Luis Walter Alvarez

Luis Walter Alvarez (June 13, 1911 – September 1, 1988) was an American experimental physicist, inventor, and professor who was awarded the Nobel Prize in Physics in 1968 for development of the hydrogen bubble chamber enabling discovery of resonance states in particle physics. The American Journal of Physics commented, "Luis Alvarez was one of the most brilliant and productive experimental physicists of the twentieth century."[1]

Luis Walter Alvarez
Born(1911-06-13)June 13, 1911
DiedSeptember 1, 1988(1988-09-01) (aged 77)
NationalityAmerican
Alma materUniversity of Chicago
Spouse(s)
Geraldine Smithwick
(m. 1936; div. 1957)

Janet L. Landis
(m. 1958)
AwardsMedal for Merit (1947)
National Medal of Science (1963)
Nobel Prize in Physics (1968)
Enrico Fermi Award (1987)
Scientific career
FieldsPhysics
InstitutionsUniversity of California, Berkeley
Doctoral advisorArthur Compton
Signature

After receiving his PhD from the University of Chicago in 1936, Alvarez went to work for Ernest Lawrence at the Radiation Laboratory at the University of California, Berkeley. Alvarez devised a set of experiments to observe K-electron capture in radioactive nuclei, predicted by the beta decay theory but never before observed. He produced tritium using the cyclotron and measured its lifetime. In collaboration with Felix Bloch, he measured the magnetic moment of the neutron.

In 1940 Alvarez joined the MIT Radiation Laboratory, where he contributed to a number of World War II radar projects, from early improvements to Identification friend or foe (IFF) radar beacons, now called transponders, to a system known as VIXEN for preventing enemy submarines from realizing that they had been found by the new airborne microwave radars. Enemy submarines would wait until the radar signal was getting strong and then submerge, escaping attack. But VIXEN transmitted a radar signal whose strength was the cube of the distance to the submarine so that as they approached the sub, the signal—as measured by the sub—got progressively weaker, and the sub assumed the plane was getting farther away and didn't submerge.[2][3] The radar system for which Alvarez is best known and which has played a major role in aviation, most particularly in the post war Berlin airlift, was Ground Controlled Approach (GCA). Alvarez spent a few months at the University of Chicago working on nuclear reactors for Enrico Fermi before coming to Los Alamos to work for Robert Oppenheimer on the Manhattan project. Alvarez worked on the design of explosive lenses, and the development of exploding-bridgewire detonators. As a member of Project Alberta, he observed the Trinity nuclear test from a B-29 Superfortress, and later the bombing of Hiroshima from the B-29 The Great Artiste.

After the war Alvarez was involved in the design of a liquid hydrogen bubble chamber that allowed his team to take millions of photographs of particle interactions, develop complex computer systems to measure and analyze these interactions, and discover entire families of new particles and resonance states. This work resulted in his being awarded the Nobel Prize in 1968. He was involved in a project to x-ray the Egyptian pyramids to search for unknown chambers. With his son, geologist Walter Alvarez, he developed the Alvarez hypothesis which proposes that the extinction event that wiped out the non-avian dinosaurs was the result of an asteroid impact.

Alvarez was a member of the JASON Defense Advisory Group, the Bohemian Club, and the Republican Party.[4]

Early life

Luis Walter Alvarez was born in San Francisco on June 13, 1911, the second child and oldest son of Walter C. Alvarez, a physician, and his wife Harriet née Smyth, and a grandson of Luis F. Álvarez, a Spanish physician, born in Asturias, Spain, who lived in Cuba for a while and finally settled in the United States, who found a better method for diagnosing macular leprosy. He had an older sister, Gladys, a younger brother, Bob, and a younger sister, Bernice.[5] His aunt, Mabel Alvarez, was a California artist specializing in oil painting.[6]

He attended Madison School in San Francisco from 1918 to 1924, and then San Francisco Polytechnic High School.[7] In 1926, his father became a researcher at the Mayo Clinic, and the family moved to Rochester, Minnesota, where Alvarez attended Rochester High School. He had always expected to attend the University of California, Berkeley, but at the urging of his teachers at Rochester, he instead went to the University of Chicago,[8] where he received his bachelor's degree in 1932, his master's degree in 1934, and his PhD in 1936.[9] As an undergraduate, he belonged to the Phi Gamma Delta fraternity. As a postgraduate he moved to Gamma Alpha.[10]

In 1932, as a graduate student at Chicago, he discovered physics there and had the rare opportunity to use the equipment of legendary physicist Albert A. Michelson.[11] Alvarez also constructed an apparatus of Geiger counter tubes arranged as a cosmic ray telescope, and under the aegis of his faculty advisor Arthur Compton, conducted an experiment in Mexico City to measure the so-called East–West effect of cosmic rays. Observing more incoming radiation from the west, Alvarez concluded that primary cosmic rays were positively charged. Compton submitted the resulting paper to the Physical Review, with Alvarez's name at the top.[12]

Alvarez was an agnostic.[13]

Early work

Nobel Laureate Arthur Compton, left, with young graduate student Luis Alvarez at the University of Chicago in 1933

Alvarez's sister, Gladys, worked for Ernest Lawrence as a part-time secretary, and mentioned Alvarez to Lawrence. Lawrence then invited Alvarez to tour the Century of Progress exhibition in Chicago with him.[14] After he completed his oral exams in 1936, Alvarez, now engaged to be married to Geraldine Smithwick, asked his sister to see if Lawrence had any jobs available at the Radiation Laboratory. A telegram soon arrived from Gladys with a job offer from Lawrence. This started a long association with the University of California, Berkeley. Alvarez and Smithwick were married in one of the chapels at the University of Chicago and then headed for California.[15] They had two children, Walter and Jean.[16] They were divorced in 1957. On December 28, 1958, he married Janet L. Landis, and had two more children, Donald and Helen.[17]

At the Radiation Laboratory he worked with Lawrence's experimental team, which was supported by a group of theoretical physicists headed by Robert Oppenheimer.[18] Alvarez devised a set of experiments to observe K-electron capture in radioactive nuclei, predicted by the beta decay theory but never observed. Using magnets to sweep aside the positrons and electrons emanating from his radioactive sources, he designed a special purpose Geiger counter to detect only the "soft" X-rays coming from K capture. He published his results in the Physical Review in 1937.[19][20]

When deuterium (hydrogen-2) is bombarded with deuterium, the fusion reaction yields either tritium (hydrogen-3) plus a proton or helium-3 plus a neutron (2
H
+ 2
H
3
H
+ p or 3
He
+ n
). This is one of the most basic fusion reactions, and the foundation of the thermonuclear weapon and the current research on controlled nuclear fusion. At that time the stability of these two reaction products was unknown, but based on existing theories Hans Bethe thought that tritium would be stable and helium-3 unstable. Alvarez proved the reverse by using his knowledge of the details of the 60-inch cyclotron operation. He tuned the machine to accelerate doubly ionized helium-3 nuclei and was able to get a beam of accelerated ions, thus using the cyclotron as a kind of super mass spectrometer. As the accelerated helium came from deep gas wells where it had been for millions of years, the helium-3 component had to be stable. Afterwards Alvarez produced the radioactive tritium using the cyclotron and the 2
H
+ 2
H
reaction and measured its lifetime.[21][22][23]

In 1938, again using his knowledge of the cyclotron and inventing what are now known as time-of-flight techniques, Alvarez created a mono-energetic beam of thermal neutrons. With this he began a long series of experiments, collaborating with Felix Bloch, to measure the magnetic moment of the neutron. Their result of μ0 = 1.93±0.02 μN, published in 1940, was a major advance over earlier work.[24]

World War II

Radiation Laboratory

The British Tizard Mission to the United States in 1940 demonstrated to leading American scientists the successful application of the cavity magnetron to produce short wavelength pulsed radar. The National Defense Research Committee, established only months earlier by President Franklin Roosevelt, created a central national laboratory at the Massachusetts Institute of Technology (MIT) for the purpose of developing military applications of microwave radar. Lawrence immediately recruited his best "cyclotroneers", among them Alvarez, who joined this new laboratory, known as the Radiation Laboratory, on November 11, 1940.[25] Alvarez contributed to a number of radar projects, from early improvements to Identification Friend or Foe (IFF) radar beacons, now called transponders, to a system known as VIXEN for preventing enemy submarines from realizing that they had been found by the new airborne microwave radars.[26]

One of the first projects was to build equipment to transition from the British long-wave radar to the new microwave centimeter-band radar made possible by the cavity magnetron. In working on the Microwave Early Warning system (MEW), Alvarez invented a linear dipole array antenna that not only suppressed the unwanted side lobes of the radiation field, but also could be electronically scanned without the need for mechanical scanning. This was the first microwave phased-array antenna, and Alvarez used it not only in MEW but in two additional radar systems. The antenna enabled the Eagle precision bombing radar to support precision bombing in bad weather or through clouds. It was completed rather late in the war; although a number of B-29s were equipped with Eagle and it worked well, it came too late to make much difference.[27]

Receiving the Collier Trophy from President Harry Truman, White House, 1946

The radar system for which Alvarez is best known and which has played a major role in aviation, most particularly in the post war Berlin airlift, was Ground Controlled Approach (GCA). Using Alvarez's dipole antenna to achieve a very high angular resolution, GCA allows ground-based radar operators watching special precision displays to guide a landing airplane to the runway by transmitting verbal commands to the pilot. The system was simple, direct, and worked well, even with previously untrained pilots. It was so successful that the military continued to use it for many years after the war, and it was still in use in some countries in the 1980s.[28] Alvarez was awarded the National Aeronautic Association's Collier Trophy in 1945 "for his conspicuous and outstanding initiative in the concept and development of the Ground Control Approach system for safe landing of aircraft under all weather and traffic conditions".[29][30]

Alvarez spent the summer of 1943 in England testing GCA, landing planes returning from battle in bad weather, and also training the British in the use of the system. While there he encountered the young Arthur C. Clarke, who was an RAF radar technician. Clarke subsequently used his experiences at the radar research station as the basis for his novel Glide Path, which contains a thinly disguised version of Alvarez.[31] Clarke and Alvarez developed a long-term friendship.[32]

Manhattan Project

In the fall of 1943, Alvarez returned to the United States with an offer from Robert Oppenheimer to work at Los Alamos on the Manhattan project. But Oppenheimer suggested that he first spend a few months at the University of Chicago working with Enrico Fermi before coming to Los Alamos. During these months, General Leslie Groves asked Alvarez to think of a way that the US could find out if the Germans were operating any nuclear reactors, and, if so, where they were. Alvarez suggested that an airplane could carry a system to detect the radioactive gases that a reactor produces, particularly xenon 133. The equipment did fly over Germany, but detected no radioactive xenon because the Germans had not built a reactor capable of a chain reaction. This was the first idea of monitoring fission products for intelligence gathering. It would become extremely important after the war.[33]

Wearing a helmet and flak jacket and standing in front of The Great Artiste, Tinian 1945

As a result of his radar work and the few months spent with Fermi, Alvarez arrived at Los Alamos in the spring of 1944, later than many of his contemporaries. The work on the "Little Boy" (a uranium bomb) was far along so Alvarez became involved in the design of the "Fat Man" (a plutonium bomb). The technique used for uranium, that of forcing the two sub-critical masses together using a type of gun, would not work with plutonium because the high level of background spontaneous neutrons would cause fissions as soon as the two parts approached each other, so heat and expansion would force the system apart before much energy has been released. It was decided to use a nearly critical sphere of plutonium and compress it quickly by explosives into a much smaller and denser core, a technical challenge at the time.[34]

To create the symmetrical implosion required to compress the plutonium core to the required density, thirty two explosive charges were to be simultaneously detonated around the spherical core. Using conventional explosive techniques with blasting caps, progress towards achieving simultaneity to within a small fraction of a microsecond was discouraging. Alvarez directed his graduate student, Lawrence H. Johnston, to use a large capacitor to deliver a high voltage charge directly to each explosive lens, replacing blasting caps with exploding-bridgewire detonators. The exploding wire detonated the thirty two charges to within a few tenths of a microsecond. The invention was critical to the success of the implosion-type nuclear weapon. He also supervised the RaLa Experiments.[35] Alvarez later wrote that:

With modern weapons-grade uranium, the background neutron rate is so low that terrorists, if they had such material, would have a good chance of setting off a high-yield explosion simply by dropping one half of the material onto the other half. Most people seem unaware that if separated U-235 is at hand, it's a trivial job to set off a nuclear explosion, whereas if only plutonium is available, making it explode is the most difficult technical job I know.[36]

Alvarez (top right) on Tinian with Harold Agnew (top left), Lawrence H. Johnston (bottom left) and Bernard Waldman (bottom right)

Again working with Johnston, Alvarez's last task for the Manhattan Project was to develop a set of calibrated microphone/transmitters to be parachuted from an aircraft to measure the strength of the blast wave from the atomic explosion, so as to allow the scientists to calculate the bomb's energy. After being commissioned as a lieutenant colonel in the United States Army, he observed the Trinity nuclear test from a B-29 Superfortress that also carried fellow Project Alberta members Harold Agnew and Deak Parsons (who were respectively commissioned at the rank of captain).[37]

Flying in the B-29 Superfortress The Great Artiste in formation with the Enola Gay, Alvarez and Johnston measured the blast effect of the Little Boy bomb which was dropped on Hiroshima.[38] A few days later, again flying in The Great Artiste, Johnston used the same equipment to measure the strength of the Nagasaki explosion.[39]

Bubble chamber

Celebrating winning the Nobel Prize, October 30, 1968. The balloons are inscribed with the names of subatomic particles that his group discovered.

Returning to the University of California, Berkeley as a full professor, Alvarez had many ideas about how to use his wartime radar knowledge to improve particle accelerators. Though some of these were to bear fruit, the "big idea" of this time would come from Edwin McMillan with his concept of phase stability which led to the synchrocyclotron. Refining and extending this concept, the Lawrence team would build the world's then-largest proton accelerator, the Bevatron, which began operating in 1954. Though the Bevatron could produce copious amounts of interesting particles, particularly in secondary collisions, these complex interactions were hard to detect and analyze at the time.[40]

Seizing upon a new development to visualize particle tracks, created by Donald Glaser and known as a bubble chamber, Alvarez realized the device was just what was needed, if only it could be made to function with liquid hydrogen. Hydrogen nuclei, which are protons, made the simplest and most desirable target for interactions with the particles produced by the Bevatron. He began a development program to build a series of small chambers, and championed the device to Ernest Lawrence.[41]

The Glaser device was a small glass cylinder (1 cm × 2 cm) filled with ether. By suddenly reducing the pressure in the device, the liquid could be placed into a temporary superheated state, which would boil along the disturbed track of a particle passing through. Glaser was able to maintain the superheated state for a few seconds before spontaneous boiling took place. The Alvarez team built chambers of 1.5 in, 2.5 in, 4 in, 10 in, and 15 in using liquid hydrogen, and constructed of metal with glass windows, so that the tracks could be photographed. The chamber could be cycled in synchronization with the accelerator beam, a picture could be taken, and the chamber recompressed in time for the next beam cycle.[42]

This program built a liquid hydrogen bubble chamber almost 7 feet (2 meters) long, employed dozens of physicists and graduate students together with hundreds of engineers and technicians, took millions of photographs of particle interactions, developed computer systems to measure and analyze the interactions, and discovered families of new particles and resonance states. This work resulted in the Nobel Prize in Physics for Alvarez in 1968,[43] "For his decisive contributions to elementary particle physics, in particular the discovery of a large number of resonant states, made possible through his development of the technique of using hydrogen bubble chambers and data analysis."[44]

Scientific detective

In 1964 Alvarez proposed what became known as the High Altitude Particle Physics Experiment (HAPPE), originally conceived as a large superconducting magnet carried to high altitude by a balloon in order to study extremely high-energy particle interactions.[45] In time the focus of the experiment changed toward the study of cosmology and the role of both particles and radiation in the early universe. This work was a large effort, carrying detectors aloft with high-altitude balloon flights and high-flying U-2 aircraft, and an early precursor of the COBE satellite-born experiments on the cosmic background radiation (which resulted in the award of the 2006 Nobel Prize, shared by George Smoot and John Mather.[45])

X-Raying the Pyramids with Egyptologist Ahmed Fakhry and Team Leader Jerry Anderson, Berkeley, 1967

Alvarez proposed Muon tomography in 1965 to search the Egyptian pyramids for unknown chambers. Using naturally occurring cosmic rays, his plan was to place spark chambers, standard equipment in the high-energy particle physics of this time, beneath the Pyramid of Khafre in a known chamber. By measuring the counting rate of the cosmic rays in different directions the detector would reveal the existence of any void in the overlaying rock structure.[46]

Alvarez assembled a team of physicists and archeologists from the United States and Egypt, the recording equipment was constructed and the experiment carried out, though it was interrupted by the 1967 Six-Day War. Restarted after the war, the effort continued, recording and analyzing the penetrating cosmic rays until 1969 when Alvarez reported to the American Physical Society that no chambers had been found in the 19% of the pyramid surveyed.[47]

In November 1966 Life published a series of photographs from the film that Abraham Zapruder took of the Kennedy assassination. Alvarez, an expert in optics and photoanalysis, became intrigued by the pictures and began to study what could be learned from the film. Alvarez demonstrated both in theory and experiment that the backward snap of the President's head was fully consistent with his being shot from behind. He also investigated the timing of the gunshots and the shockwave which disturbed the camera, and the speed of the camera, pointing out a number of things which the FBI photo analysts either overlooked or got wrong. He produced a paper intended as a tutorial, with informal advice for the physicist intent on arriving at the truth.[48]

Dinosaur extinction

Luis and Walter Alvarez at the K-T Boundary in Gubbio, Italy, 1981

In 1980 Alvarez and his son, geologist Walter Alvarez, along with nuclear chemists Frank Asaro and Helen Michel, "uncovered a calamity that literally shook the Earth and is one of the great discoveries about Earth's history".[1]

During the 1970s, Walter Alvarez was doing geologic research in central Italy. There he had located an outcrop on the walls of a gorge whose limestone layers included strata both above and below the Cretaceous–Paleogene boundary. Exactly at the boundary is a thin layer of clay. Walter told his father that the layer marked where the dinosaurs and much else became extinct and that nobody knew why, or what the clay was about — it was a big mystery and he intended to solve it.[1]

Alvarez had access to the nuclear chemists at the Lawrence Berkeley Laboratory and was able to work with Frank Asaro and Helen Michel, who used the technique of neutron activation analysis. In 1980, Alvarez, Alvarez, Asaro, and Michel published a seminal paper proposing an extraterrestrial cause for the Cretaceous-Paleogene extinction (then called the Cretaceous-Tertiary extinction).[49] In the years following the publication of their article, the clay was also found to contain soot, glassy spherules, shocked quartz crystals, microscopic diamonds, and rare minerals formed only under conditions of great temperature and pressure.[1]

Publication of the 1980 paper brought criticism from the geologic community, and an often acrimonious scientific debate ensued. Ten years later, and after Alvarez's death, evidence of a large impact crater called Chicxulub was found off the coast of Mexico, providing support for the theory. Other researchers later found that the end-Cretaceous extinction of the dinosaurs may have occurred rapidly in geologic terms, over thousands of years, rather than millions of years as had previously been supposed. Others continue to study alternative extinction causes such as increased volcanism, particularly the massive Deccan Traps eruptions that occurred around the same time, and climate change, checking against the fossil record. However, on March 4, 2010, a panel of 41 scientists agreed that the Chicxulub asteroid impact triggered the mass extinction.[50]

Aviation

In his autobiography, Alvarez said, "I think of myself as having had two separate careers, one in science and one in aviation. I've found the two almost equally rewarding." An important contributor to this was his enjoyment of flying. He learned to fly in 1933, later earning instrument and multi-engine ratings. Over the next 50 years he accumulated over 1000 hours of flight time, most of it as pilot in command.[51] He said, "I found few activities as satisfying as being pilot in command with responsibility for my passengers' lives."[52]

Alvarez made numerous professional contributions to aviation. During World War II he led the development of multiple aviation-related technologies. Several of his projects are described above, including Ground Controlled Approach (GCA) for which he was awarded the Collier Trophy in 1945. He also held the basic patent for the radar transponder, for which he assigned rights to the U.S. government for $1.[51]

Later in his career Alvarez served on multiple high level advisory committees related to civilian and military aviation. These included a Federal Aviation Administration task group on future air navigation and air traffic control systems, the President's Science Advisory Committee Military Aircraft Panel, and a committee studying how the scientific community could help improve the United States' capabilities for fighting a nonnuclear war.[53]

Alvarez's aviation responsibilities led to many adventures. For example, while working on GCA he became the first civilian to fly a low approach with his view outside the cockpit obstructed. He also flew many military aircraft from the co-pilot's seat, including a B-29 Superfortress[52] and a Lockheed F-104 Starfighter.[54] In addition, he survived a crash during World War II as a passenger in a Miles Master.[55]

Death

Alvarez died on September 1, 1988, due to complications from a succession of recent operations for esophageal cancer.[56] His remains were cremated, and his ashes were scattered over Monterey Bay.[57] His papers are in The Bancroft Library at the University of California, Berkeley.[58]

Awards and honors

Selected publications

Patents

  • Golf training device[73]
  • Electronuclear Reactor [74]
  • Optical range finder with variable angle exponential prism[75]
  • Two-element variable-power spherical lens[76]
  • Variable-power lens and system[77]
  • Subatomic particle detector with liquid electron multiplication medium[78]
  • Method of making Fresnelled optical element matrix[79]
  • Optical element of reduced thickness[80]
  • Method of forming an optical element of reduced thickness[81]
  • Deuterium tagged articles such as explosives and method for detection thereof [82]
  • Stabilized zoom binocular [83]
  • Stand alone collision avoidance system [84]
  • Television viewer[85]
  • Stabilized zoom binocular [86]
  • Optically stabilized camera lens system [87]
  • Nitrogen detection [88]
  • Inertial pendulum optical stabilizer [89]

Notes

  1. Wohl, C. G. (2007). "Scientist as detective: Luis Alvarez and the pyramid burial chambers, the JFK assassination, and the end of the dinosaurs". American Journal of Physics. 75 (11): 968. Bibcode:2007AmJPh..75..968W. doi:10.1119/1.2772290.
  2. Alvarez, L. W. (1987). Alvarez: Adventures of a Physicist. Basic Books, p.92, last paragraph, et seq., ISBN 0-465-00115-7.
  3. Fractals, Chaos and Power Laws, Manfred Schroeder, Dover, 1991, p.33.
  4. Trower, W. P. (2009). Luis Walter Alvarez 1911–1988 (PDF). Biographical Memoirs. National Academy of Sciences. Retrieved March 21, 2013.
  5. Alvarez 1987, pp. 9–10.
  6. Fernandez, R. M. (September 2011). "A Finding Aid to the Mabel Alvarez Papers, 1898–1987, in the Archives of American Art". Archives of American Art. Retrieved June 15, 2011.
  7. Trower 1987, p. 259.
  8. Alvarez 1987, pp. 12–16.
  9. "Luis W. Alvarez – Biography". Nobelprize.org. Retrieved April 17, 2011.
  10. Alvarez 1987, pp. 23–24.
  11. Alfred B. Bortz. Physics: Decade by Decade. Facts On File, Incorporated; 2007. ISBN 978-0-8160-5532-6. p. 168.
  12. Alvarez 1987, pp. 25–27.
  13. Alvarez: adventures of a physicist. Basic Books. 1987. p. 279. ISBN 9780465001156. "Physicists feel that the subject of religion is taboo. Almost all consider themselves agnostics. We talk about the big bang that started the present universe and wonder what caused it and what came before. To me the idea of a Supreme Being is attractive, but I'm sure that such a Being isn't the one described in any holy book. Since we learn about people by examining what they have done, I conclude that any Supreme Being must have been a great mathematician. The universe operates with precision according to mathematical laws of enormous complexity. I'm unable to identify its creator with the Jesus to whom my maternal grandparents, missionaries in China, devoted their lives."
  14. Alvarez 1987, p. 31.
  15. Alvarez 1987, p. 38.
  16. Alvarez 1987, p. 284.
  17. Alvarez 1987, pp. 205–207, 281.
  18. Alvarez 1987, pp. 46–48.
  19. Alvarez, L. W. (1937). "Nuclear K Electron Capture". Physical Review. 52 (2): 134–135. Bibcode:1937PhRv...52..134A. doi:10.1103/PhysRev.52.134.
  20. Alvarez 1987, pp. 54–55.
  21. Alvarez, L. W.; Cornog, R. (1939). "Helium and Hydrogen of Mass 3". Physical Review. 56 (6): 613. Bibcode:1939PhRv...56..613A. doi:10.1103/PhysRev.56.613.
  22. Trower 2009, p. 6.
  23. Alvarez 1987, pp. 67–71.
  24. Alvarez, Luis W.; Bloch, F. (1940). "A Quantitative Determination of the Neutron Moment in Absolute Nuclear Magnetons". Physical Review. 57 (2): 111–122. Bibcode:1940PhRv...57..111A. doi:10.1103/PhysRev.57.111.
  25. Alvarez 1987, pp. 78–85.
  26. Alvarez 1987, pp. 90–93.
  27. Alvarez 1987, pp. 101–103.
  28. Alvarez 1987, pp. 96–100.
  29. "Collier 1940–1949 Winners". National Aeronautic Association. Archived from the original on December 3, 2013. Retrieved March 21, 2013.
  30. "Radar Expert will Receive Collier Trophy". The Courier-Journal. Louisville, Kentucky. Associated Press. December 13, 1946. p. 16 via Newspapers.com.
  31. Alvarez 1987, pp. 104–110.
  32. Alvarez 1987, pp. 110.
  33. Alvarez 1987, pp. 114–121.
  34. Alvarez 1987, pp. 123–128.
  35. Alvarez 1987, pp. 131–136.
  36. Alvarez 1987, p. 125.
  37. Alvarez 1987, pp. 137–142.
  38. Alvarez 1987, pp. 6–8.
  39. Alvarez 1987, pp. 144–146.
  40. Alvarez 1987, pp. 153–159.
  41. Alvarez 1987, pp. 185–189.
  42. Alvarez 1987, pp. 190–194.
  43. Alvarez 1987, pp. 196–199.
  44. "The Nobel Prize in Physics 1968". The Nobel Foundation. Retrieved March 21, 2013.
  45. Alvarez, L. W. (1964). "A Study of High Energy Interactions Using a "Beam" of Primary Cosmic Ray Protons" (PDF). Alvarez Physics Memo (503). Retrieved March 21, 2013.
  46. Alvarez, L. W. (1965). "A Proposal to "X-Ray" the Egyptian Pyramids to Search for Presently Unknown Chambers" (PDF). Alvarez Physics Memo (544). Retrieved March 21, 2013.
  47. Alvarez 1987, pp. 232–236.
  48. Alvarez 1987, pp. 239–250.
  49. Alvarez, L. W.; Alvarez, W.; Asaro, F.; Michel, H. V. (1980). "Extraterrestrial Cause for the Cretaceous-Tertiary Extinction: Experiment and Theory" (PDF). Science. 208 (4448): 1095–1108. Bibcode:1980Sci...208.1095A. doi:10.1126/science.208.4448.1095. JSTOR 1683699. PMID 17783054. S2CID 16017767.
  50. Schulte, P.; et al. (2010). "The Chicxulub Asteroid Impact and Mass Extinction at the Cretaceous- Paleogene Boundary" (PDF). Science. 327 (5970): 1214–1218. Bibcode:2010Sci...327.1214S. doi:10.1126/science.1177265. PMID 20203042. S2CID 2659741.
  51. Alvarez 1987, pp. 30–31.
  52. Alvarez 1987, pp. 268.
  53. Alvarez 1987, pp. 218–223.
  54. Alvarez 1987, pp. 224.
  55. Alvarez 1987, pp. 108.
  56. Sullivan, Walter (September 2, 1988). "Luis W. Alvarez, Nobel Physicist Who Explored Atom, Dies at 77". The New York Times. ISSN 0362-4331. Retrieved January 23, 2016.
  57. "Luis W. Alvarez". Soylent Communications. Retrieved March 21, 2013.
  58. "Finding Aid to the Luis W. Alvarez Papers, 1932–1988, bulk 1943–1987". Online Archive of California. Retrieved March 21, 2013.
  59. "Collier Trophy: Collier 1940–1949 Winners". National Aeronautical Association. Archived from the original on December 3, 2013. Retrieved April 17, 2011.
  60. "Luis Walter Alvarez 1911–1988" (PDF). National Academy of Sciences. Retrieved April 17, 2011.
  61. "Dr. Luis Walter Alvarez – Public Profile". American Philosophical Society. Archived from the original on March 19, 2012. Retrieved April 17, 2011.
  62. "Book of Members, 1780–2010: Chapter A" (PDF). American Academy of Arts and Sciences. Retrieved April 17, 2011.
  63. "California Scientist of the Year Award Recipients". California Science Center. Archived from the original on February 5, 2012. Retrieved March 21, 2012.
  64. "Golden Plate Awardees of the American Academy of Achievement". www.achievement.org. American Academy of Achievement.
  65. "National Medal of Science". American Institute of Physics. Archived from the original on August 8, 2016. Retrieved March 21, 2012.
  66. "The Michelson Lectures and Award" (PDF). Case Western Reserve University. Retrieved March 21, 2012.
  67. "Dr. Luis W. Alvarez". National Academy of Engineering. Retrieved April 17, 2011.
  68. "Alumni Awards winners". University of Chicago. Retrieved March 21, 2012.
  69. "Hall of Fame / Inventor Profile – Luis Walter Alvarez". National Inventors Hall of Fame. Archived from the original on July 6, 2010. Retrieved March 21, 2012.
  70. "Luis Alvarez, 1987". The Enrico Fermi Award. US Department of Energy. Archived from the original on November 1, 2014. Retrieved April 17, 2011.
  71. "IEEE Honorary membership recipients" (PDF). IEEE. Retrieved April 17, 2011.
  72. "Boy Scout award requirements". Archived from the original on July 30, 2016. Retrieved January 20, 2015.
  73. Alvarez, Luis W. (4 March 1958). "Golf training device." U.S. Patent No. 2,825,569. Washington, DC: U.S. Patent and Trademark Office.
  74. Lawrence, E. O., McMillan, E. M., & Alvarez, L. W. (1960). Electronuclear Reactor (No. US 2933442).
  75. Alvarez, L. W. (24 January 1967). "Optical range finder with variable angle exponential prism." U.S. Patent No. 3,299,768. Washington, DC: U.S. Patent and Trademark Office.
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  79. Alvarez, L. (19 June 1973). "Method of making fresnelled optical element matrix." U.S. Patent No. 3,739,455. Washington, DC: U.S. Patent and Trademark Office.
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  82. Alvarez, Luis W.,(17 February 1981). "Deuterium tagged articles such as explosives and method for detection thereof." U.S. Patent No. 4,251,726. Washington, DC: U.S. Patent and Trademark Office.
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  84. Alvarez, Luis W. (23 February 1982). "Stand alone collision avoidance system." U.S. Patent No. 4,317,119. Washington, DC: U.S. Patent and Trademark Office.
  85. Alvarez, Luis W., (16 August 1983). "Television viewer." U.S. Patent No. 4,399,455. Washington, DC: U.S. Patent and Trademark Office.
  86. Alvarez, Luis W., and Schwemin, Arnold J. (29 November 1983). "Stabilized zoom binocular." U.S. Patent No. 4,417,788. Washington, DC: U.S. Patent and Trademark Office.
  87. Alvarez, Luis W., and Schwemin, Arnold J. (7 October 1986). "Optically stabilized camera lens system." U.S. Patent No. 4,615,590. Washington, DC: U.S. Patent and Trademark Office.
  88. Alvarez, Luis W. (12 July 1988). "Nitrogen detection." U.S. Patent No. 4,756,866. Washington, DC: U.S. Patent and Trademark Office.
  89. Alvarez, Luis W., and Sporer, Stephen F. (27 March 1990). "Inertial pendulum optical stabilizer." U.S. Patent No. 4,911,541. Washington, DC: U.S. Patent and Trademark Office.

References

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