
Physics
- 186
- briefs
- 11:17
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- 2098 min
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- 84
- researchers


First observation of gravitational waves

Nuclear fusion

Avicenna

Klaus von Klitzing

Per Bak

Nicolas Léonard Sadi Carnot

Space

Lord Kelvin

Abdus Salam

Albert Einstein

Positron

André-Marie Ampère

Arthur Ashkin

Aryabhata

Bell test

Bell's theorem

Benoit Mandelbrot

Bernhard Riemann

Stellar nucleosynthesis

Bhāskara II

Boltzmann's entropy formula

Brahmagupta

Brownian motion

Carnot heat engine

Cassini–Huygens

Cavendish experiment

Chicago Pile-1
Chicago Pile-1 proved a self-sustaining nuclear chain reaction was possible using natural uranium and purified graphite — nothing more, nothing less.

Christiaan Huygens

Compton scattering

Cosmic inflation

David Gross

David Hilbert

Matter wave

Dirac equation
The Dirac equation is the first consistent relativistic quantum wave equation. It predicts antimatter and derives spin — verified by hydrogen fine structure and Anderson’s 1932 positron detection. It does not prove antimatter; it implies it. It does not go beyond first-order fine structure. It remains indispensable in particle physics.

Eddington experiment

General relativity

Photoelectric effect

Special relativity

Galvanic cell

Photoemission spectroscopy

Emmy Noether

Enrico Fermi

Ernst Mach

Erwin Schrödinger

Eunice Newton Foote

Évariste Galois

Felix Klein

Fermat's Last Theorem
Wiles proved Fermat’s Last Theorem by establishing the modularity theorem for semistable elliptic curves — a result that, combined with Ribet’s theorem, ruled out integer solutions to a^n + b^n = c^n for n > 2. His initial 1993 proof contained a flaw in the Selmer group argument; he and Taylor repaired it in 1994 using Galois representations and Iwasawa theory. The complete proof appeared in the Annals of Mathematics in 1995.

Ferromagnetism

Fick's laws of diffusion
Fick’s laws quantify diffusion in fluids using direct measurements of salt flux and concentration. They hold for liquids, not solids. Their derivation is experimental, their form exact, and their reach vast — but they are not universal, not theoretical first principles, and not extended beyond their empirical domain.

Frank Wilczek

Kite experiment

Galileo Galilei

Georg Cantor

Georg Ohm

Georges Lemaître

Gödel's incompleteness theorems
Gödel’s 1931 incompleteness theorems show that no consistent, effectively axiomatized formal system capable of arithmetic can be both complete and self-consistent. They ended Hilbert’s program. Their method — Gödel numbering and diagonalisation — became foundational for computability theory. They do not apply outside formal systems satisfying strict technical conditions.

Graphene

Guglielmo Marconi

Hans Christian Ørsted

Hawking radiation

Uncertainty principle

Henri Poincaré

Henrietta Swan Leavitt

Hilbert's problems
Hilbert’s problems are not a discovery in the empirical sense. They are a curatorial act—23 unsolved questions published in 1900 to define mathematics’ trajectory for the next century. Their influence stems from uptake, not truth. They succeeded because mathematicians treated them as a syllabus—not because they were complete, precise or even consistent.

Hubble's law

Hugh David Politzer

IceCube Neutrino Observatory

Ilya Prigogine

Entropy (information theory)
Shannon’s 1948 theory redefined communication as a mathematical problem of uncertainty reduction. He proved entropy is the irreducible cost of lossless encoding — not a metaphor, not a heuristic, but a bound. It applies only where messages are statistically structured, and only to syntactic information — never semantics. Its power lies in its narrowness.

Isaac Newton

Isotope

James Clerk Maxwell

James Prescott Joule

Jing Fang

Jocelyn Bell Burnell

Johannes Kepler

John Tyndall

John von Neumann

John William Strutt, 3rd Baron Rayleigh

Josef Stefan

Joseph Henry

Joseph-Louis Lagrange

Kamioka Observatory

Kinetic theory of gases
Bernoulli’s 1738 kinetic theory is the first mechanistic explanation of gas behaviour. It correctly identifies pressure as momentum transfer and temperature as mean kinetic energy. It derives Boyle’s law from molecular motion. It fails to resolve energy conservation or collision elasticity — gaps that stalled acceptance for a century. Its value lies not in immediate utility but in framing matter as particulate and dynamic — a conceptual pivot that enabled thermodynamics and statistical mechanics.

Kirchhoff's circuit laws
Kirchhoff’s 1845 circuit laws are two experimentally derived equalities — one for current at junctions, one for voltage around loops — valid only under strict physical assumptions of the lumped-element model.

Knot theory

Kurt Gödel

Lise Meitner

Liu Hui

Lorentz transformation
Lorentz’s transformations were a technically successful but conceptually constrained response to experimental anomalies in electrodynamics. They preserved the aether while making predictions match observation—by introducing local time, length contraction, and time dilation as mathematical corrections. Their algebraic form survived into special relativity, but their physical meaning did not.

Ludwig Boltzmann

Magnetic resonance imaging

Marie Curie

Max Planck

Maxwell's equations

Nuclear fission

Metamaterial

Michael Faraday

Oil drop experiment

Mitchell Feigenbaum

Solar neutrino problem

Niels Bohr

Noether's theorem
Noether's theorem is the rigorous, general proof that continuous symmetries of the action imply conservation laws. It was published in 1918 in Invariante Variationsprobleme. It applies only to smooth, differentiable symmetries in conservative systems. It resolved energy conservation in general relativity. It reshaped theoretical physics’ emphasis toward symmetry.

Ohm's law

Ole Rømer

Oliver Heaviside

Omar Khayyam

Paul Dirac

Pentaquark

Perpetual motion

Pierre-Simon Laplace

Piezoelectricity

Black-body radiation

Planck postulate

Pulsar

Punctuated equilibrium
Punctuated equilibrium is a descriptive claim about fossil patterns — not a mechanism, not a refutation, not a universal law. It says what is seen (stasis), what is rare (gradualism), and where change appears (cladogenesis). Its power lies in its restraint.

Quantum electrodynamics

Quantum tunnelling

Molecular orbital theory

Quantum teleportation

2019 revision of the SI

Richard Feynman

Robert Hooke

J. Robert Oppenheimer

Roger Penrose

Galaxy rotation curve

Rutherford scattering experiments

Seismic wave

Sheldon Glashow

Shor's algorithm
Shor’s algorithm is a quantum algorithm for integer factorisation, developed by Peter Shor in 1994. It runs in polynomial time in log N and places factorisation in BQP. It is asymptotically faster than the general number field sieve.

Sophie Germain

Srinivasa Ramanujan

Stephen Hawking

Steven Weinberg

Superconductivity

High-temperature superconductivity

SN 1987A

Barometer

Caesium standard

Cold fusion

Copernican heliocentrism

Large-scale structure of the universe

Higgs boson

Mpemba effect

X-ray

Electrocardiography

Electron microscope
The electron microscope began not with biology, but with physics: a test of magnetic lensing on engineered grids. Its first success was mechanical and conceptual — not observational.

1883 eruption of Krakatoa

Event Horizon Telescope

Franck–Hertz experiment

Galvanometer

Holographic principle

Hubble Deep Field

Mandelbrot set
Mandelbrot visualised a known mathematical object with unprecedented clarity — making topology legible through computation.

Michelson–Morley experiment

N-ray

National Ignition Facility

Oscilloscope

Pauli exclusion principle
The Pauli exclusion principle is not a force or interaction. It is a constraint on how quantum states may be occupied. It arose from spectral anomalies, not theory-first deduction. Its power lies in its austerity: four numbers, one electron, and a sign flip upon exchange. It remains indispensable — and unexplained at root.

Quantum Zeno effect

Riemann hypothesis
Riemann’s 1859 hypothesis is a precise, unproven claim about zeta zeros — central to prime distribution, yet untouched by proof for 165 years.

Scanning tunneling microscope

International System of Units

Optical spectrometer

Standard Model

Stern–Gerlach experiment

Wow! signal

First law of thermodynamics

Topological insulator

Van der Waals equation
Van der Waals’s 1873 equation was the first thermodynamic model to treat fluids as composed of real molecules — with finite size and mutual attraction — and it successfully described both liquid and gas phases, predicted critical-point behaviour, and yielded quantitative estimates of molecular size and attraction strength. It did not prove molecular existence, nor does it hold across all conditions. Its value lies in making molecular assumptions productive — long before they were directly observable.

Vera Rubin

Vladimir K. Zworykin

Wendy Freedman

Werner Heisenberg

William Herschel

X-ray crystallography
The Braggs established X-ray crystallography as a quantitative physical method by linking diffraction geometry to atomic spacing — using simple crystals, mechanical rotation, film detection, and arithmetic. They did not image atoms. They inferred lattice periodicity. Their work is durable, narrow, and strictly instrumental.

Zu Chongzhi

Mass–energy equivalence
Einstein’s 1905 derivation unified mass and energy conceptually — not empirically. It replaced two conservation laws with one. It did not predict applications. It did not contain E = mc² as written. Its power lies in logical necessity, not experimental novelty.

Schrödinger's cat
Schrödinger's cat is a 1935 thought experiment designed by Erwin Schrödinger in correspondence with Einstein to critique the Copenhagen interpretation of quantum mechanics. It uses a sealed chamber containing a cat, radioactive source, Geiger counter, relay, hammer, and flask of hydrocyanic acid. The setup links a single quantum event — atomic decay — to a macroscopic outcome. Mathematically, the wave function describes a superposition of 'alive' and 'dead', yet observation always reveals one definite state. Schrödinger intended this as reductio ad absurdum, not as a proposal. No experiment was conducted. The work establishes a tension between formalism and observation — nothing more.

String theory

Accelerating expansion of the universe
The 1998 supernova measurements established cosmic acceleration via distance–redshift mismatch — not theory, not analogy, but empirical inference from standard candles. It overturned the assumption of gravitational deceleration. It did not identify dark energy. It did not prove Λ. It remains the strongest direct evidence for accelerated expansion — and the clearest signal of our ignorance about 70% of reality.

Discovery of cosmic microwave background radiation
Penzias and Wilson discovered a 3.5 K isotropic microwave background in 1964 using the Holmdel Horn Antenna at Bell Labs. They eliminated local interference — including pigeon droppings — and confirmed the signal originated outside the Milky Way. Its match to Dicke’s prediction prompted interpretation as the Big Bang’s remnant. But the work itself claimed only a persistent, unexplained antenna temperature — not cosmology.

Double-slit experiment
Young’s 1801 double-slit experiment established wave behaviour for visible light. Later versions with electrons (1927) extended it to matter. The interference pattern is real. The disappearance of that pattern upon path detection is real. But Young did not observe particles, nor did he claim duality — he argued for waves only. Duality emerged from later experiments combining his method with quantum detection.
