I suppose I am not the first Nobelist who, on the occasion
of receiving this Prize, wonders how on earth, by what strange alchemy of family
background, teachers, friends, talents and especially accidents of history and
of personal life he or she arrived at this point. I have browsed in previous
volumes of "Les Prix Nobel" and I know that there are others whose eventual
destinies were foreshadowed early in their lives – mathematical precocity,
champion bird watching, insatiable reading, mechanical genius. Not in my case,
at least not before my late teens. On the contrary: An early photo of my older
sister and myself, taken at a children's costume party in Vienna – I look
about 7 years old – shows me dressed up in a dark suit and a black top
hat, toy glasses pushed down my nose, and carrying a large sign under my arm
with the inscription "Professor Know-Nothing".
Here then is my attempt to convey to the reader how, at age 75, I see my life
which brought me to the present point: a long-retired professor of theoretical
physics at the University of California, still loving and doing physics, including
chemical physics, mostly together with young people less than half my age; moderately
involved in the life of my community of Santa Barbara and in broader political
and social issues; with unremarkable hobbies such as listening to classical
music, reading (including French literature), walking with my wife Mara or alone,
a little cooking (unjustifiably proud of my ratatouille); and a weekly half
hour of relaxed roller blading along the shore, a throwback to the ice-skating
of my Viennese childhood. My three daughters and three grandchildren all live
in California and so we get to see each other reasonably often.
I was naturalized as an American citizen in 1957 and this has been my primary
self-identity ever since. But, like many other scientists, I also have a strong
sense of global citizenship, including especially Canada, Denmark, England,
France and Israel, where I have worked and lived with a family for considerable
periods, and where I have some of my closest friends.
My feelings towards Austria, my native land, are – and will remain –
very painful. They are dominated by my vivid recollections of 1 1/2 years as
a Jewish boy under the Austrian Nazi regime, and by the subsequent murder of
my parents, Salomon and Gittel Kohn, of other relatives and several teachers,
during the holocaust. At the same time I have in recent years been glad to work
with Austrians, one or two generations younger than I: Physicists, some teachers
at my former High School and young people (Gedenkdiener) who face the dark years
of Austria's past honestly and constructively.
On another level, I want to mention that I have a strong Jewish identity and
– over the years – have been involved in several Jewish projects,
such as the establishment of a strong program of Judaic Studies at the University
of California in San Diego.
My father, who had lost a brother, fighting on the Austrian side in World War
I, was a committed pacifist. However, while the Nazi barbarians and their collaborators
threatened the entire world, I could not accept his philosophy and, after several
earlier attempts, was finally accepted into the Canadian Infantry Corps during
the last year of World War II. Many decades later I became active in attempts
to bring an end to the US-Soviet nuclear arms race and became a leader of unsuccessful
faculty initiatives to terminate the role of the University of California as
manager of the nuclear weapons laboratories at Los Alamos and Livermore. I offered
early support to Jeffrey Leiffer, the founder of the student Pugwash movement
which concerns itself with global issues having a strong scientific component
and in which scientists can play a useful role. Twenty years after its founding
this organization continues strong and vibrant. My commitment to a humane and
peaceful world continues to this day. I have just joined the Board of the Population
Institute because I am convinced that early stabilization of the world's population
is important for the attainment of this objective.
After these introductory general reflections from my present vantage point I
would now like to give an idea of my childhood and adolescence. I was born in
1923 into a middle class Jewish family in Vienna, a few years after the end
of World War I, which was disastrous from the Austrian point of view. Both my
parents were born in parts of the former Austro-Hungarian Empire, my father
in Hodonin, Moravia, my mother in Brody, then in Galicia, Poland, now in the
Ukraine. Later they both moved to the capital of Vienna along with their parents.
I have no recollection of my father's parents, who died relatively young. My
maternal grandparents Rappaport were orthodox Jews who lived a simple life of
retirement and, in the case of my grandfather, of prayer and the study of religious
texts in a small nearby synagogue, a Schul as it was called. My father carried
on a business, Postkartenverlag Brueder Kohn Wien I, whose main product was
high quality art postcards, mostly based on paintings by contemporary artists
which were commissioned by his firm. The business had flourished in the first
two decades of the century but then, in part due to the death of his brother
Adolf in World War I, to the dismantlement of the Austrian monarchy and to a
worldwide economic depression, it gradually fell on hard times in the 1920s
and 1930s. My father struggled from crisis to crisis to keep the business going
and to support the family. Left over from the prosperous times was a wonderful
summer property in Heringsdorf at the Baltic Sea, not far from Berlin, where
my mother, sister and I spent our summer vacations until Hitler came to power
in Germany in 1933. My father came for occasional visits (the firm had a branch
in Berlin). My mother was a highly educated woman with a good knowledge of German,
Latin, Polish and French and some acquaintance with Greek, Hebrew and English.
I believe that she had completed an academically oriented High School in Galicia.
Through her parents we maintained contact with traditional Judaism. At the same
time my parents, especially my father, also were a part of the secular artistic
and intellectual life of Vienna.
After I had completed a public elementary school, my mother enrolled me in the
Akademische Gymnasium, a fine public high school in Vienna's inner city. There,
for almost five years, I received an excellent education, strongly oriented
toward Latin and Greek, until March 1938, when Hitler Germany annexed Austria.
(This so-called Anschluss was, after a few weeks, supported by the great majority
of the Austrian population). Until that time my favorite subject had been Latin,
whose architecture and succinctness I loved. By contrast, I had no interest
in, nor apparent talent for, mathematics which was routinely taught and gave
me the only C in high school. During this time it was my tacit understanding
that I would eventually be asked to take over the family business, a prospect
which I faced with resignation and without the least enthusiasm.
The Anschluss changed everything: The family business was confiscated but my
father was required to continue its management without any compensation; my
sister managed to emigrate rather promptly to England; and I was expelled from
my school.
In the following fall I was able to enter a Jewish school, the Chajes Gymnasium,
where I had two extraordinary teachers: In physics, Dr. Emil Nohel, and in mathematics
Dr. Victor Sabbath. While outside the school walls arbitrary acts of persecution
and brutality took place, on the inside these two inspired teachers conveyed
to us their own deep understanding and love of their subjects. I take this occasion
to record my profound gratitude for their inspiration to which I owe my initial
interest in science. (Alas, they both became victims of Nazi barbarism).
I note with deep gratitude that twice, during the Second World War, after having
been separated from my parents who were unable to leave Austria, I was taken
into the homes of two wonderful families who had never seen me before: Charles
and Eva Hauff in Sussex, England, who also welcomed my older sister, Minna.
Charles, like my father, was in art publishing and they had a business relationship.
A few years later, Dr. Bruno Mendel and his wife Hertha of Toronto, Canada,
took me and my friend Joseph Eisinger into their family. (They also supported
three other young Nazi refugees). Both of these families strongly encouraged
me in my studies, the Hauffs at the East Grinstead County School in Sussex and
the Mendels at the University of Toronto. I cannot imagine how I might have
become a scientist without their help.
My first wife, Lois Kohn, gave me invaluable support during the early phases
of my scientific career; my present wife of over 20 years, Mara, has supported
me in the latter phases of my scientific life. She also created a wonderful
home for us, and gave me an entire new family, including her father Vishniac,
a biologist as well as a noted photographer of pre-war Jewish communities in
Eastern Europe, and her mother Luta. (They both died rather recently, well into
their nineties).
After these rather personal reminiscences I now turn to a brief description
of my life as a scientist.
When I arrived in England in August 1939, three weeks before the outbreak of
World War II, I had my mind set on becoming a farmer (I had seen too many unemployed
intellectuals during the 1930s), and I started out on a training arm in Kent.
However, I became seriously ill and physically weak with meningitis, and so
in January 1940 my "acting parents", the Hauffs, arranged for me to attend the
above-mentioned county school, where – after a period of uncertainty –
I concentrated on mathematics, physics and chemistry.
However, in May 1940, shortly after I had turned 17, and while the German army
swept through Western Europe and Britain girded for a possible German air-assault,
Churchill ordered most male "enemy aliens" (i.e., holders of enemy passports,
like myself) to be interned ("Collar the lot" was his crisp order). I spent
about two months in various British camps, including the Isle of Man, where
my school sent me the books I needed to study. There I also audited, with little
comprehension, some lectures on mathematics and physics, offered by mature interned
scientists.
In July 1940, I was shipped on, as part of a British convoy moving through U-boat-infested
waters, to Quebec City in Canada; and from there, by train, to a camp in Trois
Rivieres, which housed both German civilian internees and refugees like myself.
Again various internee-taught courses were offered. The one which interested
me most was a course on set-theory given by the mathematician Dr. Fritz Rothberger
and attended by two students. Dr. Rothberger, from Vienna, a most kind and unassuming
man, had been an advanced private scholar in Cambridge, England, when the internment
order was issued. His love for the intrinsic depth and beauty of mathematics
was gradually absorbed by his students.
Later I was moved around among various other camps in Quebec and New Brunswick.
Another fellow internee, Dr. A. Heckscher, an art historian, organized a fine
camp school for young people like myself, whose education had been interrupted
and who prepared to take official Canadian High School exams. In this way I
passed the McGill University junior Matriculation exam and exams in mathematics,
physics and chemistry on the senior matriculation level. At this point, at age
18, I was pretty firmly looking forward to a career in physics, with a strong
secondary interest in mathematics.
I mention with gratitude that camp educational programs received support from
the Canadian Red Cross and Jewish Canadian philanthropic sources. I also mention
that in most camps we had the opportunity to work as lumberjacks and earn 20
cents per day. With this princely sum, carefully saved up, I was able to buy
Hardy's Pure Mathematics and Slater's Chemical Physics, books which are still
on my shelves. In January 1942, having been cleared by Scotland Yard of being
a potential spy, I was released from internment and welcomed by the family of
Professor Bruno Mendel in Toronto. At this point I planned to take up engineering
rather than physics, in order to be able to support my parents after the war.
The Mendels introduced me to Professor Leopold Infeld who had come to Toronto
after several years with Einstein. Infeld, after talking with me (in a kind
of drawing room oral exam), concluded that my real love was physics and advised
me to major in an excellent, very stiff program, then called mathematics and
physics, at the University of Toronto. He argued that this program would enable
me to earn a decent living at least as well as an engineering program.
However, because of my now German nationality, I was not allowed into the chemistry
building, where war work was in progress, and hence I could not enroll in any
chemistry courses. (In fact, the last time I attended a chemistry class was
in my English school at the age of 17.) Since chemistry was required, this seemed
to sink any hope of enrolling. Here I express my deep appreciation to Dean and
head of mathematics, Samuel Beatty, who helped me, and several others, nevertheless
to enter mathematics and physics as special students, whose status was regularized
one or two years later.
I was fortunate to find an extraordinary mathematics and applied mathematics
program in Toronto. Luminous members whom I recall with special vividness were
the algebraist Richard Brauer, the non-Euclidean geometer, H.S.M. Coxeter, the
aforementioned Leopold Infeld, and the classical applied mathematicians John
Lighton Synge and Alexander Weinstein. This group had been largely assembled
by Dean Beatty. In those years the University of Toronto team of mathematics
students, competing with teams from the leading North-American Institutions,
consistently won the annual Putman competition. (For the record I remark that
I never participated). Physics too had many distinguished faculty members, largely
recruited by John C. McLennan, one of the earliest low temperature physicists,
who had died before I arrived. They included the Raman specialist H.L. Welsh,
M.F. Crawford in optics and the low-temperature physicists H.G. Smith and A.D.
Misener. Among my fellow students was Arthur Schawlow, who later was to share
the Nobel Prize for the development of the laser.
During one or two summers, as well as part-time during the school year, I worked
for a small Canadian company which developed electrical instruments for military
planes. A little later I spent two summers, working for a geophysicist, looking
for (and finding!) gold deposits in northern Ontario and Quebec.
After my junior year I joined the Canadian Army. An excellent upper division
course in mechanics by A. Weinstein had introduced me to the dynamics of tops
and gyroscopes. While in the army I used my spare time to develop new strict
bounds on the precession of heavy, symmetrical tops. This paper, "Contour Integration
in the Theory of the Spherical Pendulum and the Heavy Symmetrical Top" was published
in the Transactions of American Mathematical Society. At the end of one year's
army service, having completed only 2 1/2 out of the 4-year undergraduate program,
I received a war-time bachelor's degree "on – active – service"
in applied mathematics.
In the year 1945-6, after my discharge from the army, I took an excellent crash
master's program, including some of the senior courses which I had missed, graduate
courses, a master's thesis consisting of my paper on tops and a paper on scaling
of atomic wave-functions.
My teachers wisely insisted that I do not stay on in Toronto for a Ph.D, but
financial support for further study was very hard to come by. Eventually I was
thrilled to receive a fine Lehman fellowship at Harvard. Leopold Infeld recommended
that I should try to be accepted by Julian Schwinger, whom he knew and who,
still in his 20s, was already one of the most exciting theoretical physicists
in the world.
Arriving from the relatively isolated University of Toronto and finding myself
at the illustrious Harvard, where many faculty and graduate students had just
come back from doing brilliant war-related work at Los Alamos, the MIT Radiation
Laboratory, etc., I felt very insecure and set as my goal survival for at least
one year. The Department Chair, J.H. Van Vleck, was very kind and referred to
me as the Toronto-Kohn to distinguish me from another person who, I gathered,
had caused some trouble. Once Van Vleck told me of an idea in the band-theory
of solids, later known as the quantum defect method, and asked me if I would
like to work on it. I asked for time to consider. When I returned a few days
later, without in the least grasping his idea, I thanked him for the opportunity
but explained that, while I did not yet know in what subfield of physics I wanted
to do my thesis, I was sure it would not be in solid state physics. This problem
then became the thesis of Thomas Kuhn, (later a renowned philosopher of science),
and was further developed by myself and others. In spite of my original disconnect
with Van Vleck, solid state physics soon became the center of my professional
life and Van Vleck and I became lifelong friends.
After my encounter with Van Vleck I presented myself to Julian Schwinger requesting
to be accepted as one of his thesis students. His evident brilliance as a researcher
and as a lecturer in advanced graduate courses (such as waveguides and nuclear
physics) attracted large numbers of students, including many who had returned
to their studies after spending "time out" on various war-related projects.
I told Schwinger briefly of my very modest efforts using variational principles.
He himself had developed brilliant new Green's function variational principles
during the war for wave-guides, optics and nuclear physics (Soon afterwards
Green's functions played an important role in his Nobel-Prize-winning work on
quantum electrodynamics). He accepted me within minutes as one of his approximately
10 thesis students. He suggested that I should try to develop a Green's function
variational method for three-body scattering problems, like low-energy
neutron-deuteron scattering, while warning me ominously, that he himself had
tried and failed. Some six months later, when I had obtained some partial, very
unsatisfactory results, I looked for alternative approaches and soon found a
rather elementary formulation, later known as Kohn's variational principle for
scattering, and useful for nuclear, atomic and molecular problems. Since I had
circumvented Schwinger's beloved Green's functions, I felt that he was very
disappointed. Nevertheless he accepted this work as my thesis in 1948. (Much
later L. Fadeev offered his celebrated solution of the three-body scattering
problem).
My Harvard friends, close and not so close, included P.W. Anderson, N. Bloembergen,
H. Broida (a little later), K. Case, F. De Hoffman, J. Eisenstein, R. Glauber,
T. Kuhn, R. Landauer, B. Mottelson, G. Pake, F. Rohrlich, and C. Slichter. Schwinger's
brilliant lectures on nuclear physics also attracted many students and Postdocs
from MIT, including J. Blatt, M. Goldberger, and J.M. Luttinger. Quite a number
of this remarkable group would become lifelong friends, and one – J.M.
"Quin" Luttinger – also my closest collaborators for 13 years, 1954-66.
Almost all went on to outstanding careers of one sort or another.
I was totally surprised and thrilled when in the spring of 1948 Schwinger offered
to keep me at Harvard for up to three years. I had the choice of being a regular
post-doctoral fellow or dividing my time equally between research and teaching.
Wisely – as it turned out – I chose the latter. For the next two
years I shared an office with Sidney Borowitz, later Chancellor of New York
University, who had a similar appointment. We were to assist Schwinger in his
work on quantum electrodynamics and the emerging field theory of strong interactions
between nucleons and mesons. In view of Schwinger's deep physical insights and
celebrated mathematical power, I soon felt almost completely useless. Borowitz
and I did make some very minor contributions, while the greats, especially Schwinger
and Feynman, seemed to be on their way to unplumbed, perhaps ultimate depths.
For the summer of 1949, I got a job in the Polaroid laboratory in Cambridge,
Mass., just before the Polaroid camera made its public appearance. My task was
to bring some understanding to the mechanism by which charged particles falling
on a photographic plate lead to a photographic image. (This technique had just
been introduced to study cosmic rays). I therefore needed to learn something
about solid state physics and occasionally, when I encountered things I didn't
understand, I consulted Van Vleck.
It seems that these meetings gave him the erroneous impression that I knew something
about the subject. For one day he explained to me that he was about to take
a leave of absence and, "since you are familiar with solid state physics", he
asked me if I could teach a course on this subject, which he had planned to
offer. This time, frustrated with my work on quantum field theory, I agreed.
I had a family, jobs were scarce, and I thought that broadening my competence
into a new, more practical, area might give me more opportunities.
So, relying largely on the excellent, relatively recent monograph by F. Seitz,
"Modern Theory Of Solids", I taught one of the first broad courses on Solid
State Physics in the United States. My "students" included several of my friends,
N. Bloembergen, C. Slichter and G. Pake who conducted experiments (later considered
as classics) in the brand-new area of nuclear magnetic resonance which had just
been opened up by E. Purcell at Harvard and F. Bloch at Stanford. Some of my
students often understood much more than I, they were charitable towards their
teacher.
At about the same time I did some calculations suggested by Bloembergen, on
the recently discovered, so-called Knight shift of nuclear magnetic resonance,
and, in this connection, returning to my old love of variational methods, developed
a new variational approach to the study of wavefunctions in periodic crystals.
Although my appointment was good for another year and a half, I began actively
looking for a more long-term position. I was a naturalized Canadian citizen,
with the warmest feelings towards Canada, and explored every Canadian university
known to me. No opportunities presented themselves. Neither did the very meager
US market for young theorists yield an academic offer. At this point a promising
possibility appeared for a position in a new Westinghouse nuclear reactor laboratory
outside of Pittsburgh. But during a visit it turned out that US citizenship
was required and so this possibility too vanished. At that moment I was unbelievably
lucky. While in Pittsburgh, I stayed with my Canadian friend Alfred Schild,
who taught in the mathematics department at the Carnegie Institute of Technology
(now Carnegie Mellon University). He remarked that F. Seitz and several of his
colleagus had just left the physics department and moved to Illinois, so that
– he thought – there might be an opening for me there. It turned
out that the Department Chair, Ed Creutz was looking rather desperately for
somebody who could teach a course in solid state physics and also keep an eye
on the graduate students who had lost their "doctor-fathers". Within 48 hours
I had a telegram offering me a job!
A few weeks later a happy complication arose. I had earlier applied for a National
Research Council fellowship for 1950-51 and now it came through. A request for
a short postponement was firmly denied. Fortunately, Ed Creutz agreed to give
me a one-year leave of absence, provided I first taught a compressed course
in solid state physics. So on December 31, 1950 (to satisfy the terms of my
fellowship) I arrived in Copenhagen.
Originally I had planned to revert to nuclear physics there, in particular the
structure of the deuteron. But in the meantime I had become a solid state physicist.
Unfortunately no one in Copenhagen, including Niels Bohr, had even heard the
expression "Solid State Physics". For a while I worked on old projects. Then,
with an Indian visitor named Vachaspati (no initial), I published a criticism
of Froehlich's pre-BCS theory of superconductivity, and also did some work on
scattering theory.
In the spring of 1951, I was told that an expected visitor for the coming year
had dropped out and that the Bohr Institute could provide me with an Oersted
fellowship to remain there until the fall of 1952. Very exciting work was going
on in Copenhagen, which eventually led to the great "Collective Model of the
Nucleus" of A. Bohr and B. Mottelson, both of whom had become close friends.
Furthermore my family and I had fallen in love with Denmark and the Danish people.
A letter from Niels Bohr to my department chair at Carnegie quickly resulted
in the extension of my leave of absence till the fall of 1952.
In the summer of 1951, I became a substitute teacher, replacing an ill lecturer
at the first summer school at Les Houches, near Chamonix in France, conceived
and organized by a dynamic young French woman, Cécile Morette De Witt.
As an "expert" in solid state physics, I offered a few lectures on that subject.
Wolfgang Pauli, who visited, when he learned of my meager knowledge of solids,
mostly metallic sodium, asked me, true to form, if I was a professor of physics
or of sodium. He was equally acerbic about himself. Some 50 years old at the
time, he described himself as "a child-wonder in menopause" ("ein Wunderkind
in den Wechseljahren"). But my most important encounter was with Res Jost, an
assistant of Pauli at the ETH in Zurich, with whom I shared an interest in the
so-called inverse scattering problem: given asymptotic information, (such as
phase-shifts as function of energy), of a particle scattered by a potential
V(r), what quantitative information can be inferred about this potential? Later
that year, we both found ourselves in Copenhagen and addressed this problem
in earnest. Jost, at the time a senior fellow at the Institute for Advanced
Study in Princeton, had to return there before we had finished our work. A few
months later, in the spring of 1952, I received an invitation from Robert Oppenheimer,
to come to Princeton for a few weeks to finish our project. In an intensive
and most enjoyable collaboration, we succeeded in obtaining a complete solution
for S-wave scattering by a spherical potential. At about the same time I.M.
Gel'fand in the Soviet Union published his celebrated work on the inverse problem.
Jost and I remained close lifelong friends until his death in 1989.
After my return to Carnegie Tech in 1952, I began a major collaboration with
N. Rostoker, then an assistant of an experimentalist, later a distinguished
plasma theorist. We developed a theory for the energy band structure of electrons
for periodic potentials, harking back to my earlier experience with scattering,
Green's functions and variational methods. We showed how to determine the bandstructure
from a knowledge of purely geometric structure constants and a small number
(~ 3) of scattering phase-shifts of the potential in a single sphericalized
cell. By a different approach this theory was also obtained by J. Korringa.
It continues to be used under the acronym KKR. Other work during my Carnegie
years, 1950-59, includes the image of the metallic Fermi Surface in the phonon
spectrum (Kohn anomaly); exponential localization of Wannier functions; and
the nature of the insulating state.
My most distinguished colleague and good friend at Carnegie was G.C. Wick, and
my first PhD's were D. Schechter and V. Ambegaokar. I also greatly benefitted
from my interaction with T. Holstein at Westinghouse.
In 1953, with support from Van Vleck, I obtained a summerjob at Bell Labs as
assistant of W. Shockley, the co-inventor of the transistor. My project was
radiation damage of Si and Ge by energetic electrons, critical for the use of
the recently developed semiconductor devices for applications in outer space.
In particular, I established a reasonably accurate energy threshold for permanent
displacement of a nucleus from its regular lattice position, substantially smaller
than had been previously presumed. Bell Labs at that time was without question
the world's outstanding center for research in solid state physics and for the
first time, gave me a perspective over this fascinating, rich field. Bardeen,
Brattain and Shockley , after their invention of the transistor, were the great
heroes. Other world class theorists were C. Herring, G. Wannier and my brilliant
friend from Harvard, P.W. Anderson. With a few interruptions I was to return
to Bell Labs every year until 1966. I owe this institution my growing up from
amateur to professional.
In the summer of 1954 both Quin Luttinger and I were at Bell Labs and began
our 13-year long collaborations, along with other work outside our professional
"marriage". (Our close friendship lasted till his death in 1997). The all-important
impurity states in the transistor materials Si and Ge, which govern their electrical
and many of their optical properties, were under intense experimental study,
which we complemented by theoretical work using so-called effective mass theory.
In 1957, I wrote a comprehensive review on this subject. We (mostly Luttinger)
also developed an effective Hamiltonian in the presence of magnetic fields,
for the complex holes in these elements. A little later we obtained the first
non-heuristic derivation of the Boltzman transport equation for quantum mechanical
particles. There followed several years of studies of many-body theories, including
Luttinger's famous one-dimensional "Luttinger liquid" and the "Luttinger's theorem"
about the conservation of the volume enclosed by a metallic Fermi surface, in
the presence of electron electron interaction. Finally, in 1966, we showed that
superconductivity occurs even with purely repulsive interactions – contrary
to conventional wisdom and possibly relevant to the much later discovery of
high-Tc superconductors.
In 1960, when I moved to the University of California San Diego, California,
my scientific interactions with Luttinger, then at Columbia University, and
with Bell Labs gradually diminished. I did some consulting at the nearby General
Atomic Laboratory, interacting primarily with J. Appel. My university colleagues
included G. Feher, B. Maple, B. Matthias, S. Schultz, H. Suhl and J. Wheatley,
– a wonderful environment. During my 19-year stay there I typically worked
with two postdocs and four graduate students. A high water mark period were
the late 1960s, early 1970s, including N. Lang, D. Mermin, M. Rice, L.J. Sham,
D. Sherrington, and J. Smith.
I now come to the development of density functional theory (DFT). In the fall
of 1963, I spent a sabbatical semester at the École Normale Supérieure
in Paris, as guest and in the spacious office of my friend Philippe Nozières.
Since my Carnegie days I had been interested in the electronic structure of
alloys, a subject of intense experimental interest in both the physics and metallurgy
departments. In Paris I read some of the metallurgical literature, in which
the concept of the effective charge e* of an atom in an alloy was prominent,
which characterized in a rough way the transfer of charge between atomic cells.
It was a local point of view in coordinate space, in contrast
to the emphasis on delocalized waves in momentum space, such as
Bloch-waves in an average periodic crystal, used for the rough description of
substitutional alloys. At this point the question occurred to me whether, in
general, an alloy is completely or only partially characterized by its
electronic density distribution n(r): In the back of my mind I knew that this
was the case in the Thomas-Fermi approximation of interacting electron systems;
also, from the "rigid band model" of substitutional alloys of neighboring elements,
I knew that there was a 1-to-1 correspondence between a weak perturbing potential
v(r) and the corresponding small change
n(r) of the density
distribution. Finally it occurred to me that for a single particle there is
an explicit elementary relation between the potential v(r) and the density,
n(r), of the groundstate. Taken together, these provided strong support for
the conjective that the density n(r) completely determines the external potential
v(r). This would imply that n(r) which integrates to N, the total number of
electrons, also determines the total Hamilton H and hence all properties
derivable from H and N, e.g. the wavefunction of the 17th excited state,
17 (r1,...,rN)!
Could this be true? And how could it be decided? Could two different potentials,
v1(r) and v2(r), with associated different groundstates
1 (r1,...,rN) and
2 (r1,...,rN) give rise to the same
density distribution? It turned out that a simple 3-line argument, using my
beloved Rayleigh Ritz variational principle, confirmed the conjecture. It seemed
such a remarkable result that I did not trust myself.
By this time I had become friends with another inhabitant of Nozière's
office, Pierre Hohenberg, a lively young American, recently arrived in Paris
after a one-year fellowship in the Soviet Union. Having completed some work
there he seemed to be "between" problems and I asked if he would be interested
in joining me. He was. The first task was a literature search to see if this
simple result was already known; apparently not. In short order we had recast
the Rayleigh-Ritz variational theorem for the groundstate energy in terms of
the density n (r) instead of the many electron wave function , leading to what is now called the Hohenberg
Kohn (HK) variational principle. We fleshed out this work with various approximations
and published it.
Shortly afterwards I returned to San Diego where my new postdoctoral fellow,
Lu J. Sham had already arrived. Together we derived from the HK variational
principle what are now known as the Kohn-Sham (KS) equations, which have found
extensive use by physicists and chemists, including members of my group.
Since the 1970s I have also been working on the theory of surfaces, mostly electronic
structure. The work with Lang in the early 1970s, using DFT, picked up and carried
forward where J. Bardeen's thesis had left off in the 1930s.
In 1979, I moved to the University of California, Santa Barbara to become the
initial director of the National Science Foundation's Institute for Theoretical
Physics (1979-84). I have continued to work with postdoctoral fellows and students
on DFT and other problems that I had put aside in previous years. Since the
middle 1980s, I have also had increasing, fruitful interactions with theoretical
chemists. I mention especially Robert Parr, the first major theoretical chemist
to believe in the potential promise of DFT for chemistry who, together with
his young co-workers, has made major contributions, both conceptual and computational.
Since beginning this autobiographical sketch I have turned 76. I enormously
enjoy the continuing progress by my younger DFT colleagues and my own collaboration
with some of them. Looking back I feel very fortunate to have had a small part
in the great drama of scientific progress, and most thankful to all those, including
family, kindly "acting parents", teachers, colleagues, students, and collaborators
of all ages, who made it possible.
From Les Prix Nobel. The Nobel Prizes 1998, Editor Tore Frängsmyr, [Nobel Foundation], Stockholm, 1999
This autobiography/biography was written at the time of the award and later published in the book series Les Prix Nobel/Nobel Lectures. The information is sometimes updated with an addendum submitted by the Laureate. To cite this document, always state the source as shown above.