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Wolfgang Ernst Pauli was one of the most outstanding physicists
of the twentieth century. In his work he was a perfectionist. He
extended his rigorous criteria not only to his own work but also
to the work of his friends as well. He was a great critique. This
earned him the title of “conscience of Physics”. David
C. Cassidy wrote: “Pauli was called “the conscience
of physics” for his mastery of theoretical physics and his
critical assessment of ongoing work. His review articles and books
on relativity theory, statistical mechanics, and quantum physics
are masterpieces of physical insight.” Pauli helped to lay
the foundations of the quantum theory of fields. Pauli demonstrated
that a fourth quantum number called ‘spin’ quantum number,
taking on only half-integer values, was required to describe the
state of an atomic electron. However, Pauli’s most significant
contribution to physics was his exclusion principle, which states
that no two electrons in an atom can exist in exactly same state,
with the same quantum numbers. This enabled to give a clear quantum
description of electron distribution within different atomic energy
states. Pauli, and independently Arnold Sommerfeld, devised an atomic
model that explained the electrical and thermal properties of metals.
While explaining the process of radioactive beta-decay, Pauli was
the first to recognize the existence of neutrino, an uncharged and
almost massless particle which carries off energy in radioactive
beta decay. Pauli also contributed in completing Dirac’s quantum
electrodynamics. His other major contributions dealt with the electric
properties of metals and with the relation between spin and statistics
for elementary particles.
Pauli did not take much pain in publishing his
ideas and results. Instead he announced them in lengthy correspondences
with colleagues, with whom he had close friendships. He particularly
undertook lengthy correspondences with Bohr and Heisenberg. It was
not surprising that because of non-publishing, much Pauli’s
work went un-credited. It was also true that the correspondences
were often copied and circulated.
Wolfgang Ernst Pauli was born on April 25, 1900
to Wolfgang Joseph and Berta Camilla. In 1898, Wolfgang Joseph changed
his name to Wolfgang Joseph Pauli. Wolfgang Joseph was originally
a Jew but converted to a Roman Catholic. He was a qualified physician
and he had earned a good name within a short span of time but later
he gave up his medical practice for research in chemistry and physics
and he went on to become a university professor in chemistry. Pauli’s
father was influenced by his friend Ernst Mach, to study science.
Pauli’s middle name “Ernst” was given by his father
in honour of Ernst Mach. Pauli was also greatly influenced by Mach,
who also happened to be his godfather. Pauli thought that his acquaintance
with Mach was ‘the most important event’ that happened
in his intellectual life. Pauli later wrote: “Among my books
there is a somewhat dusty case; it contains a silver cup made in
the art nouveau style and in there is a card…written in old-fashioned,
adorned letters: ‘Dr. E. Mach, Professor at the University
of Vienna’….[He] had kindly agreed to assume the role
of my godfather …. (and) the result seems to be that I was
baptized in this way to (become more) anti-metaphysical than Catholic…[That]
cup…remained the symbol of aqua permanens (holy water), which
drives away the evil metaphysical spirits.”
Pauli completed his schooling at the Doblingen
Gymnasium. He was not an ordinary student. He read Einstein’s
paper on relativity while still he was in the Gymnasium. He graduated
from the Gymnasium in July 1918 with distinction and then joined
the Ludwig-Maximilian University at Munich. He submitted his first
paper on the theory of relativity within two months of leaving school.
While pursuing his undergraduate studies he wrote another two papers
on the theory of relativity. Among his teachers at Munich was Sommerfeld,
who had great regard for extraordinary talent of Pauli. Sommerfeld
asked Pauli to write a review article on relativity for the prestigious
Encyclpaedia der mathematischen Wissenschaften (German Encyclopadia
of Mathematics). Pauli completed his review article two months after
receiving his PhD. The article, which ran into 233 pages, was published
as a monograph. The work remains a standard reference to this day.
Einstein himself appreciated the report very much. He said: “Whoever
studies this nature, grandly conceived work would not believe that
the author is a twenty-one year old man. One wonders what to admire
most, the psychological understanding for the development of ideas,
the sureness of mathematical deduction, the profound physical insight,
the capacity for lucid, systematical presentation, the knowledge
of the literature, the complete treatment of the subject matter,
or the sureness of critical appraisal.”
Heisenberg commenting on Pauli’s way of
life in his student days at Munich wrote: “Wolfgang was a
typical night bird. He preferred the town, liked to spend evenings
in some café, and would thereafter work on his physics with
great intensity and great success. To Sommerfeld’s dismay
he would therefore rarely attend morning lectures and would not
turn up until about noon.”
At Munich, Pauli came in contact with Heisenberg
and both became friends. They developed a life-long professional
collaboration. They encouraged each other to make most significant
contributions in quantum physics. They undertook an extensive correspondence
and today this is an important source of history of twentieth century
physics. Cassidy wrote: “Like most quantum physicists of the
1920s, Heisenberg and Pauli were products of the European upper-middle-class
cultural elite. Both of their fathers were professors: Pauli’s,
a professor of colloid chemistry at the University of Vienna; Heisenberg’s,
a professor of Byzantine philology at the University of Munich.
Both sons attended outstanding humanistic gymnasia (high schools),
which emphasized classical languages and literature. Both were attracted
to physics by the excitement attending Albert Einstein’s theory
of relativity, and both earned doctorates in theoretical physics
with Arnold Sommerfeld in Munich. Pauli arrived at the University
of Munich in 1918, two years ahead of Heisenberg. Heisenberg’s
early encounter with Pauli, then in his last semester, helped to
turn Heisenberg toward atomic theory.”
Further he continues: “Heisenberg and Pauli
entered their profession at a time of great ferment. New data and
analyses indicated the inadequacy of the planetary quantum model
of the atom developed earlier by Bohr and Sommerfeld. At the same
time, turmoil surrounding the German defeat in World War I, hyperinflation,
and a boycott of German science made professional advancement difficult
for young physicists.” Commenting on his student days at Munich,
Pauli in his Nobel Lecture, said: “I was not spared the shock
which every physicist accustomed to the classical way of thinking
experienced when he came to know Bohr’s basic postulate of
quantum theory for the first time.”
Pauli was awarded PhD in 1921. In his report on
the thesis Sommerfeld wrote: “…like his many already
published smaller investigations and his larger Encyclopaedia article,
the full command of the tools of mathematical physics.”
In October 1921 Pauli was appointed as Max Born’s
assistant at the University of Gottingen. He spent about a year
at Gottingen. It was at Gottingen, Pauli first met Niels Bohr. Recalling
his first meeting with Bohr, Pauli wrote: “…a new phase
of my scientific life began when I met Niels Bohr personally for
the first time. This was in 1922, when he gave a series of guest
lectures at Gottingen when he reported on his theoretical investigations
on the periodic system of elements. During these meetings, Bohr
asked me whether I could come to Copenhagen for a year.” Pauli
accepted Bohr’s invitation and he spent one year (1922-23)
at Copenhagen. “Following Bohr’s invitation, I went
to Cpenhagen in autumn of 1922, where I made a serious effort to
explain the so-called ‘anomalous Zeeman effect’, …a
type of splitting of the spectral lines in a magnetic field which
is different from the normal triplet.”
From Copenhagen, Pauli went to the University
of Hamburg. Pauli later wrote: “Very soon after my return
to the University of Hamburgh, in 1923, I gave there my inaugural
lecture as privatdozent on the periodic system of elements. The
contents of the lecture appeared very unsatisfactory to me, since
the problem of the closing of the electronic shells had been clarified
no further.” In 1928, Pauli became Professor of Theoretical
Physics at the Federal Institute of Technology at Zurich. Under
his guidance the institute became a great centre of theoretical
physics.
In 1924, Pauli proposed that a fourth quantum
number is needed in quantum theory. Niels Bohr’s atomic model
proposed in 1913 was extended by Sommerfeld in 1915. According to
the Bohr-Sommerfeld model, each electron orbiting the nucleus of
an atom had three quantum numbers—principle quantum number
(n), azimuthal quantum number (l), magnetic quantum number (m).
Pauli introduced a fourth quantum number, which may take numerical
values +1/2 or -1/2. This was necessary to specify electron energy
states. It was later found that the two values correspond to possible
values of the ‘spin’ of the electron. The concept of
spin was experimentally verified in 1926. A set of four quantum
numbers could give a complete picture of the quantum states of atoms.
In 1925, Pauli introduced an additional principle,
called exclusion principle, for understanding the structure of all
atoms with more than one electron. According to Pauli’s principle:
“There cannot exist two or more equivalent electrons in the
atom for which…[the values of all four] quantum numbers coincide.
If the atom contains an electron for which these quantum numbers
have certain values then this state is “occupied””.
Thus according to this principle no two quantum states of an atom
can have the same fingerprint. This principle explained why not
all the electrons in an atom occupy the orbit nearest to the nucleus,
where the least amount of energy is required to complete an orbit.
Pauli discovered the exclusion principle as he was trying to understand
the anomalous Zeeman effect, named after the Dutch Physicist, Pieter
Zeeman. Pauli in his Nobel lecture, while describing how he discovered
the exclusion principle, said: “The history of the discovery
of the ‘exclusion principle’…goes back to my student
days…(It) was at the University of Munich that I was introduced
by Sommerfeld to the structure of the atom—somewhat strange
from the point of view of classical physics…A new phase of
my scientific life began when I met Niels Bohr personally for the
first time. This was in 1922, when he gave a series of guest lectures
at Gottingen, in which he reported on his theoretical investigations
on the Periodic System of the Elements … Following Bohr’s
invitation, I went to Copenhagen in the autumn of 1922, where I
made a serious effort to explain the so-called ‘anomalous
Zeeman effect’…”
In 1926, Pauli used Heisenberg’s matrix
theory of modern quantum mechanics to derive the observed spectrum
of the hydrogen atom. The result provided credence to Heisenberg’s
theory.
In 1927, he introduced Pauli matrices as a basis
of spin operators. This solved the non-relativistic theory of spin,
which in turn influenced Dirac in his discovery of the Dirac equation
for the relativistic electron.
In the late 1920s it was found that when a beta
particle is emitted from an atomic nucleus, invariably there was
some missing energy and momentum. This was viewed as grave violation
of laws of conservation. To save the situation Pauli proposed that
the missing energy and momentum is carried away from the nucleus
by some particle. In December 1930 Pauli proposed, in an “open
letter” to Meitner and Geiger, that the beta puzzle…might
be solved by introducing into the nucleus a new, neutral particle:
“[There is] the possibility that there could exist in the
nuclei electrically neutral particles that I wish to call neutrons,
which have spin ½ and obey the exclusion principle, and additionally
differ from light quanta in that they do not travel with the velocity
of light: The mass of the neutron must be of the same order of magnitude
as the electron mass and, in any case, not larger than 0.01 proton
mass. The continuous beta-spectrum would then become understandable
by the assumption that in beta-decay a neutron is emitted together
with the electron, in such a way that the sum of the energies of
neutron and electron is constant.” Pauli did not publish his
idea immediately. He first publicly defended his hypothesis at a
conference in Pasadena on June 16, 1931. His announcement was reported
by the New York Times on June 17, 1931. It wrote: “A new habitant
of the heart of the atom was introduced to the world of physics
today when Dr W Pauli of the Institute of Technology in Zurich,
Switzerland, postulated the existence of particles which he christened
“neutrons.” Pauli’s prediction was published in
print 1933. By that time “heavy neutron” had already
been discovered by Chadwick. Pauli had no clear idea about the properties
of the particle. In 1934, Enrico Fermi proposed that Pauli’s
particle be called a “neutrino”, which is Italian for
“little neutral one.” Fermi also correctly stated that
the particle was not a constituent of the nucleus as Pauli originally
believed. Neutrinos are so small that they were almost impossible
to detect with the technologies available at the time of their prediction.
And years passed but scientists failed to prove their existence.
The existence of the particle predicted by Pauli was finally experimentally
verified in 1956.
In 194, Pauli proved the spin-statistics theorem.
This theorem, an important result of quantum mechanics, states that
particles with half-integer spin are fermions, while particles with
integer spin are bosons.
In 1931, Pauli was awarded the Lorentz Medal in
Amsterdam. Pauli was awarded the Nobel Prize in 1945 for his “…decisive
contribution through his discovery in 1925 of a new law of Nature,
the exclusion principle or Pauli principle.” Pauli was first
nominated for Nobel Prize in 1933 and continued to receive nomination
for eight years but not the Prize. Finally he got the Prize in 1945
after Einstein nominated him. Einstein in a telegram sent to the
Nobel Committee wrote: “Nominate Wolfgang Pauli for physics
prize… [His] contribution to modern quantum theory consisting
in the so-called Pauli or exclusion principle became fundamental
part of modern quantum physics….”
Pauli could not be present at the Prize giving
ceremony at Stockholm. However, a special ceremony was organized
at Princeton on December 10, 1945. In this function I. Waller delivered
a presentation speech in Pauli’s absence. He said: “Pauli
based his investigation on a profound analysis of the experimental
and theoretical knowledge in atomic physics at the time. He found
that four quantum numbers are in general needed in order to define
the energy state of an electron. He then pronounced his principle,
which can be expressed by saying that there cannot be more than
one electron in each energy state when this state is completely
defined. Three quantum numbers only can be related to the revolution
of the electron round the nucleus. The necessity of a fourth quantum
number proved the existence of interesting properties of the electron.
Other physicists found that these properties may
be interpreted by stating that the electron has ‘spin’,
i.e., that it behaves to some extent as if it were rapidly rotating
round an axis through its centre of gravity.
Pauli showed himself that the electronic configuration
is made fully intelligible by the exclusion principle, which is
therefore essential for the elucidation of the characteristic physical
and chemical properties of different elements. Among those important
phenomena for the explanation of which the Pauli principle is indispensable,
we mention the electric conductivity of metals and the magnetic
properties of matter.
In 1925 and 1926 essential progress of another
kind was made in the quantum theory, which is the foundation of
atomic physics. New and revolutionary methods were developed for
the description of the motion of particles.”
At personal level Pauli suffered much. Pauli’s
mother committed suicide in 1927. He was much attached to his mother.
This made him lonely. The situation worsened when his father remarried
in the following year. He referred to his father’s new wife
as “the evil step-mother.” His first marriage with Kathe
Margarethe Deppner lasted less than year. After the divorce Pauli
had a severe breakdown and resorted to drinking. Pauli consulted
the psychiatrist and psycho therapist Carl Jung.
Pauli took keen interest in history and philosophy
of science. Laurikainen wrote: “During the last 1-15 years
of his life, Pauli spent much time studying the history and philosophy
of science. His starting point was the philosophy of quantum mechanics,
but this led him to psychology, the history of ideas and many other
fields, not least the relation of religion of natural science.”
In 1944, Pauli was appointed to the chair of theoretical
physics at the Institute for Advanced Study, Princeton, New Jersey
and then in 1946 he became a naturalized citizen of the United States.
After the Second World War was over, Pauli returned to Zurich. Pieter
Zeeman. In 1953, Pauli was elected a Fellow of the Royal Society
of London. He was elected Fellow of the Swiss Physical Society,
the American Physical Society, and the American Association for
the Advancement of Science. In 1958, Pauli was awarded the Planck
Medal.
Pauli died on December 15, 1958 in Zurich.
References
- Encyclopadeia Britannica:100 Years with Nobel Laureates. New
Delhi: Encyclopaedia Britsannica (India Pvt. Ltd., 2001.
- Heilbron, J. L.(Editor). The Oxford Companion to the History
of Modern Science. Oxford: Oxford University Press, 2003.
- Kragh, Helge. Quantum Generation: A History in Twentieth Century.
Hyderabad: Universities Press (India) Ltd., 2001.
- Chambers Biographical Dictionary (Centenary Edition). New York:
Chambers Harrap Publishers Ltd., 1997.
- The Cambridge Dictionary of Scientists (Second Edition). Cambridge:
Cambridge University Press, 2002.
- Oxford Dictionary of Scientists. Oxford: Oxford University
Press,
- Dardo, Mauro. Nobel Laureates and Twentieth Century Physics.
Cambridge: Cambridge University Press, 2004.
- Spangenburg, Ray and Diane K. Moser. The History of Science:
From 1895 to 1945. Hyderabad: Universities Press (India) Ltd.,
1999.
- James, Joan. Remarkable Physicists: From Galileo to Yukawa.
Cambridge: Cambridge University Press, 2004.
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