Nobel 1917 |
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Characteristic Röntgen Radiation
"for his discovery of the characteristic Röntgen radiation of the
elements"
Biography Charles Glover Barkla was born on June 7, 1877 at Widnes, Lancashire, England, where his father, J.M. Barkla, was Secretary to the Atlas Chemical Company. He was educated at the Liverpool Institute and entered University College, Liverpool, in 1894 to study mathematics and physics, the latter under Oliver Lodge. He graduated with First Class Honours in Physics in 1898 and in the following year he obtained his master's degree. Also in 1899, he was awarded a research scholarship by the Royal Commissioners for the Exhibition of 1851 and he proceeded to Trinity College, Cambridge, to work in the Cavendish Laboratory with J. J. Thomson. He migrated to King's College during 1900 and in 1902 returned to Liverpool as Oliver Lodge Fellow. From 1905 to 1909 he was successively demonstrator, assistant lecturer in physics and special lecturer in advanced electricity at the University, and in 1909 he succeeded H. A. Wilson as Wheatstone Professor of Physics in the University of London. In 1913, Barkla accepted the Chair in Natural Philosophy in the University of Edinburgh and he held this position until his death.Barkla's first researches concerned the velocity of electric waves along wires but in 1902 he commenced his investigations on Röntgen radiation which were to occupy almost his whole life. His discovery of homogeneous radiations characteristic of the elements showed that these elements had their characteristic line spectra in X-ray and he was the first to show that secondary emission is of two kinds, one consisting of X-rays scattered unchanged, and the other a fluorescent radiation peculiar to the particular substance. He discovered the polarisation of X-rays, an experimental result of considerable importance for it meant that X-radiation could be regarded as similar to ordinary light. Barkla made valuable contributions to present knowledge on the absorption and photographic action of X-rays and his later work demonstrated the relation between the characteristic X-radiation and the corpuscular radiation accompanying it. He has also shown both the applicability and the limitation of the quantum theory in relation to Röntgen radiation. The results of his findings are recorded in various papers which have appeared mainly in the Transactions and Proceedings of the Royal Society. He had a considerable reputation as an examiner in physics. Barkla, a Fellow of the Royal Society, had several honorary degrees. He was appointed Bakerian Lecturer (Royal Society) in 1916 and he was awarded the Hughes Medal in the following year. Charles Glover Barkla married Mary Esther, the eldest daughter of John T. Cowell of Douglas, Receiver-General of the Isle of Man, in 1907. They had two sons and one daughter. Their youngest son, Flight Lieutenant Michael Barkla, a brilliant scholar, was killed in action in 1943. Barkla's chief recreation was singing - he had a powerful baritone voice and he was a member of the King's College Chapel Choir, 1901-1902. Latterly, he had also become fond of golf. Barkla died at his home, Braidwood, Edinburgh, on October 23, 1944. From Nobel Lectures, Physics 1901-1921, Elsevier Publishing Company, Amsterdam, 1967
Nobel Lecture Characteristic Röntgen Radiation Source: http://nobelprize.org/nobel_prizes/physics/laureates/1917/index.html
CPH Stands of: Creative Particle of Higgs that propounded by Hossein Javadi in 1987 Biography
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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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