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The history of quantum mechanics traces the development of the physical theory describing matter and energy at atomic and subatomic scales. Beginning with Max Planck's quantization of energy in 1900, it evolved through contributions from Einstein, Bohr, Heisenberg, Schrödinger, Dirac, and others into one of the most successful and revolutionary theories in science. More Less
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1801
The resulting Huygens–Fresnel principle was extremely successful at reproducing light's behaviour and was consistent with Thomas Young's discovery of wave interference of light by his double-slit experiment in 1801, strengthening the wave view of light.
Image source: Huygens–Fresnel principle
1803 - 1860
During the early 19th century, chemical research by John Dalton and Amedeo Avogadro lent weight to the atomic theory of matter, an idea that James Clerk Maxwell, Ludwig Boltzmann and others built upon to establish the kinetic theory of gases.
Image source: Atomic theory
1850
The wave view did not immediately displace the ray and particle view, but began to dominate scientific thinking about light in the mid 19th century, since it could explain polarization phenomena that the alternatives could not.
Image source: History of quantum mechanics
1877
Ludwig Boltzmann suggested in 1877 that the energy levels of a physical system, such as a molecule, could be discrete (rather than continuous), an early hint of quantization that would later underpin quantum mechanics.
Image source: Ludwig Boltzmann
1885
By the end of the nineteenth century, a simple rule known as Balmer's formula showed how the frequencies of the different spectral lines of hydrogen related to each other, though without explaining why this was, or making any prediction about the intensities.
Image source: Balmer series
1904
By 1904 Thomson proposed the first atomic model with subatomic constituents, using circulating electrons in a background of positive charge, the so-called plum pudding model. Thomson's concepts were supported by early beta particle scattering experiments.
Image source: Plum pudding model
1911
By 1911 Hans Geiger and his student Ernest Marsden demonstrated backscattering of alpha particles which Ernest Rutherford interpreted as compelling evidence that the positive charge was concentrated in a small volume we now call the nucleus. This led to the planetary model of the atom (1911), though Rutherford's discovery did not immediately cause atomic models to be revised.
Image source: Rutherford scattering experiments
1850 - 1900
The study of black-body radiation between 1850 and 1900 could not be explained without quantum concepts. By the late 19th century, thermal radiation had been fairly well characterized experimentally, but classical physics failed to account for its spectrum.
Image source: Black-body radiation
1887
In 1887, Heinrich Hertz observed that when light with sufficient frequency hits a metallic surface, the surface emits cathode rays. This photoelectric effect would later become one of the key pieces of evidence for the quantum nature of light.
Image source: Photoelectric effect
1900
The first model that was able to explain the full spectrum of thermal radiation was put forward by Max Planck in 1900. Planck's law was the first quantum theory in physics, and Planck won the 1918 Nobel Prize in Physics 'in recognition of the services he rendered to the advancement of Physics by his discovery of energy quanta'. This marked the beginning of the old quantum theory era.
1902
In 1902, Philipp Lenard discovered that the maximum possible energy of an ejected electron is unrelated to the intensity of the monochromatic light, a puzzling result that classical wave theory could not explain.
Image source: Philipp Lenard
1905
In 1905, Albert Einstein suggested that even though continuous models of light worked extremely well for time-averaged optical phenomena, for instantaneous transitions the energy in light may occur a finite number of energy quanta. Einstein explained the photoelectric effect using the concept of photons, particles of light with quantized energy. This has been called the most 'revolutionary' sentence written by a twentieth century physicist. Einstein was awarded the 1921 Nobel Prize in Physics for this discovery.
1911 - 1913
The application of Planck's quantum theory to the electron allowed Ștefan Procopiu in 1911–1913, and subsequently Niels Bohr in 1913, to calculate the magnetic moment of the electron, which was later called the 'magneton'; similar quantum computations were subsequently made possible for both the magnetic moments of the proton and the neutron.
1913
Niels Bohr applied quantum ideas to Rutherford's nuclear atom, producing a model that explained the hydrogen emission spectrum. Bohr was awarded the 1922 Nobel Prize in Physics 'for his services in the investigation of the structure of atoms and of the radiation emanating from them'. These theories, though successful, were strictly phenomenological: during this time, there was no rigorous justification for quantization, aside, perhaps, from Henri Poincaré's discussion of Planck's theory in his 1912 paper Sur la théorie des quanta.
Image source: Bohr model
1922
In 1922, Otto Stern and Walther Gerlach set out to test the theory of space quantization, sending silver atoms through an inhomogeneous magnetic field and observing discrete deflections, providing direct evidence of quantized angular momentum.
Image source: Stern–Gerlach experiment
1924
In 1924, Louis de Broglie published a breakthrough hypothesis: matter has wave properties. De Broglie was awarded the Nobel Prize in Physics in 1929 for his hypothesis; Thomson and Davisson shared the Nobel Prize for Physics in 1937 for their experimental work confirming it.
Image source: Matter wave
1925
In 1925, Werner Heisenberg attempted to solve one of the problems that the Bohr model left unanswered, explaining the intensities of the different lines in the hydrogen emission spectrum. His approach developed into matrix mechanics, the first complete formulation of quantum mechanics.
1925
In 1925, Ralph Kronig proposed that electrons behave as if they self-rotate, or 'spin', about an axis, an idea that helped explain fine structure in atomic spectra and became a fundamental property of quantum particles.
Image source: Spin (physics)
Sep 1925
Pascual Jordan's September 1925 paper 'Zur Quantenmechanik' was a key contribution to the development of matrix mechanics, helping formalize Heisenberg's ideas into rigorous mathematics together with Born and Heisenberg.
Image source: Pascual Jordan
Jan 1926 - Jun 1926
Building on the technology developed in classical mechanics, the invention of wave mechanics by Erwin Schrödinger and expansion by many others triggers the 'modern' era beginning around 1925. In the first half of 1926, building on de Broglie's hypothesis, Erwin Schrödinger developed the equation that describes the behavior of a quantum-mechanical wave.
Image source: Schrödinger equation
1926
The term 'photon' was introduced in 1926 by Gilbert N. Lewis, giving a name to Einstein's light quantum and cementing the particle picture of electromagnetic radiation alongside its wave description.
May 1926
In May 1926, Schrödinger proved that Heisenberg's matrix mechanics and his own wave mechanics made the same predictions about the properties and behavior of the electron; mathematically, the two theories had an underlying common form.
1927
Heisenberg formulated an early version of the uncertainty principle in 1927, analyzing a thought experiment where one attempts to measure an electron's position and momentum simultaneously, establishing fundamental limits on measurement in quantum mechanics.
Image source: Uncertainty principle
1927
Arthur Compton won the 1927 Nobel Prize in Physics for his discovery of the Compton effect, the scattering of X-rays by electrons that provided strong evidence for the particle nature of light.
Image source: Arthur Compton
1927
The field of quantum chemistry was pioneered by physicists Walter Heitler and Fritz London, who published a study of the covalent bond of the hydrogen molecule in 1927, applying quantum mechanics to chemical bonding for the first time.
Image source: Quantum chemistry
1945
Pauli received the 1945 Nobel Prize in Physics for his 'decisive contribution through his discovery of a new law of Nature, the exclusion principle or Pauli principle', which explains the structure of atoms and the periodic table.
Image source: Wolfgang Pauli
1927
Starting around 1927, Paul Dirac began the process of unifying quantum mechanics with special relativity by proposing the Dirac equation for the electron, which predicted the existence of antimatter and naturally incorporated electron spin.
1930
Paul Dirac also pioneered the use of operator theory, including the influential bra–ket notation, as described in his famous 1930 textbook, which became a foundational reference for generations of physicists.
Image source: The Principles of Quantum Mechanics
1947
The Lamb–Retherford experiment discovered the Lamb shift in 1947, a small difference in energy between certain hydrogen levels that contradicted the Dirac equation's predictions and led to the development of quantum electrodynamics.
Image source: Lamb shift
1975
The theory of quantum chromodynamics as we know it today was formulated by Hugh David Politzer, David Gross and Frank Wilczek in 1975, describing the strong interaction between quarks and gluons through asymptotic freedom.
Image source: Quantum chromodynamics
1979
Building on pioneering work by Schwinger, Peter Higgs and Jeffrey Goldstone, the physicists Sheldon Glashow, Steven Weinberg and Abdus Salam independently showed how the weak nuclear force and quantum electrodynamics could be merged into a single electroweak force, for which they received the 1979 Nobel Prize in Physics.
1980
The quantum Hall effect, discovered in 1980 by Klaus von Klitzing, revealed quantized electrical conductance in two-dimensional electron systems and opened new fields of research in condensed matter physics.
Image source: Quantum Hall effect
1984 - 1994
Quantum information science developed in the latter decades of the 20th century, beginning with theoretical results like Holevo's theorem, the concept of generalized measurements or POVMs, the proposal of quantum key distribution by Bennett and Brassard in 1984, and Shor's algorithm in 1994.
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