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Optical Methods for Studying Hertzian Resonances
" for the discovery and development of optical methods for studying
Hertzian resonances in atoms"
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Alfred Kastler |
| France |
École Normale Supérieure
Paris, France |
b. 1902
d. 1984 |
Biography
Alfred Kastler was born in Guebwiller in Alsace on May 3, 1902. He
followed his early studies at the school in his native town, and continued
at the Oberrealschule of Colmar, which became the Lycee Bartholdi in 1918,
when Alsace was returned to France.
He entered the École Normale Superieure in 1921, and left in 1926 to teach
in a lycée. He taught for 5 years, first in the Mulhouse lycée, then in
those of Colmar and Bordeaux. The next stage of his career was in higher
education: assistant at the Bordeaux Faculty of Science from 1931 to 1936,
lecturer at Clermont-Ferrand from 1936 to 1938, professor at Bordeaux from
1938 to 1941. In 1941, in the midst of the German occupation, Georges
Bruhat asked him to come to Paris to help him in establishing physics
teaching at the Ecole Normale Superieure. The post was provisional, but
was confirmed by the allocation of a chair in a personal capacity at the
Paris Faculty of Sciences in 1952.
His mathematics teachers at the Colmar Lycée, Fröhlich from Bavaria and
Edouard Greiner from Alsace, were the first to awaken his interest in
science. This predilection became consolidated in the special mathematics
class held by Mahuet and Brunold, who helped Kastler to gain entry to the
École Normale Superieure by the side entrance, so to speak. In the
stimulating and friendly atmosphere of this college, the teacher Eugène
Bloch (who came from the upper Rhine and who subsequently disappeared
without trace in Auschwitz) initiated his students into the concepts of
Bohr's atom and quantum physics, and drew Kastler's attention to
Sommerfeld's book on atomic structure and spectral lines. This book
introduced him to the principle of the conservation of momentum applied by
A. Rubinowicz to the exchange of energy between atoms and radiation. This
principle was to guide the whole of Kastler's research, beginning with his
thesis up to the most recent investigations of the Parisian team.
Alfred Kastler was in 1931 appointed assistant to Pierre Daure, professor
at the Bordeaux Faculty of Science. His teaching duties were then less
onerous, and Kastler was able to devote all his free time to research,
aided by Professor Daure who initiated him into experimental spectroscopy.
For many years, he worked in the field of optical spectroscopy,
particularly on atomic fluorescence and Raman spectroscopy. [In I937 he
became interested in the luminescence of sodium atoms in the upper
atmosphere; after establishing that the D line of the twilight sky could
be absorbed by sodium vapour, and after some studies at Abisko where
twilight is prolonged, he was able to demonstrate in cooperation with his
colleague Jean Bricard, that this line is polarized, as it must be if the
emission mechanism is one of optical resonance produced by solar
radiation.]
During the years of the occupation, French scientists were virtually
isolated from the outside world. In 1945, it was possible to send pupils
to other western countries, so that they could bring their knowledge of
the most recent devel opments in scientific progress up to date. Among
them was Jean Brossel, who returned in 1951 in possession of a mass of
information gained under Francis Bitter at M.I.T.
Under the influence of Gorter,
Rabi had very successfully applied certain methods to the
investigation of atoms in their fundamental state. In 1949, Bitter
suggested extending these same methods to the excited states of atoms.
Brossel and Kastler together then proposed the " double resonance method
", which combines optical resonance with magnetic resonance.
While Brossel was at M.I.T., between 1949 and 1951, he carried out pioneer
work along these lines on the excited state of the mercury atom. At the
same time, Kastler was supplementing the method by the technique of
"optical pumping", which makes it possible to apply "optical methods for
studying the microwave resonances" to the fundamental states of atoms.
After 1951, Kastler worked in collaboration with Jean Brossel in Paris to
perfect all these methods. Among the young men and women at the École
Normale, which nurtures the intellectual elite, they found their research
workers. Their theses represent the various stages in their collective
work which has been awarded the Nobel Prize, and of which some account is
given in Kastler's Nobel lecture.
Kastler taught as Francqui Professor at the University of Louvain during
the year 1953-1954, he hold honorary doctorates from the University of
Louvain (1955), Pisa (1960), and Oxford (1966), and he was decorated by
the University of Liége.The French and Polish Societies of Physics and the
American Society of Optics have elected Kastler to honorary memberships.
In 1962, the latter society awarded him the first Mees medal bearing the
inscrip tion "Optics transcends all boundaries". In 1954, the British
Physical Society awarded him the prize commemorating Fernand Holweck, who
disappeared tragically in 1941. Kastler was made a member of the Royal
Flemish Academy of Belgium in 1954, and of the Paris Academy of Sciences
in 1964; in 1965, the National Centre for Scientific Research awarded him
their gold medal, at the same time as his friend and colleague
Louis Néel.
In Decermber 1924 Kastler married Elise Cosset, a former pupil of the
École Normale Supérieure. By working as a history teacher in secondary
schools she made it possible for her husband to devote to research all the
leisure time left to him by his own teaching duties. They have three
children: Daniel, born in 1926, Mireille born in 1928, and Claude-Yves
born in 1936. They have all married, there are now six grandchildren,
whose ages range from 14 years to 10 months. Daniel is a Professor of
Physics at the Faculty of Science in Marseilles, he is working on
theoretical physics problems; Mireille is an ophthalmologist in Paris, and
Claude-Yves teaches Russian at the Arts Faculty in Grenoble.
Nobel Lecture
Optical Methods for Studying Hertzian Resonances
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820 kb
Source:
http://nobelprize.org/nobel_prizes/physics/laureates/1966/index.html
CPH Stands
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Biography

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A New Definition for the Graviton
Mar. 21, 2006:
Logical Foundation of CPH Theory [PDF]
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21, 2006: English
Experimental Foundation of CPH Theory [PDF]
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Mar.
21, 2006: English
Definition, Principle and Explanation of CPH Theory [PDF]
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Mar.
23, 2006: English
Analysis of CPH Theory [PDF]
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Apr.
7, 2006: English
Opinions on CPH Theory [PDF]
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Apr.
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Questions and Answers on CPH Theory [PDF]
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Apr.
11, 2006: English
Realization Hawking - End of Physics by CPH [PDF]
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12, 2006: English
Maxwell's Equations in a Gravitational Field [PDF]
Persian Translation
Apr.
17, 2006: English
Effective Nuclear Charge [PDF]
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Apr. 28, 2006:
Color Charges Curve Space [PDF]
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May. 14,
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Speed of Light and CPH Theory
[PDF]
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Mar. 19, 2006:
Sub-Quantum Chromodynamics [PDF]
Mar.
19, 2006:
Color Charge/Color Magnet and CPH [PDF]
H. Poor Imani, S. Hoghoghi Esfahani:
Apr. 17, 2006:
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H. Poor Imani:
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