| Dates | Characters | Theories and discoveries |
| 1900 | Lord Rayleigh | Statistical derivation of short wavelength black body law |
| 1900 | Ernest Rutherford | First determination of a radioactive half-life |
| 1900 | Antoine Henri Becquerel | Suggests that beta rays are electrons |
| 1900 | Lummer, Pringsheim, Rubens, Kurlbaum | Failure of Wien’s black body law at short wavelengths |
| 1900 | Max Planck | Light quanta in black body radiation, Planck’s black body law & constant |
| 1900 | Paul Villard | Gamma rays |
| 1900 | Friedrich Dorn | Element 86, radon |
| 1900 | Pyotr Lebedev | Radiation pressure measured |
| 1901 | Max Planck | Determination of Planck’s constant, Boltzmann’s constant, Avogadro’s number and the charge on electron |
| 1901 | Guglielmo Marconi | Transmission of Morse signals across the Atlantic |
| 1902 | Philipp Lenard | Intensity law in photoelectric effect |
| 1902 | Rutherford and Soddy | Theory of transmutation by radiation and first use of the term “atomic energy” |
| 1902 | Kelvin, Thomson | Plum pudding model of the atom |
| 1903 | Ernest Rutherford | Alpha particles have a positive charge |
| 1903 | Curie and Laborde | Radioactive energy released by radium is large |
| 1903 | Johannes Stark | The power of the sun may be due to genesis of chemical elements |
| 1903 | Philipp Lenard | Model of atom as two separated opposite charges |
| 1904 | Albert Einstein | Energy-frequency relation of light quanta |
| 1904 | Hendrik Lorentz | The completed Lorentz transformations |
| 1904 | Hantaro Nagaoka | Planetary model of the atom |
| 1904 | Ambrose Flemming | Diode valve and rectifier |
| 1904 | Henri Poincare | Conjectured light speed as physical limit |
| 1904 | Ernest Rutherford | Age of Earth by radioactvity dating |
| 1905 | Albert Einstein | Explains Brownian motion by kinetic theory |
| 1905 | Albert Einstein | Light-quantum theory for photoelectric law |
| 1905 | Albert Einstein | Special relativity |
| 1905 | Paul Langevin | Atomic theory of paramagnetism |
| 1905 | Percival Lowell | Postulates a ninth planet beyond Neptune |
| 1905 | Bragg and Kleeman | Alpha-particles have discrete energies |
| 1905 | Hermann Nernst | Third law of thermodynamics |
| 1905 | Albert Einstein | Equivalence of mass and energy |
| 1906 | Albert Einstein | Quantum explanation of specific heat laws for solids |
| 1906 | Joseph Thomson | Thomson scattering of X-ray photons and number of electrons in an atom |
| 1906 | Ernest Rutherford | Alpha particles scatter in air |
| 1906 | Lee de Forest | Triode valve |
| 1907 | Albert Einstein | Equivalence principle and gravitational redshift |
| 1907 | Urbain & von Welsbach | Element 71, lutetium |
| 1908 | Hermann Minkowski | geometric unification of space and time |
| 1908 | Hans Geiger | Geiger counter for detecting radioactivity |
| 1908 | Heike Kammerlingh-Onnes | Liquid helium |
| 1908 | Geiger, Royds, Rutherford | Identify alpha particles as helium nuclei |
| 1909 | Albert Einstein | Particle-wave duality of photons |
| 1909 | Johannes Stark | Momentum of photons |
| 1909 | Geiger and Marsden | Anomolous scattering of alpha particles on gold foil |
| 1909 | Robert Millikan | Measured the charge on the electron |
| 1910 | Albert Einstein | Why the sky is blue |
| 1910 | Matthew Hunter | Isolation of element titanium |
| 1910 | Theodor Wulf | Excess atmospheric radiation |
| 1911 | Victor Hess | High altitude radiation from space |
| 1911 | Heike Kammerlingh-Onnes | Superconductivity |
| 1911 | Ernest Rutherford | Infers the nucleus from the alpha scattering result |
| 1912 | Joseph Thomson | Mass spectrometry and separation of isotopes |
| 1912 | Henrietta Leavitt | Period to luminosity relationship for Cepheid variable stars |
| 1912 | Robert Millikan | Measurement of Planck’s constant |
| 1912 | Peter Debye | Derivation of specific heat laws to low temperatures |
| 1912 | Charles Wilson | Cloud chamber |
| 1912 | Max Von Laue | X-rays are explained as electromagnetic radiation by diffraction |
| 1912 | Albert Einstein | Curvature of space-time |
| 1912 | Vesto Melvin Slipher | Observes blue-shift of andromeda galaxy |
| 1912 | Gustav Mie | Non-linear field theories |
| 1913 | Niels Bohr | Quantum theory of atomic orbits |
| 1913 | Niels Bohr | Radioactivity as nuclear property |
| 1913 | Jean-Baptiste Perrin | Theory of size of atoms and molecules |
| 1913 | Fajans and Gohring | Element 91, protactinium |
| 1913 | Bragg and Bragg | X-ray diffraction and crystal structure |
| 1913 | Hans Geiger | Relation of atomic number to nuclear charge |
| 1913 | Johannes Stark, | Splitting of hydrogen spectral lines in electric field |
| 1913 | Frederick Soddy | The term “isotope” |
| 1914 | James Chadwick | Primary beta spectrum is continuous and shows an energy anomaly |
| 1914 | Harry Moseley | Used X-rays to confirm the correspondence between electric charge of nucleus and atomic number |
| 1914 | Ejnar Hertzsprung | Measured distance to Large Magellanic Cloud using Cepheid variable stars |
| 1914 | Rutherford, da Costa Andrade | Gamma rays identified as hard photons |
| 1915 | Albert Einstein | General relativity |
| 1915 | David Hilbert | Action principle for gravitational field equations |
| 1915 | Albert Einstein | Prediction of light bending and explanation for perihelion shift of mercury |
| 1916 | Robert Millikan | Verification of energy law in photoelectric effect |
| 1916 | Albert Einstein | Prediction of gravitational waves |
| 1916 | Albert Einstein | Conservation of energy-momentum in general relativity |
| 1916 | Karl Schwarzschild | Singular static solution of gravitational field equations which describes a minimal black hole |
| 1916 | Arnold Sommerfeld | Further atomic quantum numbers and fine structure of spectra, fine structure constant |
| 1917 | Harlow Shapley | Estimates the diameter of the galaxy as 100000 parsecs |
| 1917 | Albert Einstein | Introduction of the cosmological constant and a steady state model of the universe |
| 1917 | Vesto Melvin Slipher | Observes that most galaxies have red-shifts |
| 1917 | Albert Einstein | Theory of stimulated emission and loss of determinism |
| 1917 | Willem de Sitter | Describes a model of a static universe with no matter |
| 1917 | Arthur Eddington | Gravitational energy is insufficient to account for the energy output of stars |
| 1917 | Rutherford, Marsden | Artificial transmutation, hydrogen and oxygen from nitrogen |
| 1918 | Harlow Shapley | Measured distance to globular clusters using Cepheid variable stars |
| 1918 | Harlow Shapley | Determined the size and shape of our galaxy |
| 1918 | Reissner and Nordstrom | Solution of Einstein’s equations which describe a charged black hole |
| 1918 | Emmy Noether | The mathematical relationships between symmetry and conservation laws in classical physics |
| 1918 | Francis Aston | Mass spectrometer |
| 1918 | Herman Weyl | Guage theory |
| 1919 | Ernest Rutherford | Existence of the proton in nucleus |
| 1919 | Oliver Lodge | Prediction of gravitational lensing |
| 1919 | Francis Aston | Hydrogen fusion to helium will release a lot of energy |
| 1919 | Crommelin Eddington | Verification of Einstein’s prediction of starlight deflection during an eclipse |
| 1919 | Arthur Eddington | Predicts the size of red gaints using stellar models |
| 1920 | Ernest Rutherford | Prediction of neutron |
| 1920 | Anderson, Michelson | Pease, size of star Betelgeuse using stellar interferometry |
| 1920 | Harkins, Eddington | Fusion of hydrogen could be the energy source of stars |
| 1920 | Shapley and Curtis | The Great Debate over the scale and structure of the universe |






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