| Dates | Characters | Theories and discoveries |
| 1921 | Theodor Kaluza | Unification of electromagnetics and gravity by introducing an extra dimension |
| 1921 | Bieler and Chadwick | Evidence for a strong nuclear interaction |
| 1921 | Stern and Gerlach | Measurement of atomic magnetic moments |
| 1921 | Walter G. Cady | Quartz crystal clock |
| 1921 | Charles Bury | Electronic structure of elements from their chemistry |
| 1922 | Cornelius Lanczos | Transformation of De Sitter universe to an expanding form |
| 1922 | Alexsandr Friedmann | A model of an expanding/oscillating universe with matter included |
| 1923 | Compton and Debye | Theory of Compton effect |
| 1923 | Arthur Compton | Verification of Compton effect confirms photon as particle |
| 1923 | Louis de Broglie | Predicts wave nature of particles |
| 1923 | Davisson & Kunsman | Electron diffraction |
| 1923 | Coster and von Hevesy | Element 72, hafnium |
| 1923 | Herman Weyl, De Sitter | Universe would predict a linear relation between distance and red-shift |
| 1924 | Edwin Hubble | Measured the distance to other galaxies using Cepheid variables proving that they lie outside our own |
| 1924 | Edward Appleton | Ionosphere |
| 1924 | Satyendra Bose | Derivation of Planck’s law |
| 1924 | Bose and Einstein | Statistics of photons and Bose-Einstein condensate |
| 1924 | Albert Einstein | Statistical physics of quantum boson molecular gas |
| 1924 | Wolfgang Pauli | Explanation of Zeeman effect and two-valuedness of electron state |
| 1924 | Wolfgang Pauli | The exclusion principle |
| 1924 | Ludwik Siberstein | Claims a redshift law for nebulae |
| 1925 | Walter Elsasser | Explanation of electron diffraction as wave property of matter |
| 1925 | Vesto Melvin Slipher | Red-shifts of galaxies suggest a distance/velocity relationship |
| 1925 | Robert Millikan | Rediscovery of “cosmic rays” in upper atmosphere |
| 1925 | Noddack, Tacke, Berg | Element 75, rhenium |
| 1925 | Werner Heisenberg | Transition amplitude theory of quantum mechanics |
| 1925 | Born and Jordan | Matrix interpretation of Heisenberg’s quantum mechanics |
| 1925 | Paul Dirac | Q-number theory of general quantum mechanics |
| 1925 | Pascual Jordan | Second quantisation |
| 1925 | Goudsmit and Uhlenbeck | Electron spin |
| 1925 | Enrico Fermi | Statistics of electrons |
| 1926 | Gilbert Lewis | First use of the term photon |
| 1926 | Oskar Klein | Kaluza-Klein theory |
| 1926 | Wolfgang Pauli | Derivation of spectrum of hydrogen atom by matrix methods |
| 1926 | Erwin Schroedinger | The particle wave equation |
| 1926 | Erwin Schroedinger | Derivation of spectrum of hydrogen atom using the wave equation |
| 1926 | Eckart, Pauli, Schroedinger | Equivalence of wave equation and matrix mechanics |
| 1926 | Max Born | Probability interpretation of wave function |
| 1926 | Albert Einstein | “God does not play dice” |
| 1926 | Paul Dirac | Distinction between bosons and fermions, symmetry and anti-symmetry of wave function |
| 1926 | Dirac, Jordan | Canonical transformation theory for quantum mechanics |
| 1926 | Klein, Fock & Gordon | Relativistic wave equation for scalar particles |
| 1926 | Ralph Fowler | Suggests that white dwarf stars are explained by the exclusion principle |
| 1926 | Born, Heisenberg, Jordan | Model of a quantised field |
| 1926 | Wolfgang Pauli | Momentum and position cannot be known simultaneously |
| 1926 | Werner Heisenberg | The uncertainty principle |
| 1927 | Davisson, Germer, Thomson | Verification of electron diffraction by a crystal |
| 1927 | Jan Oort | Observation of galactic rotation and spiral shape of our galaxy |
| 1927 | Niels Bohr | Principle of complementarity |
| 1927 | Paul Dirac | Quantisation of electromagnetic field, bosonic creation and anihilation operators, virtual particles, zero point energy |
| 1927 | Eugene Wigner | Conservation of parity |
| 1927 | Friedrich Hund | Quantum tunneling |
| 1927 | Heitler and London | Quantum theory can explain chemical bonding |
| 1927 | Fritz London | Electromagnetic guage is phase of Schroedinger equation |
| 1927 | Georges Lemaitre | Models of an expanding universe |
| 1927 | Niels Bohr | Copenhagen interpretation of Quantum Mechanics |
| 1928 | Condon, Gamow, Gurney | Alpha emission is due to quantum tunnelling |
| 1928 | Paul Dirac | Relativistic equation of the spin-half electron |
| 1928 | Willem Keeson | Phase transition in liquid Helium |
| 1928 | Jordan, Pauli | Quantum field theory of free fields |
| 1928 | Rolf Wideroe | First prototype high energy accelerator |
| 1928 | Heisenberg, Weyl | Group representation theory in quantum mechanics |
| 1929 | Ernest Lawrence | Cyclotron |
| 1929 | Robert van de Graaff | Van de Graaff generator |
| 1929 | Heisenberg, Pauli | Interacting quantum field theory and divergences |
| 1929 | J. Robert Oppenheimer | Divergence of electron self-energy |
| 1929 | Paul Dirac | Electron sea and hole theory |
| 1929 | Edwin Hubble | First measurement of Hubble’s constant leading to the conclusion that the Universe is expanding |
| 1929 | Bothe, Kolhorster | Cosmic rays are charged particles |
| 1930 | Clyde Tombaugh | Pluto discovered |
| 1930 | Becker, Bothe | Observed neutral rays later identified as neutrons |
| 1930 | Paul Dirac | Systematic canonical quantisation |
| 1930 | Arthur Eddington | Einstein’s static universe is unstable |
| 1930 | Hartree and Fock | Multi-particle quantum mechanics |
| 1931 | Dirac, Oppenheimer, Weyl | Prediction of anti-matter |
| 1931 | Albert Einstein | Discard cosmological constant, oscillating cosmology |
| 1931 | Georges Lemaitre | The primeval atom as origin of the universe |
| 1931 | Isidor Rabi | Principle of population inversion |
| 1931 | Wolfgang Pauli | Neutrino as explanation for missing energy and spin in weak nuclear decay |
| 1931 | Eugene Wigner | Symmetry in quantum mechanics |
| 1931 | Paul Dirac | Magnetic monopoles can explain quantum of charge |
| 1932 | Raman & Bhagavantam | Verification that photon is spin one |
| 1932 | Einstein, De Sitter | Flat expanding cosmology |
| 1932 | James Chadwick | Identified the neutron |
| 1932 | Knoll and Ruska | Electron microscope |
| 1932 | Carl Anderson | Positron from cosmic rays |
| 1932 | Cockroft and Walton | Linear proton accelerators to 700 keV and verification of mass/energy equivalence |
| 1932 | Karl Jansky | First radio astronomy |
| 1932 | Dmitri Iwanenko | Neutron as a constituent of nucleus |
| 1932 | Richard Tolman | Thermodynamics of oscillating cyclic universe |
| 1932 | Vladimir Fock | Fock space |
| 1932 | Urey, Brickwedde, Murphy, Washburn | Deuterium |
| 1932 | Werner Heisenberg | Nucleus is composed of protons and neutrons |
| 1933 | Lev Davidovich Landau | Proposed existence of neutron stars |
| 1933 | Paul Ehrenfest | Theory of second order phase transitions |
| 1933 | Blackett and Occhialini | Electron-positron creation and annihilation |
| 1933 | Esterman, Frisch, Stern | Measurement of proton magnetic moment |
| 1933 | Baade and Zwicky | Collapse of a white dwarf may set off a supernova and leave a neutron star |
| 1933 | Fritz Zwicky | Dark matter in galactic clusters |
| 1933 | Arthur Milne | Cosmological principle of large scale homogeneity |
| 1933 | Harlow Shapley | Observation of structure in galaxy distribution |
| 1934 | Pavel Cherenkov | Cherenkov radiation |
| 1934 | Chadwick & Goldhaber | Precise measurement of neutron mass |
| 1934 | Chadwick & Goldhaber | Measurement of nuclear force |
| 1934 | Francis Perrin | Neutrino is massless |
| 1934 | Grote Reber | Discrete radio source in Cygnus |
| 1934 | Joliot and Curie | Induced radioactivity |
| 1934 | Enrico Fermi | Fermi theory of weak interaction and beta decay |
| 1934 | Esterman and Stern | Magnetic moment of neutron |
| 1934 | Fermi and Hahn | Fission observed |
| 1934 | Paul Dirac | Polarisation of the vacuum and more divergence in QED |
| 1935 | Yukawa, Stueckelberg | Theory of strong nuclear force and the pi-meson |
| 1935 | J. Robert Oppenheimer | Spin statistics |
| 1935 | Enrico Fermi | Hypothesis of transuranic elements |
| 1935 | Robertson, Walker | Most general homogenious isotropic universe |
| 1935 | Einstein, Podolsky, Rosen | EPR Paradox of non-locality in quantum mechanics |
| 1935 | Subrahmanyan Chandrasekhar | Calculation of mass limit for stellar collapse of a white dwarf star |
| 1935 | Erwin Schroedinger | Quantum cat paradox |
| 1935 | Robert Watson-Watt | Radar |
| 1935 | Niels Bohr | Compound nucleus |
| 1935 | Anderson and Neddermeyer | Muon in cosmic rays |
| 1935 | Leon Brillouin | Theory of wave guides |
| 1936 | Breit and Coll | Isotopic spin |
| 1936 | Alan Turing | Computability |
| 1937 | Pyotr Kapitza | Superfluidity of helium II |
| 1937 | Perrier and Segre | Element 37, technetium, first element made artifically |
| 1937 | Majorana | Symmetric theory of electron and positron |
| 1937 | Julian Schwinger | Neutron spin is half |
| 1937 | Blau, Wambacher | Photographic emulsion as particle detector |
| 1937 | Bloch and Nordsieck | Operator normal ordering |
| 1937 | John Wheeler | S-matrix theory |
| 1938 | Oppenheimer & Serber | There is an upper mass limit for stability of neutron stars |
| 1938 | Bethe, Critchfield, von Weizsacker | Stars are powered by nuclear fusion CN-cycle |
| 1938 | Isador Rabi | Magnetic Resonance |
| 1938 | Hahn, Strassman | Fission induced with neutrons |
| 1938 | Oskar Klein | New field equations from higher dimensional Kaluza-Klein theory |
| 1938 | Fritz Zwicky | Clusters of galaxies |
| 1938 | Ernest Stueckelberg | Suggests baryon number conservation |
| 1938 | Hendrick Kramers | Mass renormalisation |
| 1938 | Frisch and Meitner | Theory of uranium fission |
| 1939 | Joliot,Curie-Joliot, Szilard | Theory of nuclear chain reaction |
| 1939 | Oppenheimer & Snyder | A collapsing neutron star will form a black hole |
| 1939 | Bohr, Wheeler, Khariton, Zel’dovich | Theory of U235 fission and chain reaction |
| 1939 | Bloch and Alvarez | Measurement of the neutron magnetic moment |
| 1939 | Rossi, Van Norman, Hilbery | Muon decay |
| 1939 | Teller, Szilard, Einstein | Warning letter to Roosevelt |
| 1939 | Peierls and Frisch | Critical mass and theory of A-Bomb |
| 1939 | Marguerite Perey | Element 87, francium |
| 1940 | MacMillan, Abelson | Element 93, neptunium, first transuranian elements |
| 1940 | Corson, MacKenzie, Segre | Element 85, astatine synthesised |






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