Welcome to CPH 

E-Journal

به نشریه الکترونیکی سی. پی. اچ.

خوش آمدید

Nobel 1981

English  Farsi Home Contact us News English Articles Seminars

English Articles page has been updated



 

 

Nonlinear Optics and Spectroscopy

Spectroscopy in a New Light

lectron Spectroscopy for Atoms, Molecules and Condensed Matter

 

"for their contribution to the development of laser spectroscopy"
"for his contribution to the development of high-resolution electron spectroscopy"

 

Nicolaas Bloembergen Arthur Leonard Schawlow Kai M. Siegbahn
 1/4 of the prize  1/4 of the prize  1/2 of the prize
USA USA Sweden
Harvard University
Cambridge, MA, USA
Stanford University
Stanford, CA, USA
Uppsala University
Uppsala, Sweden
b. 1920
(in Dordrecht, the Netherlands)
b. 1921
d. 1999
b. 1918
d. 2007

 

Autobiography: Nicolaas Bloembergen

My parents, Auke Bloembergen and Sophia Maria Quint, had four sons and two daughters. I am the second child, born on March 11, 1920, in Dordrecht, the Netherlands. My father, a chemical engineer, was an executive in a chemical fertilizer company. My mother, who had an advanced degree to teach French, devoted all her energies to rearing a large family.

Before I entered grade school, the family moved to Bilthoven, a residential suburb of Utrecht. We were brought up in the protestant work ethic, characteristic of the Dutch provinces. Intellectual pursuits were definitely encouraged. The way of life, however, was much more frugal than the family income would have dictated.

At the age of twelve I entered the municipal gymnasium in Utrecht, founded as a Latin school in 1474. Nearly all teachers held Ph.D. degrees. The rigid curriculum emphasized the humanities: Latin, Greek, French, German, English, Dutch, history and mathematics. My preference for science became evident only in the last years of secondary school, where the basics of physics and chemistry were well taught. The choice of physics was probably based on the fact that I found it the most difficult and challenging subject, and I still do to this day. My maternal grandfather was a high school principal with a Ph.D. in mathematical physics. So there may be some hereditary factor as well. I am ever more intrigued by the correspondence between mathematics and physical facts. The adaptability of mathematics to the description of physical phenomena is uncanny.

My parents made a rule that my siblings should tear me away from books at certain hours. The periods of relaxation were devoted to sports: canoing, sailing, swimming, rowing and skating on the Dutch waterways, as well as the competitive team sport of field hockey. I now attempt to keep the body fit by playing tennis, by hiking and by skiing.

Professor L.S. Ornstein taught the undergraduate physics course when I entered the University of Utrecht in 1938. He permitted me and my partner in the undergraduate lab, J.C. Kluyver (now professor of physics in Amsterdam) to skip some lab routines and instead assist a graduate student, G.A. W. Rutgers, in a Ph.D. research project. We were thrilled to see our first publication, "On the straggling of Po-a-particles in solid matter", in print (Physica 7, 669, 1940).

After the German occupation of Holland in May 1940, the Hitler regime removed Ornstein from the university in 1941. I made the best possible use of the continental academic system, which relied heavily on independent studies. I took a beautiful course on statistical mechanics by L. Rosenfeld, did experimental work on noise in photoelectric detectors, and prepared the notes for a seminar on Brownian motion given by J.M.W. Milatz. Just before the Nazis closed the university completely in 1943, I managed to obtain the degree of Phil. Drs., equivalent to a M.Sc. degree. The remaining two dark years of the war I spent hiding indoors from the Nazis, eating tulip bulbs to fill the stomach and reading Kramers' book "Quantum Theorie des Elektrons und der Strahlung" by the light of a storm lamp. The lamp needed cleaning every twenty minutes, because the only fuel available was some left-over number two heating oil. My parents did an amazing job of securing the safety and survival of the family.

I had always harbored plans to do some research for a Ph.D. thesis outside the Netherlands, to broaden my perspective. After the devastation of Europe, the only suitable place in 1945 appeared to be the United States. Three applications netted an acceptance in the graduate school at Harvard University. My father financed the trip and the Dutch government obliged by issuing a valuta permit for the purchase of US$ 1,850. As my good fortune would have it, my arrival at Harvard occurred six weeks after Purcell, Torrey and Pound had detected nuclear magnetic resonance (NMR) in condensed matter. Since they were busy writing volumes for the M.I.T. Radiation Laboratory series on microwave techniques, I was accepted as a graduate assistant to develop the early NMR apparatus. My thorough Dutch educational background enabled me to quickly profit from lectures by J. Schwinger, J.H. Van Vleck, E.C. Kemble and others. The hitherto unexplored field of nuclear magnetic resonance in solids, liquids and gases yielded a rich harvest. The results are laid down in one of the most-cited physics papers, commonly referred to as BPP (N. Bloembergen, E.M. Purcell and R.V. Pound, Phys. Rev. 73, 679, 1948). Essentially the same material appears in my Ph.D. thesis, "Nuclear Magnetic Relaxation", Leiden, 1948, republished by W.A. Benjamin, Inc., New York, in 1961. My thesis was submitted in Leiden because I had passed all required examinations in the Netherlands and because C.J. Gorter, who was a visiting professor at Havard during the summer of 1947, invited me to take a postdoctoral position at the Kamerlingh Onnes Laboratorium. My work in Leiden in 1947 and 1948 resulted in establishing the nuclear spin relaxation mechanism by conduction electrons in metals and by paramagnetic impurities in ionic crystals, the phenomenon of spin diffusion, and the large shifts induced by internal magnetic fields in paramagnetic crystals.

During a vacation trip of the Physics Club "Christiaan Huyghens" I met Deli (Huberta Deliana Brink) in the summer of 1948. She had spent the war years in a Japanese concentration camp in Indonesia, where she was born. She was about to start her pre-med studies. When I returned to Harvard in 1949 to join the Society of Fellows, she managed to get on a student hospitality exchange program and traveled after me to the United States on an immigrant ship. I proposed to her the day she arrived and we got married in Amsterdam in 1950. Ever since, she has been a source of light in my life. Her enduring encouragement has contributed immensely to the successes in my further career. After the difficult years as an immigrant wife, raising three children on the modest income of a struggling, albeit tenured, young faculty member, she has found the time and energy to develop her considerable talents as a pianist and artist. We became U.S. citizens in 1958.

Our children are now independent. The older daughter, Antonia, holds M.A. degrees in political science and demography, and works in the Boston area. Our son, Brink, has an M.B.A. degree and is an industrial planner in Oregon. Our younger daughter, Juliana, envisages a career in the financial world. She has interrupted her banking job to obtain an M.B.A. in Philadelphia.

In this family setting my career in teaching and research at Harvard unfolded: Junior Fellow, Society of Fellows 1949 - 1951; Associate Professor 1951- 1957; Gordon McKay Professor of Applied Physics 1957 - 1980; Rumford Professor of Physics 1974 - 1980; Gerhard Gade University Professor 1980 present. While a Junior Fellow, I broadened my experimental background to include microwave spectroscopy and some nuclear physics at the Harvard cyclotron. I preferred the smaller scale experiments of spectroscopy, where an individual, or a few researchers at most, can master all aspects of the problem. When I returned to NMR in 1951, there were still many nuggets to be unearthed. My group studied nuclear quadrupole interactions in alloys and imperfect ionic crystals, discovered the anisotropy of the Knight shift in noncubic metals, the scalar and tensor indirect nuclear spin-spin coupling in metals and insulators, the existence of different temperatures of the Zeeman, exchange and dipolar energies in ferromagnetic relaxation, and a variety of cross relaxation phenomena. All this activity culminated in the proposal for a three-level solid state maser in 1956.

Although I was well aware of the applicability of the multilevel pumping scheme to other frequency ranges, I held the opinion - even after Schawlow and Townes published their proposal for an optical maser in 1958 - that it would be impossible for a small academic laboratory, without previous expertise in optics, to compete successfully in the realization of lasers. This may have been a self-fulfilling prophesy, but it is a matter of record that nearly all types of lasers were first reduced to practice in industrial laboratories, predominantly in the U.S.A.

I recognized in 1961 that my laboratory could exploit some of the new research opportunities made accessible by laser instrumentation. Our group started a program in a field that became known as "Nonlinear Optics". The early results are incorporated in a monograph of this title, published by W. A. Benjamin, New York, in 1965, and the program is still flourishing today. The principal support for all this work, over a period of more than thirty years, has been provided by the Joint Services Electronics Program of the U. S. Department of Defense, with a minimum amount of administrative red tape and with complete freedom to choose research topics and to publish.

My academic career at Harvard has resulted in stimulating interactions with many distinguished colleagues, and also with many talented graduate students. My coworkers have included about sixty Ph.D. candidates and a similar number of postdoctoral research fellows. The contact with the younger generations keeps the mind from aging too rapidly. The opportunities to participate in international summer schools and conferences have also enhanced my professional and social life. My contacts outside the academic towers, as a consultant to various industrial and governmental organizations, have given me an appreciation for the problems of socio-economic and political origin in the "real" world, in addition to those presented by the stubborn realities of matter and instruments in the laboratory.

Sabbatical leaves from Harvard have made it possible for us to travel farther and to live for longer periods of time in different geographical and cultural environments. Fortunately, my wife shares this taste for travel adventure. In 1957 I was a Guggenheim fellow and visiting lecturer at the École Normale Supérieure in Paris, in 1964 - 1965 visiting professor at the University of California in Berkeley, in 1973 Lorentz guest professor in Leiden and visiting scientist at the Philips Research Laboratories in the Netherlands. The fall of 1979 I spent as Raman Visiting Professor in Bangalore, India, and the first semester of 1980 as Von Humboldt Senior Scientist in the Institut für Quantum Optik, in Garching near Munich, as well as visiting professor at the College de France in Paris. I highly value my international professional and social contacts, including two exchange visits to the Soviet Union and one visit to the People's Republic of China, each of one-month duration. My wife and I look forward to continuing our diverse activities and to enjoying our home in Five Fields, Lexington, Massachusetts, where we have lived for 26 years.

Honors
Correspondent, Koninklijke Akademie van Wetenschappen, Amsterdam, 1956
Fellow, American Academy of Arts and Sciences, 1956
Member, National Academy of Sciences, Washington, D. C., 1959
Foreign Honorary Member, Indian Academy of Sciences, Bangalore, 1978
Associé Étranger, Académie des Sciences, Paris, 1980
Guggenheim Fellow, 1957
Oliver Buckley Prize, American Physical Society, 1958
Morris E. Liebman Award, Institute of Radio Engineers, 1959
Stuart Ballantine Medal, Franklin Institute, Philadelphia, 1961
National Medal of Science, President of the United States of America, 1974
Lorentz Medal, Koninklijke Akademie van Wetenschappen, Amsterdam, 1979
Frederic Ives Medal, Optical Society of America, 1979
Von Humboldt Senior Scientist, 1980

From Nobel Lectures, Physics 1981-1990, Editor-in-Charge Tore Frängsmyr, Editor Gösta Ekspång, World Scientific Publishing Co., Singapore, 1993

This autobiography/biography was first published in the book series Les Prix Nobel. It was later edited and republished in Nobel Lectures. To cite this document, always state the source as shown above.

Copyright © The Nobel Foundation 1981

 

Addendum, 1991

In June 1990 I retired from the faculty of Harvard University and became Gerhard Gade University Professor Emeritus. During the past decade I was also a visiting professor or lecturer for extended periods at the California Institute of Technology, at Fermi Scuola Nationale Superiore in Pisa, Italy, and at the University of Munich, Germany.

In 1991 I serve as President of the American Physical Society. I became an honorary professor of Fudan University, Shanghai, People's Republic of China, and received honorary doctorates from Laval University, Quebec, the University of Connecticut and the University of Hartford. In 1983 I received the Medal of Honor from the Institute of Electrical and Electronic Engineers.

My research in nonlinear optics continued with special emphasis on interactions of picosecond and femtosecond laser pulses with condensed matter and of collision-induced optical coherences. My personal life and professional activities during the past decade have been a natural continuation of what I described in my autobiographical notes in 1981.

 

Autobiography: Arthur Leonard Schawlow

I was born in Mount Vernon, New York, U.S.A. on May 5, 1921. My father had come from Europe a decade earlier. He left his home in Riga to study electrical engineering at Darmstadt, but arrived too late for the beginning of the term. Therefore, he went on to visit his brother in New York, and never returned either to Europe or to electrical engineering. My mother was a Canadian and, at her urging, the family moved to Toronto in 1924. I attended public schools there, Winchester elementary school, the Normal Model School attached to the teacher's college, and Vaughan Road Collegiate Institute (high school).

As a boy, I was always interested in scientific things, electrical, mechanical or astronomical, and read nearly everything that the library could provide on these subjects. I intended to try to go to the University of Toronto to study radio engineering, and my parents encouraged me. Unfortunately my high school years, 1932 to 1937, were in the deepest part of the great economic depression. My father's salary as one of the many agents for a large insurance company could not cover the cost of a college education for my sister, Rosemary, and me. Indeed, at that time few high school graduates continued their education. Only three or four out of our high school class of sixty or so students were able to go to a unversity.

There were, at that time, no scholarships in engineering, but we were both fortunate enough to win scholarships in the faculty of Arts of the University of Toronto. My sister's was for English literature, and mine was for mathematics and physics. Physics seemed pretty close to radio engineering, and so that was what I pursued. It now seems to me to have been a most fortunate chance, for I do not have the patience with design details that an engineer must have. Physics has given me a chance to concentrate on concepts and methods, and I have enjoyed it greatly.

With jobs as scarce as they were in those years, we had to have some occupation in mind to justify college studies. A scientific career was something that few of us even dreamed possible, and nearly all of the entering class expected to teach high school mathematics or physics. However, before we graduated in 1941 Canada was at war, and all of us were involved in some way. I taught classes to armed service personnel at the University of Toronto until 1944, and then worked on microwave antenna development at a radar factory.

In 1945, graduate studies could resume, and I returned to the University. It was by then badly depleted in staff and equipment by the effects of the depression and the war, but it did have a long tradition in optical spectroscopy. There were two highly creative physics professors working on spectroscopy, Malcolm F. Crawford and Harry L. Welsh. I took courses from both of them, and did my thesis research with Crawford. It was a very rewarding experience, for he gave the students good problems and the freedom to learn by making our own mistakes. Moreover, he was always willing to discuss physics, and even to speculate about where future advances might be found.

A Carbide and Carbon Chemicals postdoctoral fellowship took me to Columbia University to work with Charles H. Townes. What a marvelous place Columbia was then, under I.I. Rabi's leadership! There were no less than eight future Nobel laureates in the physics department during my two years there. Working with Charles Townes was particularly stimulating. Not only was he the leader in research on microwave spectroscopy, but he was extraordinarily effective in getting the best from his students and colleagues. He would listen carefully to the confused beginnings of an idea, and join in developing whatever was worthwhile in it, without ever dominating the discussions. Best of all, he introduced me to his youngest sister, Aurelia, who became my wife in 1951.

From 1951 to 1961, I was a physicist at Bell Telephone Laboratories. There my research was mostly on superconductivity, with some studies of nuclear quadrupole resonance. On weekends I worked with Charles Townes on our book Microwave Spectroscopy, which had been started while I was at Columbia and was published in 1955. In 1957 and 1958, while mainly still continuing experiments on superconductivity, I worked with Charles Townes to see what would be needed to extend the principles of the maser to much shorter wavelengths, to make an optical maser or, as it is now known, a laser. Thereupon, I began work on optical properties and spectra of solids which might be relevant to laser materials, and then on lasers.

Since 1961, I have been a professor of physics at Stanford University and was chairman of the department of physics from 1966 to 1970. In 1978 I was appointed J.G. Jackson and C.J. Wood Professor of Physics. At Stanford, it has been a pleasure to do physics with an outstanding group of graduate students, occasional postdoctoral research associates and visitors. Most especially the interaction with Professor Theodor W. Hansch has been continually delightful and stimulating. Our technicians, Frans Alkemade and Kenneth Sherwin have been invaluable in constructing apparatus and keeping it in operation. My secretary for the past nineteen years, Mrs. Fred - a Jurian, provides whatever order that can be found amidst the chaos of my office. Much of the time, my thoughts are stimulated there by the sounds of traditional jazz from my large record collection.

My wife is a musician, a mezzo soprano and choral conductor. We have a son, Arthur Keith, and two daughters, Helen Aurelia and Edith Ellen. Helen has studied French literature at Stanford, the Sorbonne, and at the University of California in Berkeley, and is now on the staffof Stanford University. Edith graduated from Stanford this year with a major in psychology.

Awards
Stuart Ballantine Medal (1962)
Thomas Young Medal and Prize (1963)
Morris N. Liebmann Memorial Prize (1964)
California Scientist of the Year (1973)
Frederick Ives Medal (1976)
Marconi International Fellowship (1977)
Honorary doctorates from University of Ghent, Belgium (1968), University of Toronto, Canada (1970), University of Bradford, England (1970). Honorary professor, East China Normal University, Shanghai (1979).
Member, U.S. National Academy of Sciences
Fellow, American Academy of Arts and Sciences
President, Optical Society of America (1975)
President, American Physical Society (1981)

 

Curriculum Vitae: Kai M. Siegbahn

Born April 20, 1918, in Lund, Sweden. Parents: Manne Siegbahn and Karin Högbom. Married May 23, 1944, to Anna Brita Rhedin. Three children: Per (1945), Hans (1947) and Nils (1953). Attended the Uppsala Gymnasium; Studied physics, mathematics and chemistry at the University of Uppsala from 1936 until 1942. Graduated in Stockholm 1944. Docent in physics that year. Research associate at the Nobel Institute for Physics 1942 - 1951. Professor of physics at the Royal Institute of Technology in Stockholm from 1951 to 1954. Professor and head of the Physics Department at the University of Uppsala since 1954. Member of the Royal Swedish Academy of Sciences, Royal Swedish Academy of Engineering Sciences, Royal Society of Science, Royal Academy of Arts and Science of Uppsala, Royal Physiographical Society of Lund, Societas Scienti arum Fennica, Norwegian Academy of Science, Royal Norwegian Society of Sciences and Letters, Honorary Member of the American Academy of Arts and Sciences, Membre du Comite International des Poids et Mesures, Paris, President of the International Union of Pure and Applied Physics (IUPAP).

Awards
The Lindblom Prize 1945
Björkén Prize 1955
Celsius Medal 1962
Sixten Heyman Award, University of Gothenburg 1971
Harrison Howe Award, Rochester 1973
Maurice F. Hasler Award, Cleveland 1975
Charles Frederick Chandler Medal, Columbia University, New York 1976
Björkén Prize 1977
Torbern Bergman Medal 1979
Pittsburgh Award of Spectroscopy 1982
 
Doctor of Science, honoris cause
University of Durham 1972
University of Basel 1980
University of Liège 1981
Upsala College, New Jersey, 1982
Research in physics covering atomic and molecular physics, nuclear physics, plasma physics and electron optics. Main research activity in the field of electron spectroscopy, ESCA. Books: Beta- and Gamma-Ray Spectroscopy, 1955; Alpha-, Beta- and Gamma-Ray Spectroscopy, 1965; ESCA-Atomic, Molecular and Solid State Structure Studied by Means of Electron Spectroscopy, 1967; ESCA Applied to Free Molecules, 1969.
Surveys on ESCA
Electron Spectroscopy for Chemical Analysis, Phil. Trans. Roy. Soc. London A, 33 - 57, 1970
Electron Spectroscopy, Encyclopedia of Science and Technology, McGrawHill, 1971
Perspectives and Problems in Electron Spectroscopy, Proc. Asilomar Conference 1971, Ed. D. A. Shirley, North Holland, 1972
Electron Spectroscopy-A New Way of Looking into Matter, Endeavor 32, 1973
Electron Spectroscopy for Chemical Analysis, Proc. of Conf. on Atomic Physics 3, Boulder, 1972, Ed. S.J. Smith and G. K. Walters, Plenum, 1973
Electron Spectroscopy for Chemical Analysis (together with C.J. Allan), MTP Int. Rev. of Science, Vol. 12, Analytical Chemistry, Part 1, Butterworths, 1973
Electron Spectroscopy-An Outlook, Proc. Namur Conference 1974, Elsevier 1974
Electron Spectroscopy and Molecular Structure, Pure and Appl. Chem. 48, Pergamon, 1976
Electron Spectroscopy for Solids, Surfaces, Liquids and Free Molecules, in Molecular Spectroscopy, Ch. 15, Heyden 1977

 

Nobel Lecture: Nicolaas Bloembergen

Nonlinear Optics and Spectroscopy

Download 180 kb

Nobel Lecture: Arthur Leonard Schawlow

Spectroscopy in a New Light

Download 290 kb

Nobel Lecture: Kai M. Siegbahn

Electron Spectroscopy for Atoms, Molecules and Condensed Matter

Download 480 kb

 

Source: http://nobelprize.org/nobel_prizes/physics/laureates/1981/index.html

 

CPH  Stands of: Creative Particle of Higgs that

 propounded by Hossein Javadi in 1987 Biography

Download of GSJ; 

Hossein Javadi, F. Forouzbakhsh
Oct. 28, 2008:
A New Definition for the Graviton

Mar. 21, 2006:  Logical Foundation of CPH Theory [PDF]   Persian Translation
Mar. 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 Translation

May. 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:
Apr. 17, 2006:
Rotation, Time Revolution and its Biological Effect

H. Poor Imani:
Mar. 20, 2006:
Time, Revolution and Spin

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  HTM

 Time 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 Physics

Contains: names, biographies and lectutures

 

Faster Than Light 

Light that travels… faster than light!

Before the Big Bang

Structure of Charge Particles

Move Structure of Photon

Structure of Charge Particles

Faster Than Light 

Light that travels… faster than light!

Before the Big Bang

Structure of Charge Particles

Move Structure of Photon

Structure of Charge Particles

Zero Point Energy and the Dirac Equation [PDF] Persian Text


 
Unification and CPH Theory [PDF] 


Strong Interaction and CPH Theory [PDF]


Summary of Physics Concepts [PDF]


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] 


CPH and Time [PDF]Persian Text Only


Time Function and Work Energy Theorem [PDF] Persian Text Only 


Properties of CPH [PDF]Persian Text Only 


CPH Theory and Special Relativity [PDF] Persian Text Only


CPH Theory and Newton's Second Law [PDF] Persian Text Only 

 

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

 

free hit counters