Los Alamos National Laboratory
 
 

Materials Physics and Applications Division Condensed Matter and Magnet Science, MPA-CMMS

DIVISION

GROUPS

CONTACTS

Group History

A brief history of the Condensed Matter and Thermal Physics Group at Los Alamos

unclassified, LA-UR-07-0454

The group known today as Condensed Matter and Thermal Physics at Los Alamos National Laboratory has a history almost as long as that of Los Alamos itself.  As our group arose out of the original Chemistry, Metallurgy Research (CMR) Division, and moved through Chemistry- Metallurgy Fowler (CMF), Physics (P), Energy (Q), back to Physics (P), then to Materials Science and Technology (MST), and most recently to Materials Physics and Applications (MPA), experimental condensed-matter science at cryogenic temperatures has remained its central technical focus, with thermodynamics a primary theme, and with additional themes of low-temperature physics and cryogenic engineering. 

Milligram quantities of plutonium first arrived at Los Alamos in late 1943, and gram amounts in early 1944, so one can imagine the thrilling pace of physical-chemistry and metallurgical investigations of plutonium and some of its alloys in 1944 and early 1945, driven simultaneously by the unbelievable excitement of learning about a completely new element and by the urgent need to deliver the “pit” for Trinity, the first nuclear explosion. 

After the end of World War II, many opportunities for fundamental science arose hand in hand with the ongoing development of nuclear weapons.  The earliest members of our group initially teamed up to determine the properties of plutonium with high precision, recognizing that measurements of some of its properties at cryogenic temperatures were essential for developing an understanding of this very unusual metal as well as for accessing the practical issue of the thermal stability of properties below room temperature.  These very early studies included isothermal compressibility, sound velocity, and thermal conductivity measurements that later were extended to electrical resistivity and specific heat.  Thus the Metals Physics group was born at Los Alamos in 1945. 

MPA-CMMS sign

Figure 1.  This sign has been hanging above the front door of our building for as long as we can remember.  (Note: da Vinci was not a member of our group.)

Our group’s cutting-edge fundamental science and practical support for the mission of Los Alamos Scientific Laboratory expanded in the late 1940s with a new applied focus:  the so-called “Super,” using a fission trigger to unleash the energy of fusion of light nuclei.  It was known that deuterons fuse much more easily than protons and that a high initial density of deuterons was advantageous, so it was obvious that research on the fundamental properties of cryogenic liquid deuterium would be needed, as well as engineering research into the separation and purification of the hydrogen isotopes and the liquefaction, storage, and transport of deuterium.  Tritium—the radioactive isotope of hydrogen—was also of interest.  In 1948, our group was renamed Low Temperature Physics and Cryoengineering, and undertook a systematic scientific and engineering study of the low-temperature thermodynamic and transport properties of all the helium and hydrogen isotopes.  This fundamental work was punctuated by the “Mike” shot at Eniwetok atoll, using liquid deuterium fuel and producing a thermonuclear yield of roughly 10 megatons of TNT.  (See Figure 2.)  

thermonuclear fusion

Figure 2. Mike, the first large-scale experiment with thermonuclear fusion. 1952. Photo courtesy of National Nuclear Security Administration / Nevada Site Office.

The record shows that many group members of that era somehow accomplished both fundamental research and meaningful participation in Mike and other south-Pacific weapons tests.  When our group’s new building, shown in Figure 3, was opened in the mid 1950s, the street in front was named Eniwetok in memory of those intense years of work.  Although cryogenic liquid deuterium was soon replaced by room-temperature solid lithium deuteride as the fuel for thermonuclear weapons, the extensive low-temperature science and engineering associated with Mike underpinned other important future developments ranging from the use of liquid hydrogen as space-shuttle fuel through the development of standards for safe handling of large quantities of cryogenic liquids to the physics of superfluid helium. 

To appreciate the scientific excitement of low-temperature physics in this era, one should remember that helium superfluidity was not discovered until 1937-38 and the two-fluid model of superfluidity was not established until the late 1940s.  As had been the case with plutonium a few years earlier, with 3He our group took advantage of the unique opportunity to explore the properties of an entirely new material, motivated by and enabled by applied work.  The natural abundance of 3He is tiny, but thermonuclear weapons production established a new, industrial-scale production of tritium, which decays with a 12-year half-life into 3He, giving our group the first access to this fascinating and complex solid and liquid.  Our group accomplished the historic initial liquefaction of 3He in 1948 and performed measurements of its thermodynamic and transport properties throughout the 1950s. Remember, too, that this was an era when most research equipment was still built by technicians — not bought from companies — and experiments were still done by people — not by computers.  Each cryostat and its associated plumbing were individually designed and carefully built.  Data acquisition rates and accuracy were usually limited by how well group members could read mercury manometers, analog galvanometers, and optical levers with linear scales, and how quickly and accurately they could write the numbers in their lab books.  Temperatures were held constant by homemade rubber-membrane manostats regulating the pressure in pumped helium baths, or in rare, sophisticated circumstances by homemade electronic feedback circuits using vacuum tubes.  Data analysis relied mostly on pencils, paper, and slide rules.  (Later, a lab book might occasionally be taken to the ladies whose job it was to transcribe data onto IBM punch cards for processing at the central computing facility.)  Secretarial skill was measured by the number of typing errors per page of technical manuscript, a number that was often far smaller than one, despite staff member handwriting that made the distinctions between words like “monatomic” and “monotonic” a matter of judgment for the typist.

MPA-CMMS buildings

Figure 3. The buildings that still hold most of our group, as they appeared in 1957 when the only other nearby buildings were the CMR building (left), the administration building (background), and the steam plant (right background). SM32 (known then as the Cryogenic Engineering Laboratory) and SM34 (known then as the Low Temperature Physics Laboratory) had a much higher ratio of lab space to office space than is typical in today’s new construction. Parts of the sawtooth roof on the east end of SM32 were deliberately weak — potential sacrifices, to save the rest of the building in case of explosion during the years that they housed hydrogen liquefaction equipment.

By the mid 1960s, the “Low Temperature Group” included 10 physicists, 9 physical chemists, 7 technicians, 5 chemical engineers, 4 machinists, 2 mechanical engineers, 2 secretaries, 2 postdocs, and 1 electrical engineer.  Already, a tremendous breadth of interests in low-temperature physics was evident:  Scientific studies underway included equation of state and thermal properties of the helium isotopes, neutron diffraction studies of solidified gases, superfluid hydrodynamics, superconductivity, Mossbauer studies of lattice dynamics and magnetism, the Kondo effect, and nuclear physics with cryogenic polarized targets.  Cryogenic engineering research and development in that era included measurement of transport properties of helium and hydrogen liquids, the design and construction of several superconducting magnets and radio-frequency cavities for use elsewhere at Los Alamos, and solid hydrogen and deuterium target development for the Los Alamos Meson Physics Facility.  At the interface between low-temperature physics and cryogenic engineering, our group had the first working 3He-4He dilution refrigerator in the US, thanks to the technician who assembled it perfectly leak-free on his first attempt;  and one of our early dilution refrigerators stayed cold for three months, which was a remarkable accomplishment at that time.

In the 1970s, a new national need gained attention, and our group responded again with a combination of fundamental research and technology development.  The 1973 OPEC oil embargo triggered the widespread realization that US energy sources were being depleted and imported energy was undependable;  furthermore, acid rain and other pollution were problematic.  Many group members naturally carried their low-temperature-physics and cryogenic-engineering talents into energy R&D.  Fundamental work included research on flux motion, losses, and pinning in Type II superconductors, dielectric breakdown at cryogenic temperatures, properties of A15 superconductors (e.g., Nb3Ge), and the stability of superconductor/normal-metal composites, while applied efforts included the development of dc and ac superconducting power transmission lines, superconducting magnetic energy storage for electric utilities, a car fueled by cryogenic hydrogen, and cryogenic distillation purification of hydrogen isotopes for fusion-energy fuel.  Federal support for such energy R&D dropped abruptly in the early 1980s, but many of these developments are receiving renewed attention today, and significant spin-offs from that era of our group, such as the Los Alamos Tritium Systems Test Assembly, now have significant histories of their own.

machine shop

Figure 4. Our group’s machine shop has changed little through many decades, until the present era of numerically controlled machines. Under microscopic examination, the calendar on the left in this photo displays January 1964, and the floor in the foreground is littered with doughnut crumbs — evidence that our traditional celebration of the exceptional work our group’s technicians goes back at least 43 years.

In the late 1970s and early 1980s, the study of thermodynamic cycles and processes, and the relevant properties of materials used in them, began with an effort in magnetic refrigeration and later included engines and refrigerators using liquids near their critical points.  Advances in magnetic refrigeration quickly took that team out of our group and into industry.  3He–4He mixtures below 1 Kelvin proved to be ideal for studying the fundamentals of yet another type of thermodynamic process:  spinodal decomposition of supersaturated phase transitions.  Another aspect of our group’s focus on cycles and processes, the development of the fundamentals and applications of thermoacoustic engines, refrigerators, and (later) mixture separators, began in 1981 with the invention of the thermoacoustic refrigerator in our group.  In the 1990s, the thermodynamic-cycles and -processes focus grew further to include the invention and development of tiny hollow, spherical, cryogenic deuterium­–tritium shells for inertial-confinement fusion targets, an effort which soon matured and moved out of our group.

The early to middle 1980s was a transitional period for fundamental research in our group, refocusing on more-fundamental problems in fluid dynamics and on strongly correlated f-electron phenomena.  Appropriate to this change in fundamental focus and to the continuation of thermodynamic-cycle and -process research, our group’s name was changed to Condensed Matter and Thermal Physics.  Correlated-electron phenomena, fundamentals of fluid dynamics, and thermoacoustics remain central research themes of our group today. 
The fluid-dynamics focus of the 1980s included an experimental program in chaos, pattern formation, and turbulence, which continues today.  Still based in part on low-temperature techniques, the fluids focus also served as an incubator for a cryogenic neutrino-mass experiment based on spin-polarized hydrogen in the 1980s.  In the 1990s, the fluids focus expanded to include the study of lead-bismuth mixtures and other liquids, and their interactions with steels, of interest in advanced nuclear reactors and the accelerator transmutation of nuclear waste;  and the thermoacoustics team began the development of thermoacoustics for industrial-scale liquefaction of natural gas.

The research focus on correlated-electron materials, their growth as single crystals, and earlier experience with applications of superconductors positioned our group to respond immediately to the 1986 discovery of high-temperature superconductivity.  As in many other laboratories around the world, this discovery marked a sea change in our group and triggered the expansion of experimental capabilities necessary to explore and understand this surprising phenomenon.  By the end of the 1980s, these capabilities included electronic transport, thermodynamics, heat transport, and nuclear-magnetic and muon-spin resonance.  Los Alamos, like the rest of the nation, saw high-temperature superconductivity as an opportunity to reinvigorate energy-related research, and formed the Superconducting Technology Center from a nucleus of group members to develop applications of this discovery.  Fundamental research on strongly correlated electron physics, including f-electron and cuprate materials, remained in our group and provided a basis for Los Alamos to collaborate with the state of Florida in establishing the new National High Magnetic Field Laboratory.  With our group’s interests in the physics of correlated materials at extremes of low temperatures and high pressures, it was natural for the newly created Los Alamos Pulsed Field Facility to find its home in our group until 1998, when the Magnet Lab was spun off as a separate Laboratory Center. 

During the 1990s, our group also diversified into ultra-fast optics (which opened new windows for investigating correlated-electron materials but also impacted weapons diagnostics), started an effort in magnetic resonance force microscopy, and added neutron scattering and photoemission to its growing repertoire of materials-characterization techniques.  These years laid the foundation for the 2002 discovery in our group of the first plutonium-based superconductor, a direct result of our earlier work on related heavy-fermion superconductors and magnets.  With this discovery and with photoemission research, part of our group returned to its roots in the study of plutonium.  Despite its continuing relevance to the Los Alamos’s mission, relatively little progress had been made on fundamental understanding of the “plutonium problem” during the previous six decades, but superconductivity in the new plutonium compound opened entirely new avenues for investigation and engaged the international condensed-matter community in plutonium for the first time.

click here for June 1999 Group Reunion photo

Summarizing the activities of hundreds of people over the course of 60 years in such a short note is a matter of brutal down-selection.  Many precious memories are unrecorded here;  entire lines of research whose stories could each occupy many pages have been completely omitted.  Nevertheless, we hope this short note communicates the pride that we feel for the history of our group, for its responsiveness to the applied needs and the scientific frontiers in each decade of its existence, and for its enduring commitment to technical excellence.

Greg Swift and Joe Thompson, 2006

(We gratefully acknowledge documents and stories from Ed Hammel, Dean Taylor, Jim Hoffer, and Marty Maley.)

Top of page

Group History

MPA-10 FACTS

Group Leaders

  • 1945-1970 Ed Hammel (Ph.D. physical chemistry, Princeton, 1944)
  • 1970-1985 Bill Keller (Ph.D. physical chemistry, Harvard, 1948)
  • 1985-1992 Bob Heffner (Ph.D. physics, Washington, 1973)
  • 1992-2001 Joe Thompson (Ph.D. physics, Cincinnati, 1975)
  • 2001-2002 Art Ramirez (Ph.D. physics, Yale, 1984)
  • 2002-2006 John Sarrao (Ph.D. physics, UCLA, 1993)
  • 2006- Mike Hundley (Ph.D. physics, Berkeley, 1988)

APS Fellows

  • Al Arko
  • Larry Campbell
  • Greg Dash
  • Bob Ecke
  • Zach Fisk
  • Chris Hammel
  • Ed Hammel
  • Bob Heffner
  • Bill Keller
  • Marty Maley
  • Al Migliori
  • Roman Movshovich
  • Bill Overton
  • Art Ramirez
  • John Sarrao
  • Adam Schuch
  • Bill Steyert
  • Greg Swift
  • Toni Taylor
  • Joe Thompson
  • John Wheatley

Laboratory Fellows*

  • Al Arko
  • Bob Ecke
  • Zach Fisk
  • Chris Hammel
  • Al Migliori
  • Bob Mills
  • Roman Movshovich
  • Greg Swift
  • Joe Thompson
  • *Los Alamos Fellows established in 1981

Present staff members

  • Scott Backhaus (p)
  • Wei Bao
  • Eric Bauer (p)
  • Nick Curro (p)
  • Tomasz Durakiewicz (p)
  • David Gardner
  • Mike Hundley (p)
  • John Joyce (p)
  • Jackie Kiplinger (p)
  • Ning Li (p)
  • Roman Movshovich (p)
  • Mike Rivera (p)
  • Filip Ronning (p)
  • Greg Swift (p)
  • Joe Thompson (p)
  • (p) indicates former postdoc

Former staff members

  • (Date ranges are years in our group; Los Alamos presence may be longer.)
  • Al Arko
  • Rick Averitt
  • Bill Ball
  • John Barclay
  • Roger Bartlett
  • John Bartlit '62-'80
  • Phil Bendt '56-'72
  • Hans Bevens '45-'48
  • Heinrich Boenig
  • John Bronson
  • Larry Campbell (p)
  • '67-'80 & '95-'98
  • Dick Carlson (p)
  • Prit Choudhuri
  • Jack Conant
  • Paul Craig
  • Tim Darling (p)
  • Greg Dash '51-'60
  • John Dean '74-'79
  • Bob Ecke (p)
  • Fred Edeskuty '50-??
  • Anatoly Efimov (p)
  • ?? Faveuff
  • Zach Fisk (s)
  • Tim Gosnell
  • Ed Grilly '47-'80
  • Chris Hammel (p)
  • Ed Hammel '45-'70
  • Bill Hassenzahl
  • Bob Heffner (p)
  • Mike Henke
  • Jim Hoffer '70-'01(p)
  • Charlie Hoffman
  • Chester Hwang
  • Chou Yen Huang
  • Il-Kyoung Jeong (p)
  • Kamal Khallafala
  • Bill Keller, '50-'85
  • Gene Kerr
  • Tsuyoshi Kimura (p)
  • Tom Kitchens (p)
  • George Kwei
  • Alex Lacerda (p)
  • Henry Laquer '47-'77
  • Don Liebenberg
  • Don Lester
  • Jim Lindsay
  • Earl Long
  • Marty Maley (p) '65-'67 & '74-'89
  • Tom McDonald
  • Albert Migliori (p)
  • Bob Mills
  • Gil Miranda
  • Jan Novak '60-'70
  • Bill Overton
  • Denis Pelekhov (p)
  • Cal Potts
  • Art Ramirez
  • Jeff Roberts
  • Tom Roberts
  • George Rodriguez (p)
  • John Rogers '51-'92
  • Ray Rylander
  • Tom Sandenaw
  • John Sarrao (s)
  • Dave Schiferl (p)
  • Adam Schuch '49-??
  • Al Sesonske
  • Bob Sherman
  • Bob Shermer
  • Henry Sommers
  • Walt Stewart
  • Bill Steyert
  • Bob Stokes
  • John Sullivan
  • Steve Sydoriak '48-'80
  • Dean Taylor '54-'90
  • Toni Taylor
  • Joe Tesmer
  • Walt Trela
  • John Wheatley '81-'86
  • Ken Williamson
  • Walt Willis '60-??
  • Jeff Willis (p)
  • Mahlon Wilson '65-'67
  • Stefan Wipf

Technicians and machinists

  • present
  • Carmen Espinoza
  • Kevin Graham
  • Warren Pierce
  • Roy Rockage
  • Mike Torrez
  • Todd Womack
  • former
  • Bob Aiken
  • John Bailey
  • Thom Bell
  • Marcus Bennett
  • Johnathan Betts
  • Art Briesmeister
  • Dick Briesmeister
  • Bob Candler
  • Don Clinton
  • Bob Chrisman
  • Bob Cole
  • Yates Coulter
  • Sam Cunningham
  • Glen Dill
  • Jack Dyson
  • Albert Eisensee
  • Chris Espinoza
  • Caleb Evans
  • Harry Ficht
  • Stretch Fretwell
  • Eleutario Garcia
  • Guadalupe Garcia
  • Barney Geelan '51-'83
  • Ron Haggard
  • Dean Harkleroad
  • Clarence Harmer
  • Doug Hatch
  • Jim Harlow '48-'78
  • Harvey Haagenstad
  • Joe Hand
  • Bob Johns
  • Joe King
  • Epolito Lopez
  • Mike McClannahan
  • Willard McCormick
  • Quinn McCulloch
  • Jimmy Martinez
  • Joe Martinez
  • Robert Martinez
  • Candido Maestas
  • Eldon Murley (?)
  • Bob Oziemski
  • Tim Pierce
  • Ernesto Romero
  • Jen Roper
  • Ray Rylander
  • Leander Salzer
  • Paul Saunier
  • Leroy Schmidt
  • Bob Stokes
  • James Taylor '63-'81
  • Ike Valdez
  • Sherman Vernon
  • Jimmy Wade
  • Gerry Weeks
  • Bill Yeamons

Secretaries and admins

  • present
  • Juanita Armijo
  • former
  • Judy Ackerhalt
  • Maxine Beckmann
  • Peg Bivins
  • Virginia Brennan
  • Michelle Brewer
  • Judi Briesmeister, '74-'76
  • Sylvia Charmatz
  • Betsy Coca
  • Mary Curfman
  • Adeline Damiano
  • Stephanie Davis
  • Gin Desjardin
  • Judy Gallegos
  • Julie Gallegos
  • Claire Gillis
  • Helen Hansen
  • Carol Harkleroad
  • Eunice Kern
  • Melanie Maestas
  • Vicky Maestas
  • Manuelita Mtz-Brito
  • Lou Miller
  • Shirley Montoya
  • Nancy Morrison
  • Pam Rockage
  • Norma Stibbard
  • Nissa Strottman

Post docs and students

  • ("s" indicates student)
  • present
  • Mahesh Bandi
  • Tod Caldwell
  • Jun Chen
  • John Clark (s)
  • Peter Hoseman
  • Tomasz Klimczuk
  • Han-Oh Lee
  • Evgueni Nazaretski
  • Tuson Park
  • Eric Schelter
  • Yoshi Tokiwa
  • Mike Twardos
  • Ricardo Urbano
  • former
  • Clint Ackerman
  • Jason Alexander (s)
  • Ballard Andrews
  • Meigan Aronson
  • Marie Aronsson
  • Melanie Asaki (s)
  • Fedor Balakirev
  • Marty Banton
  • Ward Beyermann
  • Simon Billinge
  • Robert Blyth
  • Corwin Booth
  • Hortencio Borges
  • Tamas Borzsonyi
  • Steve Boyd (s)
  • J. Boyer
  • Tim Braje (s)
  • Theresa Brandman (s)
  • John Brisson
  • Stuart Brown
  • Scott Buchanan
  • Lou Bucholtz
  • Francesca Calgaro
  • Keith Carroll
  • Paul Canfield
  • Bill Challener
  • Houtang Chen
  • Sang Cheong (s)
  • Elbert Chia
  • H. Coburn
  • Andy Cornelius
  • Gary Cort
  • Zahir Daya
  • Giovanni Donati (s)
  • Peter Ebey
  • Matt Eisaman (s)
  • John Engelhardt
  • Dennis Erickson
  • Arshang Fartash (s)
  • Franz Freibert
  • Jim Fraser
  • Veronika Fritsch
  • Andy Fusco
  • Brian Gamble (s)
  • Elke Gampers (s)
  • Jason Gardner
  • Drew Geller
  • Tom Graf
  • Chunlei Guo
  • Ela Guziewicz
  • (Dave?) Haensch
  • Mike Hayden
  • Hans Haucke (s)
  • Kaden Hazzard (s)
  • Helmut Hegger
  • Jerry Helfrich (s)
  • Jeff Hill
  • Bob Hiller
  • David Hilton
  • Daniela Hristova (s)
  • Tom Hofler (s)
  • Yuchou Hu
  • Namjung Hur
  • Randy Jacobs (s)
  • Marcelo Jaime
  • Kimberly Jantunen (s)
  • Del Jones
  • Ki-Yong Kim
  • Yongmin Kim
  • Padma Kodali
  • Vince Kotsubo
  • Ken Krane
  • Raymond Kwok (s)
  • Lianping Le
  • Hae Ja Lee
  • Ming Lei
  • Jason Leonard (s)
  • Rich LeSar
  • Jon Levine (s)
  • K.C. Lim
  • Ana Lima
  • Scott List
  • Yuanming Liu
  • Anna Llobet
  • Ahmed Lobad
  • Despo Louca
  • Mary Lowe
  • McLean Machut
  • Yoshi Maeno (s)
  • David Mandrus
  • Joe Martindale
  • Janine Martinez (s)
  • Karlene Maskaly (s)
  • Joe Matthews (s)
  • Konstantin Matveev
  • Pat Maxton (s)
  • Mike McHenry
  • Chuck Mielke
  • Robert Modler
  • David Moore
  • Greg Moore
  • Mark Moores (s)
  • Evangelia Moshopoulou
  • Karl Mueller
  • Carl Mungan
  • John Neumeier
  • Michael Nicklas
  • Fenglei Niu
  • John Norvell
  • John O'Hara
  • Jeff Olson
  • Fiorenzo Omenetto
  • Willie Padilla
  • Pascoal Pagliuso
  • Cedomir Petrovic (s)
  • Long Pham (s)
  • Rohit Prasankumar
  • Bill Pratt
  • Andrea Prodi (s)
  • Dave Reagor
  • Bob Reid (s)
  • Erin Rericha (s)
  • Arneil Reyes
  • Brandon Rohrer
  • Larry Schwalbe
  • John Shier
  • Shoou-Shinn Shiah (s)
  • Craig Siders
  • Jenifer Siders
  • Barb Simovic
  • Dipen Sinha
  • Jim Sites
  • Bart Smith
  • Mike Smith
  • Jin So
  • Jeff Sonier
  • Guenter Sparn
  • Phil Spoor
  • Andrew Stockham (s)
  • Thor Stromberg
  • Byong Jin Suh
  • Tim Sullivan
  • Andreas Suter
  • Verner Thorsmolle
  • Rod Thurston
  • Peter Vorobieff
  • Bill Ward
  • Atsu Watanabe (s)
  • Dzmitry Yarotski (s)
  • Balakishore Yellampalle
  • Yohsuke Yoshinari
  • Ben-Li Young
  • Huidan Yu
  • Zhenyong Zhang
  • Fang Zhong
  • E. Zirngiebl
  • Bob Ziff
  • Carl Zimm

Long-term visitors

  • (visiting staff members, consultants, collaborators)
  • present
  • Tim Darling
  • Leticie Ferreira
  • Zach Fisk
  • Bob Heffner
  • Jon Lawrence
  • Moshe Pasternak
  • Vladimir Sidorov
  • Dean Taylor
  • former
  • whose names do not appear elsewhere
  • Bernie Abraham
  • Paul Barrett
  • Jacob Bigeleisen
  • Ferdinand Brickwedde
  • Bob Brout
  • Ludwig Bruch
  • John Clem
  • Eddie Cohen
  • Michael Cohen
  • Heikke Collan
  • John Daunt
  • Daniel Decker
  • Mel Daybell
  • Yehiel Disatnik
  • Dick Etters
  • Henry Fairbank
  • Hans Frauenfelder
  • Louis Goldstein
  • Lenny Gruenberg
  • George Gruner
  • Bob Hake
  • A. Hildebrandt
  • Dieter Hochheimer
  • Col. Hutchinson
  • Elisha Huggins
  • Hubert James
  • Henry Kierstead
  • John Kilpatrick
  • Myra Kilpatrick
  • Matti Krusius
  • Sig Larsen
  • Elliott Leib
  • Bob Leisure
  • Doug MacLaughlin
  • Dillon Mapother
  • Darrell Osborne
  • Hans Ott
  • Ron Parks
  • C. B. Pierce
  • Philippe Pruzan
  • John Raich
  • Roger Shaw
  • John Sheliak
  • Sergei Stishov
  • Masashi Takigawa
  • Hirofumi Wada
  • Bernie Weinstock
  • Gene Wells
Operated by Los Alamos National Security, LLC for the U.S. Department of Energy's NNSA
Inside | © Copyright 2014 Los Alamos National Security, LLC All rights reserved | Disclaimer/Privacy | Web Contact