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The Development of the Electron Microscope and of Electron MicroscopyScanning Tunneling Microscopy – From Birth to Adolescence Scanning Tunneling Microscopy – From Birth to Adolescence
"for his fundamental work in electron
optics, and for the design of the first electron microscope"
"for their design of the scanning
tunneling microscope"
Autobiography: Ernst RuskaI was born on 25 December 1906 in Heidelberg as the
fifth of seven children of Professor Julius Ruska and his wife Elisbeth (née
Merx). After graduating from grammar school in Heidelberg I studied
electronics at the Technical College in Munich, studies which I began in
the autumn of 1925 and continued two years later in Berlin. I received my
practical training from Brown-Boveri & Co in Mannheim and Siemens & Halske
Ltd in Berlin. Whilst still a student at the Technical College in Berlin I
began my involvement with high voltage and vacuum technology at the
Institute of High Voltage, whose director was Professor Adolf Matthias.
Under the direct tutelage of Dr Max Knoll and together with other doctoral
students I worked on the development of a high performance cathode ray
oscilloscope. On the one hand my interest lay principally in the
development of materials for the building of vacuum instruments according
to the principles of construction; on the other it lay in continuing
theoretical lectures and practical experiments in the optical behaviour of
electron rays. (added by the editor): Ernst Ruska died on May 25, 1988.
Autobiography: I was born in Frankfurt, W. Germany, on 7.20., '47 as
the first of two sons. My childhood was very much influenced by the Second
World War, which had only just ended. We children had great fun playing
among the ruins of the demolished buildings, but naturally were too young
to realize that much more than just buildings had been destroyed. (added in 1991:)
Autobiography: I was born in Buchs, St. Gallen, Switzerland on 6.6., '33 as the third child, half an hour after my twin sister. We were fortunate to enjoy a carefree childhood with a sound mixture of freedom, school and farm work. In 1949, the family moved to Zürich and our way of life changed from country to town. My finding to physics was rather accidental. My natural bent was towards classical languages and natural sciences, and only when I had to register at the ETH (Swiss Federal Institute of Technology) in autumn 1951, did I decide in favor of physics. In the next four years, Professors G. Busch, W. Pauli, and P. Scherrer taught me the rudiments. In autumn 1955, I started work on my Ph.D. Thesis and it was fortuitous that Jörgen Lykke Olsen trusted me to measure the length changes of superconductors at the magnetic-field-induced superconducting transition. He had already pioneered the field with measurements on the discontinuity of Young's modulus. Following in his footsteps, I lost all respect for angstroms. The mechanical transducers were very vibration sensitive, and I learned to work after midnight, when the town was asleep. My four graduate years were a most memorable time, in a group of distinguished graduate students always receptive for fun, and including the interruptions by my basic training courses in the Swiss mountain infantry.In summer 1961, Rose-Marie Egger became my wife, and her stabilizing influence has kept me on an even keel ever since. Our honeymoon trip led us to the United States where I spent two post-doe years working on thermal conductivity of type-II superconductors and metals in the group of Professor Bernie Serin at Rutgers University in New Jersey. Then in the summer of 1963, Professor Ambros Speiser, Director of the newly founded IBM Research Laboratory in Rüschlikon, Switzerland, made me an offer to join the physics effort there. Encouraged by Bruno Lüthi, who later became a Professor at the University of Frankfurt, and, at the time, strongly recommended the hiring of Gerd Binnig, I accepted to start in December 1963, after having responded to the call of the wild in the form of a four-month camping trip through the USA. My first couple of years in Rüschlikon were spent studying mainly Kondo systems with magnetoresistance in pulsed magnetic fields. End of the sixties, Keith Blazey interested me to work on GdAlO3, an antiferromagnet on which he had done optic experiments. This started a fruitful cooperation on magnetic phase diagrams, which eventually brought me into the field of critical phenomena. Encouraged by K. Alex Müller, who had pioneered the critical-phenomena effort in our Laboratory, I focused on the bicritical and tetracritical behavior and finally on the random-field problem. These were most enjoyable years, during which so many patient colleagues taught me physics. I left them with some regret, when I ventured with Gerd to discover new shores. We found them. Thank you, Gerd. In 1974/75, I spent a sabbatical year with Professor Vince Jaccarino and Dr. Alan King at the University of California in Santa Barbara, to get a taste of nuclear magnetic resonance. We solved a specific problem on the bicritical point of MnF2, their home-base material. We traded experience, NMR and critical phenomena. Rose-Marie and I also took the opportunity at the beginning and end of my sabbatical to show the USA to our two daughters, Doris and Ellen, on two extended camping trips from coast to coast. In all the years with IBM Research, I have especially appreciated the freedom to pursue the activities I found interesting, and greatly enjoyed the stimulus, collegial cooperation, frankness, and intellectual generosity of two scientific communities, namely, in superconductivity and critical phenomena. I should also like to take this opportunity to thank the many, many friends, teachers, and seniors who have contributed towards my scientific career in any way whatsoever, and most particularly my mother for her unstinting aid and assistance, especially when times were difficult.
Scanning Tunneling Microscopy – From Birth to Adolescence
Scanning Tunneling Microscopy – From Birth to Adolescence Source: http://nobelprize.org/nobel_prizes/physics/laureates/1986/index.html
CPH Stands of: Creative Particle of Higgs that propounded by Hossein Javadi in 1987 Biography
Download of GSJ;
Hossein Javadi, F. Forouzbakhsh Mar. 21, 2006: Logical Foundation of CPH Theory [PDF] Persian TranslationMar. 21, 2006: English Experimental Foundation of CPH Theory [PDF] Persian Translation Mar. 21, 2006: English Definition, Principle and Explanation of CPH Theory [PDF] Persian Translation Mar. 23, 2006: English Analysis of CPH Theory [PDF] Persian Translation Apr. 7, 2006: English Opinions on CPH Theory [PDF] Persian Translation Apr. 7, 2006: English Questions and Answers on CPH Theory [PDF] Persian Translation Apr. 11, 2006: English Realization Hawking - End of Physics by CPH [PDF] Persian Translation Only Apr. 12, 2006: English Maxwell's Equations in a Gravitational Field [PDF] Persian Translation Apr. 17, 2006: English Effective Nuclear Charge [PDF] Persian Translation Apr. 28, 2006: Color Charges Curve Space [PDF] Persian TranslationMay. 14, 2006:English Speed of Light and CPH Theory [PDF] Persian Translation Mar. 19, 2006: Sub-Quantum Chromodynamics [PDF]Mar. 19, 2006: Color Charge/Color Magnet and CPH [PDF]
H. Poor Imani, S. Hoghoghi Esfahani:
H. Poor Imani: Download of CPH Theory site Section 1; Logical Foundation of CPH Theory PDF DOC HTM Section 2; Experimental Foundation of CPH Theory PDF DOC HTM Section 3; Theory of CPH; Formats Defination and Principle of CPH PDF DOC HTM Section 4; Analysis of CPH Theory PDF DOC HTM Section Five; Opinions About CPH Theory PDF DOC HTM Section six; Questions and answers CPH Theory PDF DOC HTM Section Nine; Maxwell equations in gravitational Field PDF DOC HTM Section Ten; Effective Nuclear Charge PDF DOC HTM Section Eleven; Color Charges Curve Space PDF DOC HTM Section 12; Speed of Light and CPH Theory PDF DOC HTMTime Function and Absolute Black Hole PDF H. Poor Imani: Time, Revolution and Spin PDF DOC H. Poor Imani and Salman Hoghoghi: Time, Revolution and Biological Time PDF All Nobel Laureates in PhysicsContains: names, biographies and lectutures
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faster than light!
faster than light!
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Strong Interaction and CPH Theory [PDF]
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Quantum Electrodynamics and CPH Theory [PDF]
Vocabulary of CPH Theory [PDF]
Thermodynamic Laws, Entropy and CPH Theory [PDF]
Time Function and Absolute Black Hole [PDF]
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A New Mechanism of Higgs Bosons in Producing Charge Particles [PDF] Persian Text
Logical Foundation of CPH Theory [PDF] Persian Text
Experimental Foundation of CPH Theory [PDF] Persian Text
Definition, Principle and Explanation of CPH Theory [PDF] Persian Text
Analysis of CPH Theory Persian Text
Opinions on CPH Theory [PDF] Persian Text
Questions and Answers on CPH Theory [PDF] Persian Text
Realization Hawking - End of Physics by CPH [PDF]Persian Text Only
Maxwell's Equations in a Gravitational Field [PDF] Persian Text
Effective Nuclear Charge [PDF] Persian Text
Color Charges Curve Space [PDF] Persian Text
Sub-Quantum Chromodynamics [PDF]
Color Charge/Color Magnet and CPH [PDF]
Speed of Light and CPH Theory [PDF] Persian Text
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