|
Deep Inelastic Scattering: Comparisons with the Quark
Model
Deep Inelastic Scattering:
Experiments on the Proton and the Observation of Scaling
Deep Inelastic Scattering: The Early Years
"for their pioneering
investigations concerning deep inelastic scattering of electrons on
protons and bound neutrons, which have been of essential importance for
the development of the quark model in particle physics"
 |
 |
 |
|
Jerome I. Friedman |
Henry W. Kendall |
Richard E. Taylor |
| 1/3 of
the prize |
1/3 of
the prize |
1/3 of
the prize |
| USA |
USA |
Canada |
Massachusetts Institute of Technology (MIT)
Cambridge, MA, USA |
Massachusetts Institute of Technology (MIT)
Cambridge, MA, USA |
Stanford
University
Stanford, CA, USA |
| b. 1930 |
b. 1926
d. 1999 |
b. 1929 |
Autobiography: Jerome I. Friedman
I was born in Chicago, Illinois on March
28, 1930, the second of two children of Selig and Lillian Friedman,
nee Warsaw, who were immigrants from Russia. My father came to the
United States in 1913 and later served in the U.S. Army Artillery
Corps in World War I. After the war he was employed by the Singer
Sewing Machine Co. and later established his own business, repairing
and selling used commercial and home sewing machines. My mother
arrived in the United States in 1914 on one of the last voyages of the
Lusitania. She supported herself until she was married by working in a
garment factory. My parents had little formal education, except for
courses in English after they arrived in the United States, but were
self taught and had wide ranging interests. My father was an avid
reader, having interests in science and political history, and our
home was filled with books. My mother, who had a lovely singing voice,
loved music and, in particular, opera. The education of my brother and
myself was of paramount importance to my parents, and in addition to
their strong encouragement, they were prepared to make any sacrifice
to further our intellectual development. When there were financial
difficulties they still managed to provide us with music and art
lessons. They greatly respected scholarship in itself, but they also
impressed upon us that there were great opportunities available for
those who were well educated. I received my primary and secondary
education in Chicago. As I very much liked to draw and paint as a
child, I entered a special art program in high school, which was very
much like being in an art school imbedded in a regular high school
curriculum. While I always had some interest in science, I developed a
strong interest in physics when I was in high school as a result of
reading a short book entitled Relativity, by
Einstein.
It opened a new vista for me and deepened my curiosity about the
physical world. Instead of accepting a scholarship to the Art
Institute of Chicago Museum School and against the strong advice of my
art teacher, I decided to continue my formal education and sought
admission to the University of Chicago because of its excellent
reputation and because
Enrico Fermi
taught there. I was fortunate to have been accepted with a full
scholarship. As my parents had limited means, my university training
would not have been possible without such help. After finishing my
requirements in an highly innovative and intellectually stimulating
liberal arts program (established by Robert M. Hutchins who was then
President of the University), I entered the Physics Department in
1950, receiving a Master's degree in 1953 and a Ph.D. in 1956. It is
difficult to convey the sense of excitement that pervaded the
Department at that time. Fermi's brilliance, his stimulating, crystal
clear lectures that he gave in numerous seminars and courses, the
outstanding faculty in the Department, the many notable physicists who
frequently came to visit Fermi, and the pioneering investigations of
pion proton scattering at the newly constructed cyclotron all combined
to create an especially lively atmosphere. I was indeed fortunate to
have seen the practice of physics carried out at its "very best" at
such an early stage in my development. I also had the great privilege
of being supervised by Fermi, and I can remember being overwhelmed
with a sense of my good fortune to have been given the opportunity to
work for this great man. It was a remarkably stimulating experience
that shaped the way I think about physics. My thesis project was an
investigation in nuclear emulsion of proton polarization produced in
scattering from nuclei at cyclotron energies. The objective was to
determine whether the polarization resulted from elastic or inelastic
scattering. Professor Fermi tragically died in 1954 after a short
illness. What an immense loss it was to all of us. My thesis work was
not yet completed, and John Marshall kindly took over my supervision
and signed my thesis. After I received my Ph.D., I continued working
as a post-doc at the University of Chicago nuclear emulsion
laboratory, which was then led by Valentine Telegdi. That year Val
Telegdi and I did an emulsion experiment in which we searched for
parity violation in muon decay. We were one of the first groups to
observe this surprising effect which had been suggested by
T.D. Lee and C.N. Yang.
Val was not only an excellent mentor but he was instrumental in
getting me my first real job with Robert Hofstadter.
In 1957, I joined Hofstadter's group at the High Energy Physics
Laboratory at Stanford University as a Research Associate. This was
where I learned counter physics and the techniques of electron
scattering. While there I did a number of experiments studying elastic
and inelastic electrondeuteron scattering. In an experiment to measure
a weighted sum-rule for inelastic electron deuteron scattering which
was related to the n-p interaction I had to confront the problem of
making radiative corrections to inelastic spectra, and I developed a
technique which proved to be valuable in my later work. Henry Kendall
independently developed a similar technique and later we combined
efforts to develop a radiative corrections program for our deep
inelastic scattering work at SLAC. It was in Hofstadter's group that I
began my long collaboration with Henry Kendall who was also a member
of the group. During this period I became acquainted with Richard
Taylor, who was just finishing his thesis in another group, and with
other future collaborators in the deep inelastic program at SLAC, Dave
Coward and Hobey DeStacbler. One of the highlights of this period was
attending the wonderfully informal and informative high energy physics
seminars in the home of W.K.H. Panofsky, who was Director of the
Laboratory.
In 1960, I was hired as a faculty member in the Physics Department of
the Massachusetts Institute of Technology. When I arrived I joined
David Ritson's research group. A short time later he accepted a
position at Stanford University and I inherited a small group. With
these resources I soon began working on collaborative effort to
measure muon pair production at the Cambridge Electron Accelerator (CEA)
in order to test the validity of Quantum Electro-Dynamics. Henry
Kendall joined my group in 1961 and we have been collaborators at MIT
since that time. The last measurement we did at the CEA was a
measurement of the deuteron form factor at the highest momentum
transfers that could be reached at that accelerator to get some limits
on the size of relativistic effects and meson currents.
In 1963, Henry Kendall and I started a collaboration with W.K.H.
Panofsky, Richard Taylor and other physicists from the Stanford Linear
Accelerator Center and the California Institute of Technology to
develop electron scattering facilities for a physics program at the
Stanford Linear Accelerator, a 20 GeV electron linac that was being
constructed under the leadership of Panofsky. This required that we
both travel between MIT and SLAC on a regular basis. The MIT Physics
Department gave us special support by reducing our teaching
responsibilities. We soon set up a small MIT group at SLAC and for
extended periods of time one of us was always there. We had a rare
opportunity. We were part of a group of physicists who were provided a
new accelerator, given the support to design and construct optimal
experimental facilities, and had the opportunity to participate in the
exploration of a new energy range with electrons. From 1967 to about
1975 the MIT and SLAC groups carried out a series of measurements of
inelastic electron scattering from the proton and neutron which
provided the first direct evidence of the quark sub-structure of the
nucleon. It was a very exciting time for all of us. This program is
described in detail in the adjoining Physics Nobel Lectures.
As the program at SLAC was nearing completion we joined a
collaborative effort at Fermilab involving a number of institutions to
build a beam line and a single-arm spectrometer in the Meson
Laboratory. During the latter half of the 1970's this collaboration
carried out a series of experiments to investigate elastic scattering,
Feynman
scaling and production mechanisms in inclusive hadron scattering. When
this work was completed, our group joined another collaboration to
build a large neutrino detector at Fermilab. The objective of this
program was to study the weak neutral currents in measurements of
inclusive neutrino and anti-neutrino nucleon scattering, which were
done in the first half of the 1980's. These investigations confirmed
the predictions of the Standard Model.
In 1980, I became Director of the Laboratory for Nuclear Science at
MIT and then served as Head of the Physics Department from 1983 to
1988. During the time I was in these administrative positions I
managed to maintain a foothold in research, which greatly eased my
transition back to full-time teaching and research in 1988. While it
was a very interesting period in my life, I was happy to get back to
more direct contact with students in the classroom and in my research
projects. Currently, our MIT group is participating in the
construction of a large detector to study electron-positron
annihilations at the Stanford Linear Collider and has also been
engaged in design work for a detector for the Superconducting Super
Collider, which is now under construction.
Over the years I have served on a number of program and scientific
policy advisory committees at various accelerators. I also was a
member of the Board of the University Research Association for six
years, serving as Vice President for three years. I am currently a
member of the High Energy Advisory Panel for the Department of Energy
and also Chairman of the Scientific Policy Committee of the
Superconducting Super Collider Laboratory.
Experimental high energy physics research is a group effort. I have
been very fortunate to have had outstanding students and colleagues
who have made invaluable contributions to the research with which I
have been associated. I thank them not only for their contributions,
but also for their friendship.
My life has been enhanced by my marriage to Tania Letetsky-Baranovsky
who has broadened my horizons and has been an unfaltering source of
support. She has endured with cheerful resignation my many absences
when I have had to travel to distant particle accelerators. There are
four grown children in our family, Ellena, Joel, Martin, and Sandra
who pursue their activities in various parts of the country.
With regard to my non-vocational activities, in addition to getting
much pleasure from various cultural activities, such as theater,
music, ballet, etc., I enjoy painting and study Asian ceramics.
Autobiography: Henry W. Kendall
I was born on December 9, 1926 in Boston,
Massachusetts. My parents were Henry P. Kendall, a Boston businessman,
and Evelyn Way Kendall, originally from Canada.
I lived in Boston until the early 1930s when the family - there were
five, for by then I had a younger brother and a younger sister - moved
to a small town outside Boston, where the three of us grew up and
where I still live.
I went briefly to a local grade school but was held back by a reading
disability which was cured after I was moved to a school some miles
distant. From age 14 to 18, most of the period of World War II, I
spent at Deerfield Academy, a college preparatory school. My academic
work was poor for I was more interested in non-academic matters and
was bored with school work. I had developed - or had been born with -
an active curiosity and an intense interest in things mechanical,
chemical and electrical and do not remember when I was not fascinated
with them and devoted to their exploration. Father was a great
encouragement in these projects except when they involved hazards,
such as the point, at about age 11, when I embarked on the culture of
pathogenic bacteria. He also instilled in both me and my brother a
love and respect for the outdoors, especially the mountains and the
sea.
I entered the US Merchant Marine Academy in the summer of 1945. I was
there, in basic training, when the first atom bombs were exploded over
Japan. I was unaware of the human side of these events and only recall
a feeling that some of the last secrets of nature had been penetrated
and that little would be left to explore. I spent the winter of
1945-46 on a troop transport on the North Atlantic (a most interesting
experience), returning to the Academy for advanced training in the
spring of 1946. I resigned in October, 1946, to start as a freshman at
Amherst College. Although a mathematics major at college, my interest
in physics was great and I did undergraduate research and a thesis in
that field. But history, English and biology were all most attractive
and there was a period, early on, when any one of these might have
ended up as the major subject. Non-college enterprises, in the summers
particularly, absorbed considerable time. I and a Deerfield friend
became interested in diving and two summers were spent in organizing
and running a small diving and salvage operation. We wrote our first
books after that; one on shallow water diving, another on underwater
photography, with a considerable success for both. These activities,
mostly self-taught, were a good introduction to two skills very
helpful in later experimental work: seeing projects through to
successful conclusions and doing them safely.
On the urging of Karl Compton, a family friend and then President of
MIT, I applied for, and was accepted at that institution's school of
physics in 1950. The years at graduate school were a continuing
delight - the first sustained immersion in science at a full
professional level. My thesis, carried out under the supervision of
Martin Deutsch, was an attempt to measure the Lamb shift in
positronium, a transient atom discovered by Deutsch a few years
before. The attempt was unsuccessful but it served as a very
interesting introduction to electromagnetic interactions and the power
of the underlying theory.
The two years after receiving the PhD degree were spent as a National
Science Foundation Postdoctoral Fellow at MIT and at Brookhaven
National Laboratory, followed by a trip west to join the research
group of Robert Hofstadter and the faculty of the Stanford University
physics department. Hofstadter was engaged in the study of the proton
and neutron structure that was later to bring him
the Nobel Prize,
work that even at the time was clearly of the greatest interest and
importance. The principal facility used in this research was a 300 ft.
linear electron accelerator, a precursor to the 2 mile machine at the
Stanford Linear Accelerator Center (SLAC), later built in the hills
behind the University. Here I met and worked with Jerome Friedman, got
to know Richard Taylor, then a graduate student in another group and
W.K.H. Panofsky, the driving force behind SLAC. Friedman, Taylor and I
were later to join in the long series of measurements on deep
inelastic scattering at SLAC.
As in the college years, absorbing non-physics matters claimed a
portion of my leisure time: mountaineering and mountain photography.
Stanford and the San Francisco Bay area offered a number of skilled
climbs as well as Yosemite Valley not far away. After two years of
rock and mountain climbing, I was invited on the first-of several
expeditions to the Andes. Later there have been trips to the Himalayas
and the Arctic, with cameras of increasing size to capture some of the
astonishing beauty of those remote places. Many of the friends made
during those years have remained through life.
After five years at Stanford I moved back to MIT as a member of the
faculty. Friedman had gone there a year earlier and we reestablished
our collaboration. By 1964, the joint work with Taylor, by then a
research group leader at SLAC, was initiated. This collaboration was
surely the most enjoyable of any physics I have ever done. It was a
pleasure shared by most people in the effort and well recognized at
the time. All three of us have remained, up to the present, in the
universities we were at then. I have been involved in research in
later years, after the SLAC effort wound down in the middle 1970s, at
the proton accelerator at Fermilab and since 1981, again at SLAC. The
most interesting physics for me has always been the searches for new
phenomena or new effects. With colleagues I have searched for limits
to quantum electrodynamics, heavy electrons, parity breakdown in
electron properties, and other such things. Unfortunately, the
ever-growing size, scale, and duration of particle experiments, as
well as the much larger collaborations, have made such programs less
and less congenial to me over the years, circumstances that disturb
many in the physics community.
At the start of the 1960s, troubled by the massive build-up of the
superpower's nuclear arsenals, I joined a group of academic scientists
advising the U.S. Defense Department. The opportunity to observe the
operation of the Defense establishment from the "inside," both in the
nuclear weapons area and in the counterinsurgency activities that
later expanded to be the U.S. military involvement in South East Asia
proved a valuable experience, helpful in later activities in the
public domain. It was clear that changing unwise Government policies
from inside, especially those the Government is deeply attached to,
involves severe, often insurmountable, problems.
In 1969, I was one of a group founding the Union of Concerned
Scientists (UCS), and have played a substantial role in its activities
in the years hence. UCS is a public interest group, supported by funds
raised from the general public, that presses for control of
technologies which may be harmful or dangerous. The organization has
had an important national role in the controversies over nuclear
reactor safety, the wisdom of the US Strategic Defense Initiative, the
B2 (Stealth) bomber, and the challenge posed by fossil fuel burning
and possible greenhouse warming of the atmosphere, among others. I
have been Chairman of the organization since 1974. The activities of
the organization are part of a slowly growing interest among
scientists to take more responsibility for helping society control the
exceedingly powerful technologies that scientific research has
spawned. It is hard to conclude that scientists are in the main
responsible for the damage and risks that are now so apparent in such
areas as environmental matters and nuclear armaments; these have been
largely the consequence of governmental and industrial imperatives,
both here and abroad. Yet it seems clear that without scientists'
participation in the public debates, the chances of great injury to
all humanity is much enhanced. In my view, the scientific community
has not participated in this effort at a level commensurate with the
need, nor with the special responsibilities that scientists
ineluctably have in this area.
This expenditure of effort and the sense of responsibility to help
achieve control of aberrant technologies which drives it, stems in no
small measure from the example set by my Father, who, throughout his
life, spent a great deal of time and no small amount of energy on
quiet, pro bono work. He was not alone among his own friends -
nor among his own contemporaries - in this; it has been a tradition in
New England of very long standing. In continuing to pursue such
objectives, my expectation is that the challenges facing both me and
the Union will be made substantially easier by the award of the Nobel
Prize. This is perhaps the most attractive part of having gained this
exceptional honor.
Autobiography: Richard E. Taylor
Medicine Hat is a small town in Southwestern Alberta founded
just over 100 years ago in a valley where the Canadian Pacific Railway crossed
the South Saskatchewan River. I was born there on November 2, 1929 and raised in
comfortable if somewhat Spartan circumstances. My father was the son of a
Northern Irish carpenter and his Scottish wife who homesteaded on the Canadian
prairies; my mother was an American, the daughter of Norwegian immigrants to the
northern United States who moved to a farm in Alberta shortly after the first
World War. During my early years our family of three was part of a large family
clan headed by my Scottish grandmother. I attended schools named after English
Generals and Royalty - Kitchener, Connaught, Alexandra.
Although I read quite a bit and found mathematics easy, I was not an outstanding
student. In high school I did reasonably well in mathematics and science thanks
to some talented and dedicated teachers.
I was nearly ten years old when World War II began. That conflict had a great
effect on our town, and on me. In rapid succession the town found itself host to
an R.A.F. flight training school, a prisoner of war camp and a military research
establishment. The wartime glamor of the military, the sudden infusion of groups
of sophisticated and highly-educated people, and new cultural opportunities (the
first live symphonic music I ever heard was played by German prisoners of war)
all transformed our town and widened the horizons of the young people there. I
developed an interest in explosives and blew three fingers off my left hand just
before hostilities ended in Europe. The atomic bomb that ended the war later
that summer made me intensely aware of physicists and physics.
Higher education was highly prized in the society of a small prairie town and I
was expected to continue on to university. After some difficulties over low
grades in some high school subjects, I was admitted to the University of Alberta
in Edmonton. I registered in a special program emphasizing mathematics and
physics and gradually became interested in experimental physics, continuing my
studies towards a Masters degree at the same institution. My thesis research was
a rather primitive effort to measure double
b-decay
in an aging Wilson cloud chamber. Between sessions at the University, I spent
two summers as a research assistant at the Defense Research Board installation
near Medicine Hat working with Dr. E.J. Wiggins, who encouraged me to continue
my studies either in eastern Canada or in the United States.
Those were interesting years, and during this time I met, courted and married
Rita Bonneau - a partnership which has enriched my life in every way. Together
we decided to try California, and I was accepted into the graduate program at
Stanford, while she found work teaching in a military school in order to support
us both. The first two years at Stanford were exciting beyond description - the
Physics Department at Stanford included
Felix Bloch,
Leonard Schiff,
Willis Lamb,
Robert Hofstadter,
and W.K.H. (Pief) Panofsky who had just arrived from Berkeley. I found that I
had to work hard to keep up with my fellow students, but learning physics was
great fun in those surroundings. At the end of the second year I joined the High
Energy Physics Laboratory where the new linear accelerator was just beginning to
do experiments. My thesis work was accomplished there under Prof. Robert F.
Mozley, on a rather diffcult experiment producing polarized
g-rays
from the accelerator beam and then using those
g-rays
to study
p-meson
production.
In 1958 I was invited to join a group of physicists at the École Normale
Supérieure in Paris who were planning experiments at an accelerator (similar to
the linac at Stanford) which was under construction in Orsay. I stayed in France
for about three years working on the experimental facilities for the
accelerator, and then participated in some electron scattering experiments. My
wife began a new career there as a librarian at the Orsay laboratory, a career
which was interrupted for a while when our son, Ted, was born in 1960. We
returned to the United States in 1961 but a continuing connection to French
physics and physicists has been a significant element in my life since that time
- including a Doctorate (Honoris Causa) very kindly conferred upon me in 1980 by
the Université de Paris-Sud.
Upon our return to the United States, I joined the staff of the Lawrence
Berkeley Laboratory at the University of California. After less than a year in
Berkeley, I moved back to Stanford where work on the construction of Stanford
Linear Accelerator Center (SLAC) was just beginning. At SLAC, I started working
on the design of the experimental areas for the new accelerator. By 1963 I had
joined the group considering the requirements for electron scattering apparatus
in the larger of two experimental areas. I worked closely with Pief Panofsky,
and with collaborators from the California Institute of Technology and the
Massachusetts Institute of Technology. I spent the next decade helping to build
equipment and taking part in various electron scattering experiments, a number
of which are the subject of the 1990 Nobel lectures. This was a period of
intense activity, but also one of intense enjoyment for me. I was surrounded by
people I liked and admired, and deeply involved in experiments which generated
interest in laboratories and universities all over the world. I count myself
extremely fortunate to have been at SLAC at that time.
I became a member of the SLAC faculty in 1968. In 1971, I was awarded a
Guggenheim fellowship and spent an interesting sabbatical year at CERN, where I
was impressed by the great progress that European science had made in the decade
since I had worked in France.
Well before my trip to CERN, colleagues in the group at SLAC had become
interested in testing some of the invariance properties of the electromagnetic
interaction, a field which would absorb our efforts for most of the 1970s. When
Charles Prescott joined the group in 1970, he began a serious study of ways to
test parity conservation in the interaction between an electron and a nucleon.
The electroweak theories of
Weinberg and Salam
predicted levels of nonconservation that looked extremely hard to measure. We
attempted an experiment with the existing Yale polarized source, but the
measurements did not reach the desired level of sensitivity. I was not very
encouraging to my colleagues who wished to pursue the experiment to higher
levels of accuracy. After the theoretical work of Veltman and van't Hooft and
the discovery of neutral currents at CERN (during the year I was there) and at
NAL (now Fermilab), the interest in experiments on parity conservation greatly
intensified. In 1975 a new method for producing polarized electrons was
discovered by a group in Colorado which included E.L. Garwin of SLAC. In 1978,
after building a source for the linac based on the new method, we were able to
demonstrate a violation of parity in close agreement with the electroweak
predictions.
After the parity experiments, our group presented two proposals for large
experimental facilities at PEP, the e+e-
collider then being built at SLAC. Both those proposals were rejected. The group
was finally successful in proposing a relatively small PEP detector, but I did
not take part in that experiment.
In 1981, I received an Alexander von Humboldt award which allowed me to spend
most of the 1981-82 academic year at DESY in Hamburg. In 1982 I returned to SLAC
as Associate Director for Research, a post I held until 1986 when I resigned to
return to research. Since that time I have spent quite a bit of time in Europe
and I am presently playing a very small role in the H1 detector
preparations at HERA.
Nobel Lecture: Jerome I. Friedman
Deep Inelastic
Scattering: Comparisons with the Quark Model
Nobel Lecture:
Henry W. Kendall
Deep
Inelastic Scattering: Experiments on the Proton and the Observation of
Scaling
Nobel Lecture:
Richard E. Taylor
Deep Inelastic Scattering: The Early Years
Source:
http://nobelprize.org/nobel_prizes/physics/laureates/1990/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
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DOC
HTM
Section Five;
Opinions About CPH
Theory
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DOC
HTM
Section six; Questions and answers
CPH Theory
PDF
DOC
HTM
Section Nine; Maxwell equations in
gravitational Field
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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
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H. Poor Imani: Time,
Revolution and Spin
PDF
DOC
H. Poor Imani and Salman
Hoghoghi: Time, Revolution and Biological Time
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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
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