Historical Faculty Information
Departmental History Awards
Physics Department History
The Early Years,
1891 through the 1930's
Stanford University opened in 1891, with
the Department of Physics among the very
first departments at the new University.
As the Register for 1891-92 indicates,
five courses in physics -- both laboratory
and classroom -- were offered to the
inaugural class of enthusiastic young men
and women. Research was not far behind,
however. By the early 1900s, research on
X-rays had begun, first under the
direction of David Webster, and later
under Paul Kirkpatrick. It was not until
the arrival of Swiss physicist Felix
Bloch, however, in 1934, that physics
research at Stanford truly caught fire. A
refugee from the Nazis, Bloch was only 28
years old when he answered David Webster's
invitation to join the Stanford faculty.
Yet he had already made extraordinary
contributions to physics, through his
theory of electron transport, the
Bethe-Bloch equation of the stopping power
of fast particles in matter, the theory of
ferromagnetism, his invention of spin
waves, and Bloch walls. Soon after he
arrived at Stanford, Bloch, together with
Berkeley physicist Robert Oppenheimer,
organized a joint seminar on theoretical
physics that met alternately at Stanford
and Berkeley. Many of the leading
physicists of Europe and the United States
traveled to the West Coast to speak at
these seminars, and many came to Stanford
as summer visitors. By the mid-1930s,
Stanford was recognized as an important
center for physics, despite the fact that
geographically it was considered far
removed from the center of "civilization!"
The Middle 1930's
through the 1960's
Encouraged initially by Enrico Fermi to
do experimental physics because, among
other things, it was "fun," in 1938 Bloch
(in collaboration with Luis Alvarez) made
the first experimental measurement of the
magnetic moment of the neutron, marking
the beginning of the work for which he is
perhaps best known. By the end of the
Second World War, Bloch, working with Bill
Hansen and Martin Packard, had succeeded
in observing nuclear magnetic resonance
(NMR) in condensed matter by the method of
nuclear induction. For these discoveries,
and the discoveries made with this
technique, Bloch shared the 1952 Nobel
Prize in Physics with Harvard's Edward
Purcell. It was Stanford's first Nobel
Prize. NMR has since become the most
important spectroscopic technique in
chemistry and biology, and magnetic
resonance imaging (MRI), an imaging
technique based upon it, is considered the
greatest advance in medical imaging since
the discovery of X-rays in 1895.
In the late 1930s, Research Associates
Russell and Sigurd Varian, working in
collaboration with their mentor, Professor
Bill Hansen, invented the klystron, a
high-power microwave source and amplifier.
The klystron was rapidly developed during
World War II for use in radar, navigation,
and blind-landing devices for aircraft.
But Hansen, whose own contribution to the
klystron was the resonant cavity called a
rhumbatron, was interested in using the
klystron for the acceleration of
particles. And by 1947 he had built the
first linear electron accelerator, the
Mark I, which accelerated electrons to 6
MeV. Then, just four years later, Edward
Ginzton and Marvin Chodorow completed the
Mark III, a 1-GeV electron accelerator. It
was the Mark III that allowed Robert
Hofstadter to study the charge and
magnetic structure of nuclei and nucleons,
work that earned him the 1961 Nobel Prize
in Physics.
Stanford Linear
Accelerator Center
Hansen's work has continued to be highly
fruitful. In 1967, the Stanford Linear
Accelerator Center (SLAC), a national
facility designed to hold a new two-mile
accelerator, was completed and running,
and nine years later, Stanford's Burton
Richter shared the Nobel Prize for the
discovery of the Psi/J-particle. In 1988,
Mel Schwartz, a long-time member of the
department, shared the Nobel Prize for his
discovery of the muon neutrino, though
this work had been done earlier at
Brookhaven. Then, in 1990, Dick Taylor
shared the Nobel Prize for his studies of
deep inelastic scattering, which showed
the existence of point-like objects in
nucleons, now recognized as quarks. In
1995, Martin Perl won the Nobel Prize in
Physics for his discovery of a new
elementary particle known as the tau
lepton.
Quantum Mechanics
and Leonard Schiff
Shifting focus to another area of
investigation, we come to Leonard Schiff,
whose book, Quantum Mechanics, published
in 1949, provided the means by which
several generations of physicists learned
this subject. Schiff had become department
chair in 1948 and, together with Bloch,
had formed an appointments committee that
gave the department clear international
stature in short order. A nuclear physics
group was built up under Walter Meyerhof
and Stanley Hanna; an Institute for
Theoretical Physics was soon established;
and, under the direction of Wolfgang
Panofsky and Robert Hofstadter, the High
Energy Physics Laboratory was organized.
In 1971, Sandy Fetter and Dirk Walecka
published Quantum Theory of Many-Particle
Systems and later Theoretical Mechanics of
Particles and Continua, sustaining the
line of superb graduate texts initiated
with Schiff's Quantum Mechanics. Both
volumes evolved from the authors' elegant
and inspiring graduate lectures on these
subjects, modeled on the Schiff dictum:
excellence in teaching goes hand-in-hand
with excellence in research -- a theme
still emphasized in the department today.
Low Temperature
Physics
Paul Kirkpatrick's pioneering research on
reflecting X-ray optics and holography
continued throughout the 1950s. In the
late '50s Bill Little and, shortly
thereafter, Bill Fairbank joined the
department to establish low-temperature
laboratories. In 1961, Fairbank and Bascom
Deaver discovered flux quantization while
Little and Ron Park discovered quantum
interference effects in superconductors,
both precursors to the SQUID. Fairbank's
earlier work on high-Q cavities led to his
proposal in 1961 for a superconducting
accelerator, eventually brought to reality
at Stanford in collaboration with Mike
McAshan, Alan Schwettman, Todd Smith, John
Turneaure and Perry Wilson. This, and the
klystrons of the earlier era, have become
the enabling technologies for many of
today's accelerators relying on
superconducting cavities like CEBAF and
LEP at CERN, as well as linear colliders
currently under discussion.
Little's controversial proposal in 1964
for a high-temperature, organic
superconductor stimulated much interest in
low-dimensional and organic conductors.
This was followed in 1969 by the discovery
of two-dimensional superconductors and, in
1975 at Stanford, polymeric
superconductors. We now know of many
organic superconductors; studies of these,
the fullerenes, and the high-transition
temperature ceramic superconductors have
become a vigorous area of condensed-matter
research.
Art Schawlow joined the Stanford faculty
shortly after he invented the laser, in
collaboration with Charles Townes, at Bell
Laboratories in 1958. An exciting time
followed, as new and powerful advances
were made in optics and laser
spectroscopy. Ted Hänsch and Schawlow
pioneered the development of Doppler-free
high-precision spectroscopy and other
powerful laser techniques that have made
possible new and fundamental studies of
atomic and molecular systems. In 1981
Schawlow shared the Nobel Prize for
physics for the discovery of these new
techniques in laser spectroscopy. Since
then, Steve Chu, who won the Nobel Prize
in physics in 1997, has taken these
optical techniques to yet another
dimension, with "optical molasses" (the
cooling of particles in a light field to
microkelvin temperatures), the laser
trapping of atoms, and the development of
optical tweezers for biological
experiments. Recently, Mark Kasevich has
returned to Stanford from several years at
Yale. His very broad interests include
both pure and applied physics; they range
from Bose-Einstein condensates in optical
lattices (which provide an important
analogy to condensed-matter systems) to
high-precision gravimeters and gyroscopes
based on atomic fountains and
interferometers.
Astrophysics
Astrophysics is on the upswing in the
department, and now includes theoretical
studies on a wide range of exotic topics
complemented by enterprising experimental
programs. These have included
participation in the Gamma-ray
astronomical observatory, EGRET (initiated
by Hofstadter in the 1970s and
subsequently under Peter Michelson's
direction), and the current development of
GLAST, a next-generation large-area
orbiting gamma-ray telescope, also led by
Michelson. Searches for dark matter in the
form of elementary particles such as WIMPs
(weakly interacting massive particles)
have been developed by Blas Cabrera. The
calculations of primordial elemental
abundances by Wagoner, the discovery of
giant luminous arcs due to gravitation
lensing by Petrosian, and the elucidation
of inflation and phase transitions in
cosmology by Linde are major cornerstones
in cosmology and astrophysics. Roger
Romani's research focuses on black holes
and neutron stars and he has been
instrumental in initiating Stanford's
membership in the Hobby-Eberly Telescope,
a 10-meter spectroscopic survey telescope
at MacDonald Observatory in Texas. Sarah
Church, an experimentalist working on
observations of the cosmic microwave
background, joined our department in 1999,
further enhancing our astrophysics
program. Phillip Scherrer leads an ongoing
major study of solar physics relying on
data from NASA satellites. In 2002,
Stanford received a major gift that led to
the formation of the Kavli Institute for
Astrophysics and Cosmology (KIPAC), based
both at SLAC and in the Physics
Department. Roger Blandford became
the Director of KIPAC, and Steven Kahn the
Deputy Director, in 2003. In 2004,
Tom Abel, a theoretical astrophysicist,
and Steven Allen, an experimental
astrophysicist, were hired with joint
faculty appointments in Physics and SLAC.
Gravity Probe B
A new experimental test of the general
theory of relativity was proposed in a
classic paper by Schiff in 1960. It
suggested the measurement of the minute
precession of a gyroscope orbiting a
rotating gravitating body. Fairbank and
Robert Cannon from the School of
Engineering then initiated a program to
develop the technology and attain the
necessary sensitivity. The Gravity Probe B
Project, as it is known, now under the
direction of Francis Everitt, has evolved
into the top-priority scientific
experiment in gravitational physics for
NASA. The first space flight is
anticipated within the next few years.
Condensed
Matter Physics
Condensed-matter physics at Stanford is
led by a group of enthusiastic faculty who
are breaking new ground. Robert Laughlin
shared the 1998 Nobel Prize for his
explanation of the quantum and fractional
quantum Hall effects. Doug Osheroff, the
1996 co-recipient of the Nobel Prize in
Physics for his discovery of superfluid
3He, is a leading experimentalist in the
area of quantum solids and fluids and
other properties of matter very near to
absolute zero. Sandy Fetter, who has made
important theoretical contributions in
vortex structures found in superfluid 4He
and 3He, is active in the theory of
Bose-Einstein condensates. Aharon
Kapitulnik is a low-temperature
experimentalist studying high-Tc
superconductors and the metal-insulator
transition (a quantum phase transition).
Sebastian Doniach is a theorist studying
superconductivity and flux pinning in
superconductors as well as various
biophysics problems. Shoucheng Zhang, who
applies quantum-field-theoretic techniques
to condensed-matter problems such as the
fractional quantum Hall effect, is
especially noted for his invention of the
“SO(5)” theory that unifies
antiferromagnetism and superconductivity,
as a possible model for high-Tc
superconducting materials. Blas Cabrera
performs experiments on superconductivity
such as measuring the Cooper pair mass and
studies of vortex pinning, and uses the
unusual quantum effects found in condensed
matter at low temperature to develop novel
detectors for particle astrophysics. David
Goldhaber-Gordon studies quantum dots,
which are artificial atoms fabricated from
mesoscopic structures on semiconducting
films. Hari Manoharan uses the scanning
tunneling microscope to create
atomic-scale structures on the surfaces of
metals and semiconductors. Steve
Kivelson, who joined the Physics faculty
in 2004, plays a leading role in the
theoretical physics of correlated electron
systems.
Other Disciplines
Finally, both theoretical and
experimental particle physics continue to
thrive at Stanford. Leonard Susskind and
Savas Dimopoulos, the main authors of
technicolor and supersymmetry as
extensions of the Standard Model, along
with Renata Kallosh, a leading expert on
supergravity and superstring theory, form
the nucleus of a dynamic and synergistic
particle-theory group that is closely
linked to our astrophysics,
condensed-matter, and SLAC theorists.
Stephen Shenker, a world leader in
theoretical particle physics and string
theory, is the Director of the Stanford
Institute for Theoretical Physics. In
addition, Shamit Kachru and Eva
Silverstein, two string theorists, have
joint appointments in the Physics
Department and SLAC, thus strengthening
the already strong ties between the two
entities.
On the experimental side, Stan Wojcicki
will study neutrino oscillations using a
neutrino beam created at Fermilab and an
underground detector in Minnesota.
Wojcicki is currently spokesperson for the
MINOS experiment, which should reveal
whether or not neutrinos actually
oscillate, and if so, will be able to
measure the oscillation mode and mixing
parameters. Patricia Burchat is one of the
leaders of the BABAR experiment at the B
factory facility at SLAC, which explores
CP violation in the decays of B mesons.
Giorgio Gratta has recently completed an
experiment searching for neutrino
oscillations with the Palo Verde reactor
and is now working on experimental studies
of neutrino properties and astrophysics
with the KamLAND detector in Japan. Gratta
is also active in developing new
techniques in particle detection.
In addition to research in the Physics
Department and at SLAC, graduate students
in Physics have access to research
projects in Applied Physics, Electrical
Engineering, Materials Science and
Engineering, and collaborative efforts
with the Medical School. A major factor in
Stanford's successful history of
innovation has been the ease of
collaborations across disciplinary and
departmental boundaries; this tradition
continues today.
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