| Dates | Characters | Theories and discoveries |
| 1941 | MacMillan, Kennedy, Seaborg, Wahl | Element 94, plutonium, second transuranian elements |
| 1941 | Lev Davidovich Landau | Theory of superfluids |
| 1941 | Rossi and Hall | Muon decay used to verify relativistic time dilation |
| 1941 | Mckellar and Adams | Cosmic cyanogen observed to be at temperature of CBR, but significance not recognised |
| 1941 | J. Robert Oppenheimer | “Manhatten Project” is founded to develop atomic bomb |
| 1942 | Enrico Fermi | The first self sustaining fission reaction |
| 1942 | Grote Reber | Radio map of the sky |
| 1943 | Ernest Stueckelberg | Renormalisation of QED |
| 1943 | Sakata, Inoue | Theory of pion decay to muons |
| 1944 | Lars Onsager | General theory of phase transitions |
| 1944 | Seaborg, James, Morgan, Ghiorso, Thompson | Elements 95; americium, 96; curium |
| 1944 | Leprince-Ringuet and Lheritier | The K+ found in cosmic rays |
| 1945 | Robert Oppenheimer et al | First atomic bomb |
| 1945 | Mauchly and Eckert | First electronic computer ENIAC |
| 1946 | James Hey | Discovery of radio source Cygnus A |
| 1946 | George Gamow | Cold big bang model |
| 1946 | Bloch and Purcell | Nuclear magnetic resonance |
| 1947 | Claude Shannon | Information theory |
| 1947 | Conversi, Pancini, Piccioni | Indication that the muon is not the mediator of the strong force |
| 1947 | Hartmut Kallman | Scintillation counter |
| 1947 | Denis Gabor | Theory of holograms |
| 1947 | Powell, Occhialini | Negative pion found |
| 1947 | Willis Lamb | Fine structure of hydrogen spectrum, the Lamb shift |
| 1947 | Hans Bethe | Renormalisation of Lamb shift calculation |
| 1947 | Kusch and Folley | Measurement of the anomolous magnetic moment of the electron |
| 1947 | Hartland Snyder | Quantised space-time |
| 1948 | Tomonaga, Schwinger, Feynman | Renormalisation of QED |
| 1948 | Alpher, Bethe & Gamow | Explain nucleosynthesis in hot big bang |
| 1948 | Alpher and Herman | Prediction of cosmic background radiation |
| 1948 | Bondi, Gold, Hoyle | Steady state theory of the universe |
| 1948 | Goldhaber & Goldhaber | Experimental proof that beta particles are electrons |
| 1948 | Richard Feynman | Path integral approach to quantum theory |
| 1948 | Bardeen, Brattain, Shockley | Semi-conductors and transistors |
| 1948 | Snell and Miller | Decay of the neutron |
| 1948 | Freeman Dyson | Equivalence of Feynman and Schwinger-Tomonaga QED |
| 1948 | Hendrik Casimir | Theory of Casimir force |
| 1949 | Leighton, Anderson, Seriff | Muon is spin half |
| 1949 | Seaborg, Ghiorso, Thompson | Element 97, berkelium |
| 1949 | Haxel, Jensen, Mayer, Suess | Nuclear shell model |
| 1949 | Fred Hoyle | First use of the term “big bang” |
| 1950 | Paul Dirac | First suggestion of string theory |
| 1950 | Seaborg, Ghiorso, Street, Thompson | Element 98, californium |
| 1950 | Jan Oort | Theory of comet origins |
| 1950 | Bjorklund, Crandall, Moyer, York | Neutral pion |
| 1950 | Albert Einstein | Einstein’s failed unified theory |
| 1951 | Smith and Baade | Identify a radio galaxy |
| 1951 | Petermann, Stueckelberg | Renormalisation group |
| 1952 | Courant, Livingston, Snyder | Strong focusing principle for particle accelerators |
| 1952 | Glaser, Alvarez | Bubble chamber |
| 1952 | Seaborg et al | Elements 99; einsteinium, 100; fermium |
| 1952 | Walter Baade | Resolves confusion over two different types of Cepheid variable stars |
| 1952 | Edward Teller et al | Hydrogen bomb |
| 1952 | Joseph Weber | Described the principle of the maser |
| 1953 | Gell-Mann and Nishijima | Strangeness |
| 1953 | Gerard de Vaucouleurs | Galaxy superclusters and large scale inhomogenieties |
| 1953 | Charles Townes | Maser |
| 1953 | Alpher, Herman, Follin | First recognition of the horizon problem in cosmology |
| 1954 | Yang and Mills | Non-abelian gauge theory |
| 1954 | Low and Gell-Mann | Renormalisation group revisited |
| 1955 | Louis Essen | Caesium atomic clock |
| 1955 | Martin Ryle | Radio telescope interferometry |
| 1955 | John Wheeler | Describes the space-time foam at the Planck scale |
| 1955 | Ilya Prigogine | Thermodynamics of irreversible processes |
| 1955 | Carl von Weizsacker | Multiple Quantisation and ur-theory |
| 1955 | Seaborg et al | Element 101, mendelevium |
| 1955 | Chamberlain, Segre & Wiegand | Anti-proton |
| 1956 | Reines and Cowan | Neutrino detection |
| 1956 | Cork, Lambertson, Piccioni, Wenzel | Evidence for anti-neutron |
| 1956 | Block, Lee and Yang | Weak interaction could violate parity |
| 1956 | Reines and Cowan | Anti-neutrino detection |
| 1956 | Erwin Muller | Field ion microscope and first images of individual atoms |
| 1956 | Cook, Lambertson, Piconi, Wentzel | Anti-neutron |
| 1968 | Abdus Salam | 2-component neutrino |
| 1957 | Burbidge, Burbidge, Hoyle, Fowler | Formation of light elements in stars |
| 1957 | Friedman, Lederman, Telegdi, Wu | Parity violation in weak decays |
| 1957 | Bardeen, Cooper, Schrieffer | BCS theory of superconductivity |
| 1957 | Hugh Everett | Many worlds interpretation of quantum mechanics |
| 1957 | Feynman, Gell-Mann, Marshak, Sudarshan | V-A theory of weak interactions |
| 1957 | John Wheeler | Pregeometry and space-time foam |
| 1958 | Townes and Schawlow | Theory of laser |
| 1958 | Martin Ryle | Evidence for evolution of distant cosmological radio sources |
| 1958 | Seaborg et al | Element 102, nobelium |
| 1958 | Gary Feinberg | Predicts that muon neutrino is distinct from electron neutrino |
| 1958 | David Finkelstein | Resolves the nature of the black hole event horizon |
| 1959 | MIT | Radar echo from Venus |
| 1959 | Ramsey, Kleppner, Goldenberg | Hydrogen maser atomic clock |
| 1959 | Tulio Regge | Theory of Regge poles |
| 1960 | Theodore Maiman | Ruby laser |
| 1960 | Martin Kruskal | New coordinates to study Schwarzschild black hole |
| 1960 | Eugene Wigner | The unreasonable effectiveness of mathematics in natural science |
| 1960 | Pound and Rebka | Measurement of gravitational red-shift |
| 1960 | Matthews and Sandage | Optical identification of a quasar |






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