1965 Nobel Prize in Physics

Reason for Award

for their fundamental work in quantum electrodynamics, with deep-ploughing consequences for the physics of elementary particles

Laureates

Shin-ichiro Tomonaga
Shin-ichiro Tomonaga

JapanJapan

Julian Schwinger
Julian Schwinger

United States of AmericaUnited States of America

Richard P. Feynman
Richard P. Feynman

United States of AmericaUnited States of America

Explanation

Electricity can light bulbs and magnets can stick to metal; both phenomena come from the same electromagnetic force. Quantum electrodynamics (QED) is a rulebook that explains this force for objects smaller than atoms, like electrons and photons. Sin-itiro Tomonaga, Julian Schwinger and Richard Feynman completed that rulebook and provided a clear way to do the calculations. Thanks to them we can predict with amazing accuracy how an electron emits or absorbs light. The glowing of fluorescent lamps or TV screens can be described in detail by this theory. QED forms the basis of many modern technologies that rely on electricity and light, such as smartphones and medical lasers.

Related Keywords

quantum electrodynamics

Quantum electrodynamics (QED) is a relativistic field theory based on U(1) gauge symmetry that treats the interaction of charged fermions such as electrons and positrons with photons. The perturbative series converges extremely well, giving agreement between theory and experiment at the 10^−12 level. Scattering amplitudes are calculated systematically with Feynman diagrams and loop corrections are rendered finite by renormalization. The mathematical structure of QED served as the template for gauge theories of the weak and strong interactions. The renormalization-group idea originating in QED now finds applications in critical phenomena and statistical physics.

vacuum polarization

Vacuum polarization is the phenomenon in which an electromagnetic field induces virtual electron–positron pairs, making the vacuum behave like a medium. The effect appears as the photon self-energy and modifies the Coulomb potential at short distances. First formalized by Uehling in the 1930s, it is one of the most important one-loop effects in QED. Vacuum polarization is confirmed through high-precision measurements of the Lamb shift and the electron g-2 and is indispensable for testing theory. It also influences astrophysical problems such as cosmic-microwave-background propagation and birefringence in strong magnetic fields.

electron anomalous magnetic moment

The magnetic moment measures how strongly a particle behaves like a tiny magnet; the Dirac equation predicts g=2. QED loop corrections shift it slightly, giving a_e=(g−2)/2≈0.00116. Schwinger derived the one-loop value α/2π, and subsequent four- and five-loop calculations have reduced the theoretical uncertainty to 10^−13. Experiments using Penning traps measure the value with comparable precision, agreeing with theory to more than 12 digits. This agreement is one of the clearest demonstrations of the validity of quantum field theory.

perturbation theory

Perturbation theory approximates solutions by expanding in a small parameter when interactions are weak. In QED the fine-structure constant α≈1/137 serves as the expansion parameter. Contributions at each order are organized with Feynman diagrams; higher loops are more complex but increase precision. Divergent terms are absorbed through renormalization so that only finite observables remain. Perturbative methods are also widely used in high-energy QCD and in weakly coupled electron gases of solid-state physics.

Feynman diagram

Feynman diagrams graphically depict particle world-lines with arrows and wavy lines, providing a visual representation of scattering processes. By associating rules to each line and vertex, the corresponding mathematical expression can be written down automatically. The topology of a diagram expresses the combinatorial equivalence of physical processes and clarifies symmetry factors in multiparticle amplitudes. Computer algorithms can now generate and evaluate such diagrams automatically, forming the basis of high-loop analyses. The diagrammatic technique developed for QED later spread to all gauge theories and even to string-theory world-sheet diagrams.

renormalization

Renormalization is the procedure of absorbing infinities that arise in calculations into redefined physical observables, yielding finite predictions. Tomonaga, Schwinger and others solved QED’s divergence problem by replacing bare charge and mass with measured values. The technique was refined into systematic algorithms such as the BPHZ method and the MS scheme. The renormalization group describes how theory parameters flow with energy scale, underpinning our understanding of critical phenomena and asymptotic freedom. The concept influences areas outside physics, including economics and the analysis of hierarchical complex systems.

beta function

The beta function is the main term in the renormalization-group equation that gives the rate at which a coupling constant changes with energy scale. In QED β>0, so the coupling grows monotonically at higher energies but remains small over experimentally accessible ranges. This property means the theory is perturbatively controllable in the infrared. In QCD, where the sign is opposite, asymptotic freedom arises, revolutionizing our understanding of the strong force. The beta-function concept is also applied to critical exponents in statistical physics and to fractal-dimension analysis in chaos theory.

Tomonaga-Schwinger equation

The Tomonaga-Schwinger equation is a covariant evolution equation that describes how a quantum-field state changes as a spatial hypersurface is deformed. It generalizes the ordinary Schrödinger equation’s time parameter to an arbitrary three-dimensional surface. This allows consistent descriptions in different reference frames and clarifies local time evolution in field theory. Applications range from the Keldysh formalism of nonequilibrium statistics to quantum fields in curved spacetime. Mathematically it relates to Hamiltonian-density commutation relations in integrable systems and remains an active research topic.

photon

The photon is the quantum of the electromagnetic field, a massless, neutral, spin-1 boson. Exchange of photons mediates Coulomb and magnetic forces between charges. Because photons do not interact with themselves, QED calculations are relatively simple and can achieve very high precision. At high energies, nontrivial processes such as photon–photon scattering and photon-fusion particle production are observed. Understanding photon properties underpins laser technology, quantum communications and a wide range of astronomical observations.

elementary particle

Elementary particles are the smallest units of matter that cannot be subdivided within current theory. In the Standard Model they include six quark flavors, six leptons, gauge bosons and the Higgs particle. Electrons and photons are prime examples, and their interactions are described precisely by QED. Particle physics is closely connected to the early universe and the stability of matter and is tested through accelerator experiments and astronomical observations. Many open questions remain, such as the origin of neutrino masses and the nature of dark matter.