reines

69. B APPENDIX A /b 1911 Dutch physicist heike Kamerlingh Onnes discovers superconductivity in mercuryat temperature of 4 K. 1913 Kamerlingh Onnes is awarded the nobel Prize in http://www.ornl.gov/reports/m/ornlm3063r1/app_a.html

APPENDIX A SUPERCONDUCTIVITY MILESTONES Dutch physicist Heike Kamerlingh Onnes discovers superconductivity in mercury at temperature of 4 K. Kamerlingh Onnes is awarded the Nobel Prize in Physics for his research on the properties of matter at low temperature. W. Meissner and R. Ochsenfeld discover the Meissner Effect. Scientists report superconductivity in niobium nitride at 16 K. Vanadium-3 silicon found to superconduct at 17.5 K. Westinghouse scientists develop the first commercial niobium- titanium superconducting wire. John Bardeen, Leon Cooper, and John Schrieffer win the Nobel Prize in Physics for the first successful theory of how superconductivity works. Scientific groups at the University of Houston and the University of Alabama at Huntsville substitute yttrium for lanthanum and make a ceramic that superconducts at 92 K, bringing superconductivity into the liquid nitrogen range. A. Schilling, M. Cantoni, J. D. Guo, and H. R. Ott from Zurich, Switzerland, produces a superconductor from mercury, barium and copper, (HgBa Ca Cu O ) with maximum transition temperature of 133K.

70. HISTORICAL BACKGROUND in 1911 by the Dutch physicist,heike Kammerlingh Onnes Kamerlingh Onnes called thisnewly discovered state, Superconductivity and was awarded the nobel Prize in http://www.ornl.gov/reports/m/ornlm3063r1/pt2.html

HISTORICAL BACKGROUND Major advances in low-temperature refrigeration were made during the late 19th century. Superconductivity was first discovered in 1911 by the Dutch physicist,Heike Kammerlingh Onnes. Onnes dedicated his scientific career to exploring extremely cold refrigeration. On July 10, 1908, he successfully liquified helium by cooling it to 452 degrees below zero Fahrenheit (4 Kelvin or 4 K). Onnes produced only a few milliliters of liquid helium that day, but this was to be the new beginnings of his explorations in temperature regions previously unreachable. Liquid helium enabled him to cool other materials closer to absolute zero (0 Kelvin), the coldest temperature imaginable. Absolute zero is the temperature at which the energy of material becomes as small as possible. In 1911, Onnes began to investigate the electrical properties of metals in extremely cold temperatures. It had been known for many years that the resistance of metals fell when cooled below room temperature, but it was not known what limiting value the resistance would approach, if the temperature were reduced to very close to K. Some scientists, such as William Kelvin, believed that electrons flowing through a conductor would come to a complete halt as the temperature approached absolute zero. Other scientists, including Onnes, felt that a cold wire's resistance would dissipate. This suggested that there would be a steady decrease in electrical resistance, allowing for better conduction of electricity. At some very low temperature point, scientists felt that there would be a leveling off as the resistance reached some ill-defined minimum value allowing the current to flow with little or no resistance.Onnes passed a current through a very pure mercury wire and measured its resistance as he steadily lowered the temperature. Much to his surprise there was no leveling off of resistance, let alone the stopping of electrons as suggested by Kelvin. At 4.2 K the resistance suddenly vanished. Current was flowing through the mercury wire and nothing was stopping it, the resistance was zero.

71. Superconductivity Find a good quote from Onnes' nobel speech. 1911, 4.154, Hg (superconductivitydiscovered) heike Kamerlingh Onnes, Georg Holst Universiteit Leiden. http://hypertextbook.com/physics/modern/superconductivity/

72. Errore Translate this page ERA IL 1911, quando un fisico olandese, chiamato heike Kamerlingh Onnes, scoprìla dei suoi studi sulle basse temperature Onnes ricevette il premio nobel. http://www.enel.it/it/enel/magazine/boiler/boiler46/html/articoli/FocusUngaro-St

Siamo spiacenti, Certi della vostra collaborazione ci scusiamo per l' inconveniente tecnico.

73. Superconductor History superconductivity was first observed in mercury by Dutch physicist heike KamerlinghOnnes of Leiden Later, in 1913, he won a nobel Prize in physics for his http://superconductors.org/History.htm

VISITOR ALERT: We have detected that your browser is not Java-enabled. Please enable Java and Java Script by clicking on your Browser's "PREFERENCES" area. If you don't not wish to enable Java, you will not be able to view all of the information available on this website. Java is used extensively. T h e H i s t o r y o f S u p e r c o n d u c t o r s Superconductors , materials that have no resistance to the flow of electricity, are one of the last great frontiers of scientific discovery. Not only have the limits of superconductivity not yet been reached, but the theories that explain superconductor behavior seem to be constantly under review. In 1911 superconductivity was first observed in mercury by Dutch physicist Heike Kamerlingh Onnes of Leiden University (shown above). When he cooled it to the temperature of liquid helium, 4 degrees Kelvin (-452F, -269C), its resistance suddenly disappeared. The Kelvin scale represents an "absolute" scale of temperature. Thus, it was necessary for Onnes to come within 4 degrees of the coldest temperature that is theoretically attainable to witness the phenomenon of superconductivity. Later, in 1913, he won a Nobel Prize in physics for his research in this area. The next great milestone in understanding how matter behaves at extreme cold temperatures occurred in 1933. Walter Meissner and Robert Ochsenfeld discovered that a superconducting material will repel a magnetic field (see above graphic). A magnet moving by a conductor induces currents in the conductor. This is the principle upon which the electric generator operates. But, in a superconductor the induced currents exactly mirror the field that would have otherwise penetrated the superconducting material - causing the magnet to be repulsed. This phenomenon is known as diamagnetism and is today often referred to as the "Meissner effect". The Meissner effect is so strong that a magnet can actually be

74. FÍSICA - SUPERCONDUTIVIDADE Translate this page A supercondutividade foi descoberta em 1911 pelo holandês heike Kamerlingh Onnes. essateoria, Bardeen, Cooper e Schrieffer ganharam o prêmio nobel de 1972. http://www.fisica.ufc.br/supercondutividade.htm

A SUPERCONDUTIVIDADE A supercondutividade foi descoberta em 1911 pelo holandês Heike Kamerlingh Onnes. Um metal a temperatura ambiente tem resistência elétrica pequena mas não nula. Quando a temperatura baixa a resistência do metal também diminui. Que acontece se a temperatura baixar tanto que se aproxime do zero absoluto? Essa questão foi muito debatida no início desse século. Onnes achava que a resistência deveria diminuir cada vez mais, chegando a zero no zero absoluto. Ele achava que as vibrações dos átomos do metal, que dificultam o deslocamento dos elétrons e causam a resistência, deveriam cessar no zero absoluto. Nesse caso, a resistência elétrica cairia a zero gradualmente. Já Lord Kelvin previa que os próprios elétrons deveriam se "congelar" no zero absoluto. Assim, a resistência elétrica na temperatura zero seria infinita. Para resolver esse debate só medindo a resistência dos metais em baixíssimas temperaturas. Ninguém melhor para isso que o próprio Onnes que dispunha do melhor laboratório de baixas temperaturas do mundo na época. Ele conseguira liquefazer o gás hélio em 1908, atingindo temperaturas abaixo de 4 graus absolutos. NOTA: hoje dizemos 4 Kelvins ( e não 4 graus Kelvin). A escala absoluta de temperaturas homenageia o velho Lord. Só que, no caso do debate sobre a resistência a zero Kelvins, o inglês errou feio.

75. Superconductividad: La Resistencia Es Inútil Translate this page La superconductividad fue descubierta en 1911 por el físico holandés heike KamerlinghOnnes. un descubrimiento histórico Onnes recibió el nobel de física http://www.arrakis.es/~cris/supercon.htm

llamada fonones gap BIBLIOGRAFIA VOLVER A LA PAGINA PRINCIPAL

76. Ficha 2 Ficha 2 (e). Listado de PREMIOS nobel europeos*. flecha.gif (1003 bytes). Waals,Johannes D. Van der (1910). Kamerlingh Onnes, heike (1913) Zernike, Frits (1953). http://www.euro.mineco.es/guiadidactica/guia4/FCHAU2E.htm

Ficha 2 (e) Listado de PREMIOS NOBEL europeos* GRECIA LITERATURA Seferiades, Giorgios (1963) Elitis, Odiseo (1979) HOLANDA QUÍMICA Van´t Hoff, Jacobus H. (1901) Crutzen, Paul (1995) FÍSICA Lorentz, Hendrik A. (1902) Zeeman, Pieter (1902) Waals, Johannes D. Van der (1910) Kamerlingh Onnes, Heike (1913) Zernike, Frits (1953) Van der Meer, Simon (1984) FISIOLOGÍA/MEDICINA Einthoven, Willem (1924) Eijkman, Christian (1929) Tinbergen, Nikolaas (1973) PAZ Asser, Tobias M.C. (1911) CIENCIAS ECONÓMICAS Tinbergen, Jan (1969) ITALIA LITERATURA Carducci, Giosué (1906) Deledda, Grazia (1926) Pirandello, Luigi (1934) Quasimodo, Salvatore (1959) Montale, Eugenio (1975 QUÍMICA Natta, giulio (1963) FÍSICA Marconi, Guglielmo (1909) Fermi, Enrico (1938) Rubbia, Carlo (1984) FISIOLOGÍA/MEDICINA Golgi, Camillo (1906) Bovet, Daniel (1957) Levi-Montalcini, Rita (1986) PAZ Moneta, Ernesto T. (1907) IRLANDA LITERATURA Yeats, William Butler (1923) Beckett, Samuel (1969) Heaney, Seamus (1995) FÍSICA Walton, Ernst T.S. (1951) PAZ MacBride, Sean (1974) Corrigan, Mairead (1976) Williams, Betty (1976)

77. Premi Nobel Fisica Translate this page 1915, SIR WILLIAM HENRY BRAGG - SIR WILLIAM LAWRENCE BRAGG. 1914, MAX VON LAUE.1913, heike KAMERLINGH - ONNES. 1912, NILS GUSTAF DALEN. 1911, WILHELM WIEN. http://www.econofisica.com/premi nobel fisica.htm

ANNO PREMIATO ZHORES I. ALFEROV - HERBERT KROEMER JACK ST. CLAIR KILBY GERARDUS 'T HOOFT - MARTINUS J.G. VELTMAN ROBERT B. LAUGHLIN - HORST L. STORMER - DANIEL C. TSUI STEVEN CHU - CLAUDE COHEN TANNOUDJI - WILLIAM D. PHILLIPS DAVID M. LEE - DOUGLAS D. OSHEROFF - ROBERT C. RICHARDSON MARTIN L. PERL - FREDERICK REINES BERTRAM N. BROCKHOUSE - CLIFFORD G. SHULL RUSSEL A. HULSE - JOSERPH H. TAYLOR JR GEORGES CHARPAK PIERRE-GILLES DE GENNES JEROME I. FRIEDMAN - HENRY W. KENDALL - RICHARD E. TAYLOR NORMAN F. RAMSEY - HANS G. DEHMELT - WOLFGANG PAUL LEON M. LEDERMAN - MELVIN SCHWARTZ - JACK STEINBERGER J. GEORG BEDNORZ - K. ALEXANDER MULLER ERNST RUSKA - GERD BINNIG - HEINRICH ROHRER KLAUS VON KLITZING CARLO RUBBIA - SIMON VAN DER MEER SUBRAMANYAN CHANDRASEKHAR - WILLIAM A. FOWLER KENNETH G. WILSON NICOLAAS BLOEMBERGEN - ARTHUR L. SCHAWLOW - KAI M. SIEGBAHN JAMES W. CRONIN - VAL L. FITCH SHELDON L. GLASHOW - ABDUS SALAM - STEVEN WEINBERG

78. 1911-1920 Translate this page 1911. heike KAMERLINGH ONNES SCOPRE. il limite irraggiungibile di temperatura cheera stato stabilito dal fisico tedesco Walter Nemst (1 864-1941 - nobel nel 1920 http://web.tiscali.it/no-redirect-tiscali/dannad/photo.htm

Cronologia storica Home Scoperte Elettroniche Bibbliografia Info ... Home HEIKE KAMERLINGH ONNES SCOPRE LA SUPERCONDUTIVITA' Il fisico olandese (1853-1926) riesce a liquefare l'elio a 4 gradi Kelvin (v.) e successivamente riesce a raggiungere la temperatura di 1 grado Kelvin, cioè un grado al di sopra dello zero assoluto, il limite irraggiungibile di temperatura che era stato stabilito dal fisico tedesco Walter Nemst (1 864-1941 - Nobel nel 1920). Studiando il comportamento della materia a queste temperature, KamerUngh Onnes scopre che la resistenza elettrica di alcuni metalli a 4 kelvin si annulla completamente. Chiama il fenomeno « superconduttività». La superconduttività si rivelerà di grande importanza negli anni '70 e '80 nella costruzione di acceleratori di particelle e resterà legata a queste bassissime temperature finché nel 1986 Mufler e Bednorz non realizzeranno materiali in grado di presentare questo fenomeno a temperature molto più elevate. Per la sua scoperta, Kamerlingh Onnes otterrà il Nobel nel 1913. ERNEST RUTHERFORD PRFSENTA LA TEORIA DELL'ATOMO CHARLES WILSON REALIZZA LA «CAMERA A NEBBIA»

79. NOBEL Per La FISICA Translate this page nobel per la FISICA Solvay 1927 1901. Röentgen, Wilhelm C. (Germania). 1902. 1912.Dalén, Nils Gustaf (Svezia). 1913. Kamerlingh Onnes, heike (Paesi Bassi). 1914. http://digilander.libero.it/andreawentura/fisica/nobel.htm

NOBEL per la FISICA Solvay 1927 Röentgen, Wilhelm C. (Germania) Lorentz, Hendrik A. (Paesi Bassi) Zeeman, Pieter (Paesi Bassi) Curie, Pierre (Francia) Curie, Marie (Francia) Becquerel, Antoine H. (Francia) Rayleigh, John W. (Gran Bretagna) Lenard, Philipp (Germania) Thomson, Joseph John (Gran Bretagna) Michelson, Albert A. (USA) Lippmann, Gabriel (Francia) Marconi, Guglielmo (Italia) Braun, Karl F. (Germania) Waals, Johannes D. van der (Paesi Bassi) Wien, Wilhelm (Germania) Dalén, Nils Gustaf (Svezia) Kamerlingh Onnes, Heike (Paesi Bassi) Laue, Max von (Germania) Bragg, William H. (Gran Bretagna) Bragg, William L. (Gran Bretagna) Non assegnato Barkla, Charles G. (Gran Bretagna) Planck, Max Karl E.L. (Germania) Stark, Johannes (Germania) Guillaume, Charles E. (Francia) Einstein, Albert (USA) Bohr, Niels Henrik D. (Danimarca) Millikan, Robert A. (USA) Siegbahn, Karl M.G. (Svezia) Franck, James (Germania) Herz, Gustav (Germania)

80. Physics 1913 b.1853 d.1926. The nobel Prize in Physics 1913 Presentation Speech HeikeKamerlingh Onnes Biography nobel Lecture Swedish nobel Stamps. 1912, 1914. http://www.nobel.se/physics/laureates/1913/

The Nobel Prize in Physics 1913 "for his investigations on the properties of matter at low temperatures which led, inter alia, to the production of liquid helium" Heike Kamerlingh Onnes the Netherlands Leiden University Leiden, the Netherlands b.1853 d.1926 The Nobel Prize in Physics 1913 Presentation Speech Heike Kamerlingh Onnes Biography ... Swedish Nobel Stamps The 1913 Prize in: Physics Chemistry Physiology or Medicine Literature ... Peace Find a Laureate: Last modified June 16, 2000 The Official Web Site of The Nobel Foundation

A  B  C  D  E  F  G  H  I  J  K  L  M  N  O  P  Q  R  S  T  U  V  W  X  Y  Z

Page 4     61-80 of 87    Back | 1  | 2  | 3  | 4  | 5  | Next 20