sciencebriefs
13:00in productionCh. 1 · A letter to Pauli/ 13:00 · ceiling 15 min
Physics

Uncertainty principle

1927

Werner Heisenberg's 1927 principle is often mistaken for a statement about clumsy measuring instruments, but it describes a limit built into quantum mechanics itself, one later physicists made more precise rather than ever overturned.

In 1927, working at Niels Bohr's Institute in Copenhagen, Werner Heisenberg formulated the uncertainty principle, first outlined in a February letter to Wolfgang Pauli before formal publication, stating that certain pairs of properties, most famously a particle's position and momentum, cannot both be known to arbitrary precision at once. The effect is not caused by measurement disturbing a particle but reflects a mathematical property of quantum systems themselves, tied to the fixed lower bound on how precisely position and momentum can jointly be defined. Earle Hesse Kennard derived the precise inequality that same year, and Howard Percy Robertson and Erwin Schrödinger generalised it further by 1929 and 1930 into more complete mathematical forms, refining rather than challenging Heisenberg's original claim. Heisenberg received the 1932 Nobel Prize in Physics for his broader work founding quantum mechanics, and later joined Germany's wartime nuclear research programme, with declassified 1992 records suggesting his actual progress toward a weapon had been limited.

Chapters & takeaways6
  1. 0:08
    A letter to Pauli

    Heisenberg first described the principle privately before publishing it in 1927.

  2. 2:10
    Not a measurement problem

    The limit is built into quantum systems, not caused by clumsy observation.

  3. 4:20
    Position and momentum, tied together

    A fixed lower bound links how precisely each quantity can be known.

  4. 6:30
    Refined by other physicists

    Kennard, Robertson and Schrödinger generalised the relation over the following years.

  5. 8:40
    A Nobel, then a wartime programme

    Recognition in 1932 preceded a far more complicated later chapter of his life.

  6. 10:50
    Is it worth your time

    A fundamental physical limit paired with an unusually complicated biography.

Worth your time?

Yes. Study the whole thing.

4.5/ 5
What works
  • the core claim has never been overturned, only generalised into more precise mathematical form
  • the distinction between a fundamental limit and a measurement artifact is well established
  • the historical sequence of refinements from Kennard through Schrödinger is clearly documented
What does not
  • the popular observer-effect explanation of the principle is a common but inaccurate simplification
  • declassified wartime records leave real ambiguity about how far Heisenberg's weapons work actually progressed
Study it if
  • anyone who wants to understand what the uncertainty principle actually claims, not the popular myth
  • readers interested in how a foundational idea gets refined mathematically over successive years
  • people curious about Heisenberg's more complicated wartime history
Skip it if
  • readers wanting the full mathematics of the Robertson-Schrödinger relation worked through
  • anyone looking for a definitive verdict on Heisenberg's wartime conduct
The written brief3 min read

A letter to Pauli

In 1927, working at Niels Bohr’s Institute of Theoretical Physics in Copenhagen, Werner Heisenberg formulated what became known as the uncertainty principle, first setting the idea out in a letter to the physicist Wolfgang Pauli on 23 February 1927 before publishing it formally. In his own paper he used the German word Ungenauigkeit, meaning imprecision, rather than the English term uncertainty that later became standard. The claim itself was specific: certain pairs of physical properties, most famously a particle’s position and its momentum, cannot both be known to arbitrary precision at the same time, and the more precisely one is pinned down, the less precisely the other can be.

Not a measurement problem

The principle is often misunderstood as a statement about the limits of measuring instruments, the idea that observing a particle inevitably disturbs it, but that is not what it actually describes. It reflects an intrinsic property of quantum systems themselves, independent of any particular measuring apparatus: position and momentum are represented mathematically as operators that do not commute with each other, meaning the order in which they are applied changes the result, and that non-commuting relationship alone guarantees no quantum state can simultaneously be an exact position state and an exact momentum state, regardless of how careful or non-invasive any hypothetical measurement might be.

Position and momentum, tied together

The relationship can be expressed as a lower bound: the product of the uncertainty in a particle’s position and the uncertainty in its momentum can never fall below a fixed value tied to the reduced Planck constant, roughly half of that constant. The same kind of relationship appears between other paired quantities, generally called complementary or canonically conjugate variables, including energy and time, and the different components of angular momentum, though position and momentum remain the version most commonly cited and taught, and the one Heisenberg himself originally worked through in his 1927 paper.

Refined by other physicists

Heisenberg’s original argument was refined mathematically by others rather than challenged. Earle Hesse Kennard derived the precise inequality relating the standard deviations of position and momentum that same year, 1927, and Hermann Weyl extended related formulations in 1928. Howard Percy Robertson generalised the relationship in 1929 to apply to any pair of quantities represented by Hermitian operators, not just position and momentum specifically, and Erwin Schrödinger refined that further in 1930 into what is now called the Robertson-Schrödinger relation, accounting for correlations the earlier version had not captured. None of these refinements overturned Heisenberg’s basic claim; they made it more general and mathematically precise.

A Nobel, then a wartime programme

The effect is meaningful only at quantum scales and becomes negligible for ordinary macroscopic objects, which is why nothing in everyday experience hints at it directly. Certain quantum states come as close as mathematically possible to the theoretical minimum uncertainty allowed, including the ground state of a quantum harmonic oscillator and so-called coherent states, while other states sit somewhat above that minimum. Heisenberg received the 1932 Nobel Prize in Physics for his broader creation of quantum mechanics, though the announcement was delayed until November 1933. He later joined Germany’s wartime nuclear research programme from September 1939 and was appointed director of the Kaiser Wilhelm Institute for Physics in 1942, and declassified recordings from his wartime detention, released only in 1992, indicated he had not worked out the critical mass needed for a bomb before learning of the Hiroshima attack.

Is it worth your time

This is worth an hour both for the physics itself, a genuinely fundamental limit rather than a shortcoming of instruments, refined into increasingly general mathematical form by several physicists across the following years rather than settled all at once, and for the more complicated later chapter of Heisenberg’s own life. The same mind that formalised the deepest limits of what can be known about a particle spent the Second World War inside a weapons programme whose actual progress historians are still working to understand fully, from records only released decades afterward.

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Planck postulateMax Planck's law for how a heated body radiates energy across different frequencies matched experiment only if he assumed that oscillators emit energy in discrete units proportional to frequency, E equals h times frequency. Planck treated this as a mathematical convenience rather than a claim about nature, and it took Einstein's 1905 explanation of the photoelectric effect, which Planck himself resisted, to turn the assumption into a physical idea taken seriously by other physicists.
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Compton scattering1922Working at Washington University in St Louis, Arthur Compton discovered in 1922 that X-rays scattered off free electrons emerged with a longer wavelength than the incoming beam, a shift that depended only on the scattering angle and not on the beam's intensity, contrary to what a purely wave-based theory of light predicted. Published in 1923, the result made sense only if each X-ray behaved as a discrete photon carrying momentum, colliding with an electron much as one particle strikes another. The interpretation was fiercely contested when first presented, but no wave-only alternative survived scrutiny, and the finding became one of the key pieces of evidence, alongside the photoelectric effect, for the quantum picture of light. Compton shared the 1927 Nobel Prize in Physics with C. T. R. Wilson, and went on to oversee the Manhattan Project laboratory where the first nuclear reactor achieved criticality in 1942.
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Hawking radiationBuilding on Jacob Bekenstein's 1972 proposal that black holes carry entropy proportional to the area of their event horizon, Stephen Hawking applied quantum field theory to the physics near that horizon and showed in 1974 and 1975 that black holes should emit thermal radiation and slowly lose mass over time, a result known as Hawking radiation. The predicted temperature is inversely proportional to a black hole's mass, so a stellar-mass black hole would sit far colder than the cosmic microwave background surrounding it, meaning such black holes currently absorb more energy from that background than they emit and are not actually shrinking, while only much smaller, hypothetical primordial black holes could have evaporated within the age of the universe. No direct astronomical detection of Hawking radiation has been made, though physicists have built laboratory analogue systems, using sound waves in fluids or light in optical media, that reproduce a mathematically similar effect. The theory also creates the black hole information paradox, since radiation calculated to be effectively random appears to erase information about whatever originally fell into the black hole, an apparent conflict with quantum mechanics that remains an open problem in theoretical physics.
13:00
Photoelectric effectThe photoelectric effect, in which light striking certain materials ejects electrons from their surface, produced three observations wave theory could not explain: emission only above a threshold frequency regardless of intensity, near-instantaneous emission once above it, and ejected electrons whose energy depended on frequency rather than intensity. In 1905, one of four papers from his miracle year, Einstein proposed that light delivers its energy in discrete packets, photons, each proportional to frequency, from which followed a simple equation for the electrons' maximum energy that explained all three puzzles at once. Robert Millikan verified the theory experimentally in 1914 through precise measurements, despite his own reported doubts about treating light as particles. Einstein received the 1921 Nobel Prize in Physics specifically for this work rather than for relativity, though the citation itself stopped short of endorsing the particle theory of light outright, full acceptance only arriving after Satyendra Nath Bose's 1924 theoretical work.
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